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  • Astrophysics  (3,736)
  • Topographic effects
  • 2020-2022  (4)
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  • 1
    Publication Date: 2022-05-25
    Description: Author Posting. © American Meteorological Society, 2010. This article is posted here by permission of American Meteorological Society for personal use, not for redistribution. The definitive version was published in Journal of Physical Oceanography 40 (2010): 1075-1086, doi:10.1175/2009JPO4375.1.
    Description: A quasigeostrophic, two-layer model is used to study the baroclinic circulation around a thin, meridionally elongated island. The flow is driven by either buoyancy forcing or wind stress, each of whose structure would produce an antisymmetric double-gyre flow. The ocean bottom is flat. When the island partially straddles the intergyre boundary, fluid from one gyre is forced to flow into the other. The amount of the intergyre flow depends on the island constant, that is, the value of the geostrophic streamfunction on the island in each layer. That constant is calculated in a manner similar to earlier studies and is determined by the average, along the meridional length of the island, of the interior Sverdrup solution just to the east of the island. Explicit solutions are given for both buoyancy and wind-driven flows. The presence of an island of nonzero width requires the determination of the baroclinic streamfunction on the basin’s eastern boundary. The value of the boundary term is proportional to the island’s area. This adds a generally small additional baroclinic intergyre flow. In all cases, the intergyre flow produced by the island is not related to topographic steering of the flow but rather the pressure anomaly on the island as manifested by the barotropic and baroclinic island constants. The vertical structure of the flow around the island is a function of the parameterization of the vertical mixing in the problem and, in particular, the degree to which long baroclinic Rossby waves can traverse the basin before becoming thermally damped.
    Description: This research was supported in part by NSF Grant OCE 0451086.
    Keywords: Gyres ; Baroclinic flows ; Topographic effects ; Streamfunction ; Orographic effects
    Repository Name: Woods Hole Open Access Server
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  • 2
    Publication Date: 2022-05-25
    Description: Author Posting. © American Meteorological Society, 2011. This article is posted here by permission of American Meteorological Society for personal use, not for redistribution. The definitive version was published in Journal of Physical Oceanography 41 (2011): 889–910, doi:10.1175/2010JPO4496.1.
    Description: This paper examines interaction between a barotropic point vortex and a steplike topography with a bay-shaped shelf. The interaction is governed by two mechanisms: propagation of topographic Rossby waves and advection by the forcing vortex. Topographic waves are supported by the potential vorticity (PV) jump across the topography and propagate along the step only in one direction, having higher PV on the right. Near one side boundary of the bay, which is in the wave propagation direction and has a narrow shelf, waves are blocked by the boundary, inducing strong out-of-bay transport in the form of detached crests. The wave–boundary interaction as well as out-of-bay transport is strengthened as the minimum shelf width is decreased. The two control mechanisms are related differently in anticyclone- and cyclone-induced interactions. In anticyclone-induced interactions, the PV front deformations are moved in opposite directions by the point vortex and topographic waves; a topographic cyclone forms out of the balance between the two opposing mechanisms and is advected by the forcing vortex into the deep ocean. In cyclone-induced interactions, the PV front deformations are moved in the same direction by the two mechanisms; a topographic cyclone forms out of the wave–boundary interaction but is confined to the coast. Therefore, anticyclonic vortices are more capable of driving water off the topography. The anticyclone-induced transport is enhanced for smaller vortex–step distance or smaller topography when the vortex advection is relatively strong compared to the wave propagation mechanism.
    Description: Y. Zhang acknowledges the support of theMIT-WHOI Joint Programin Physical Oceanography, NSF OCE-9901654 and OCE-0451086. J. Pedlosky acknowledges the support of NSF OCE- 9901654 and OCE-0451086.
    Keywords: Transport ; Eddies ; Barotropic flow ; Topographic effects ; Vortices ; Currents ; Potential vorticity ; Rossby waves
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  • 3
    Publication Date: 2022-05-25
    Description: Author Posting. © American Meteorological Society, 2013. This article is posted here by permission of American Meteorological Society for personal use, not for redistribution. The definitive version was published in Journal of Physical Oceanography 43 (2013): 418–431, doi:10.1175/JPO-D-12-087.1.
    Description: The overflow of the dense water mass across the Greenland–Scotland Ridge (GSR) from the Nordic Seas drives the Atlantic meridional overturning circulation (AMOC). The Nordic Seas is a large basin with an enormous reservoir capacity. The volume of the dense water above the GSR sill depth in the Nordic Seas, according to previous estimates, is sufficient to supply decades of overflow transport. This large capacity buffers overflow’s responses to atmospheric variations and prevents an abrupt shutdown of the AMOC. In this study, the authors use a numerical and an analytical model to show that the effective reservoir capacity of the Nordic Seas is actually much smaller than what was estimated previously. Basin-scale oceanic circulation is nearly geostrophic and its streamlines are basically the same as the isobaths. The vast majority of the dense water is stored inside closed geostrophic contours in the deep basin and thus is not freely available to the overflow. The positive wind stress curl in the Nordic Seas forces a convergence of the dense water toward the deep basin and makes the interior water even more removed from the overflow-feeding boundary current. Eddies generated by the baroclinic instability help transport the interior water mass to the boundary current. But in absence of a robust renewal of deep water, the boundary current weakens rapidly and the eddy-generating mechanism becomes less effective. This study indicates that the Nordic Seas has a relatively small capacity as a dense water reservoir and thus the overflow transport is sensitive to climate changes.
    Description: This study has been supported by National Science Foundation (OCE0927017,ARC1107412).
    Description: 2013-08-01
    Keywords: Bottom currents ; Drainage flow ; Meridional overturning circulation ; Ocean dynamics ; Potential vorticity ; Topographic effects
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  • 4
    Publication Date: 2022-05-25
    Description: Author Posting. © American Meteorological Society, 2009. This article is posted here by permission of American Meteorological Society for personal use, not for redistribution. The definitive version was published in Journal of Physical Oceanography 39 (2009): 1258-1271, doi:10.1175/2008JPO4028.1.
    Description: This paper presents a set of laboratory experiments focused on how a buoyant coastal current flowing over a sloping bottom interacts with a canyon and what controls the separation, if any, of the current from the upstream canyon bend. The results show that the separation of a buoyant coastal current depends on the current width W relative to the radius of curvature of the bathymetry ρc. The flow moved across the mouth of the canyon (i.e., separated) for W/ρc 〉 1, in agreement with previous results. The present study extends previous work by examining both slope-controlled and surface-trapped currents, and using a geometry specific to investigating buoyant current–canyon interaction. The authors find that, although bottom friction is important in setting the position of the buoyant front, the separation process driven by the inertia of the flow could overcome even the strongest bathymetric influence. Application of the laboratory results to the East Greenland Current (EGC), an Arctic-origin buoyant current that is observed to flow in two branches south of Denmark Strait, suggests that the path of the EGC is influenced by the large canyons cutting across the shelf, as the range of W/ρc in the ocean spans those observed in the laboratory. What causes the formation of a two-branched EGC structure downstream of the Kangerdlugssuaq Canyon (68°N, 32°W) is still unclear, but potential mechanisms are discussed.
    Description: This work was partially funded by NSF Grant OCE-0450658. DS also received support from the Academic Programs Office of the Woods Hole Oceanographic Institution, while CC had partial support from NSF OCE-0350891.
    Keywords: Coastal flows ; Buoyancy ; Currents ; Experimental design ; Topographic effects
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  • 5
    Publication Date: 2022-05-25
    Description: Author Posting. © American Meteorological Society, 2008. This article is posted here by permission of American Meteorological Society for personal use, not for redistribution. The definitive version was published in Journal of Physical Oceanography 38 (2008): 104–120, doi:10.1175/2007JPO3686.1.
    Description: Recent studies have indicated that the North Atlantic Ocean subpolar gyre circulation undergoes significant interannual-to-decadal changes in response to variability in atmospheric forcing. There are also observations, however, suggesting that the southern limb of the subpolar gyre, namely, the eastward-flowing North Atlantic Current (NAC), may be quasi-locked to particular latitudes in the central North Atlantic by fracture zones (gaps) in the Mid-Atlantic Ridge. This could constrain the current’s ability to respond to variability in forcing. In the present study, subsurface float trajectories at 100–1000 m collected during 1997–99 and satellite-derived surface geostrophic velocities from 1992 to 2006 are used to provide an improved description of the detailed pathways of the NAC over the ridge and their relationship to bathymetry. Both the float and satellite observations indicate that in 1997–99, the northern branch of the NAC was split into two branches as it crossed the ridge, one quasi-locked to the Charlie–Gibbs Fracture Zone (CGFZ; 52°–53°N) and the other to the Faraday Fracture Zone (50°–51°N). The longer satellite time series shows, however, that this pattern did not persist outside the float sampling period and that other branching modes persisted for one or more years, including an approximately 12-month time period in 2002–03 when the strongest eastward flow over the ridge was at 49°N. Schott et al. showed how northward excursions of the NAC can temporarily block the westward flow of the Iceland–Scotland Overflow Water through the CGFZ. From the 13-yr time series of surface geostrophic velocity, it is estimated that such blocking may occur on average 6% of the time, although estimates for any given 12-month period range from 0% to 35%.
    Description: This research was supported by National Science Foundation Grants OCE-9531877 to the Woods Hole Oceanographic Institution (WHOI) and OCE-9906775 to the University of Rhode Island, by the WHOI Summer Student Fellowship Program, and by the Lawrence J. Pratt and Melinda M. Hall Endowed Fund for Interdisciplinary Research at the Woods Hole Oceanographic Institution.
    Keywords: Currents ; Topographic effects ; Interannual variability ; Forcing ; Gyres
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  • 6
    Publication Date: 2022-05-25
    Description: Author Posting. © American Meteorological Society, 2008. This article is posted here by permission of American Meteorological Society for personal use, not for redistribution. The definitive version was published in Journal of Physical Oceanography 38 (2008): 380-399, doi:10.1175/2007JPO3728.1.
    Description: Barotropic to baroclinic conversion and attendant phenomena were recently examined at the Kaena Ridge as an aspect of the Hawaii Ocean Mixing Experiment. Two distinct mixing processes appear to be at work in the waters above the 1100-m-deep ridge crest. At middepths, above 400 m, mixing events resemble their open-ocean counterparts. There is no apparent modulation of mixing rates with the fortnightly cycle, and they are well modeled by standard open-ocean parameterizations. Nearer to the topography, there is quasi-deterministic breaking associated with each baroclinic crest passage. Large-amplitude, small-scale internal waves are triggered by tidal forcing, consistent with lee-wave formation at the ridge break. These waves have vertical wavelengths on the order of 400 m. During spring tides, the waves are nonlinear and exhibit convective instabilities on their leading edge. Dissipation rates exceed those predicted by the open-ocean parameterizations by up to a factor of 100, with the disparity increasing as the seafloor is approached. These observations are based on a set of repeated CTD and microconductivity profiles obtained from the research platform (R/P) Floating Instrument Platform (FLIP), which was trimoored over the southern edge of the ridge crest. Ocean velocity and shear were resolved to a 4-m vertical scale by a suspended Doppler sonar. Dissipation was estimated both by measuring overturn displacements and from microconductivity wavenumber spectra. The methods agreed in water deeper than 200 m, where sensor resolution limitations do not limit the turbulence estimates. At intense mixing sites new phenomena await discovery, and existing parameterizations cannot be expected to apply.
    Description: This work was funded by the National Science Foundation as a component of the Hawaii Ocean Mixing Program. Added support for FLIP was provided by the Office of Naval Research.
    Keywords: Pacific Ocean ; Topographic effects ; Internal waves ; Barotropic flows ; Baroclinic flows
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  • 7
    Publication Date: 2022-05-25
    Description: Author Posting. © American Meteorological Society, 2011. This article is posted here by permission of American Meteorological Society for personal use, not for redistribution. The definitive version was published in Journal of Physical Oceanography 41 (2011): 2168–2186, doi:10.1175/JPO-D-11-08.1.
    Description: This paper studies the interaction of an Antarctic Circumpolar Current (ACC)–like wind-driven channel flow with a continental slope and a flat-bottomed bay-shaped shelf near the channel’s southern boundary. Interaction between the model ACC and the topography in the second layer induces local changes of the potential vorticity (PV) flux, which further causes the formation of a first-layer PV front near the base of the topography. Located between the ACC and the first-layer slope, the newly formed PV front is constantly perturbed by the ACC and in turn forces the first-layer slope with its own variability in an intermittent but persistent way. The volume transport of the slope water across the first-layer slope edge is mostly directly driven by eddies and meanders of the new front, and its magnitude is similar to the maximum Ekman transport in the channel. Near the bay’s opening, the effect of the topographic waves, excited by offshore variability, dominates the cross-isobath exchange and induces a mean clockwise shelf circulation. The waves’ propagation is only toward the west and tends to be blocked by the bay’s western boundary in the narrow-shelf region. The ensuing wave–coast interaction amplifies the wave amplitude and the cross-shelf transport. Because the interaction only occurs near the western boundary, the shelf water in the west of the bay is more readily carried offshore than that in the east and the mean shelf circulation is also intensified along the bay’s western boundary.
    Description: Y. Zhang acknowledges the support of the MIT-WHOI Joint Program in Physical Oceanography and NSF OCE-9901654 and OCE- 0451086. J. Pedlosky acknowledges the support of NSF OCE-9901654 and OCE-0451086.
    Keywords: Baroclinic flows ; Eddies ; Fronts ; Mass fluxes/transport ; Mesoscale processes ; Topographic effects
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  • 8
    Publication Date: 2022-05-25
    Description: Author Posting. © American Meteorological Society, 2009. This article is posted here by permission of American Meteorological Society for personal use, not for redistribution. The definitive version was published in Journal of Physical Oceanography 39 (2009): 387-403, doi:10.1175/2008JPO3934.1.
    Description: Marginal sea overflows and the overlying upper ocean are coupled in the vertical by two distinct mechanisms—by an interfacial mass flux from the upper ocean to the overflow layer that accompanies entrainment and by a divergent eddy flux associated with baroclinic instability. Because both mechanisms tend to be localized in space, the resulting upper ocean circulation can be characterized as a β plume for which the relevant background potential vorticity is set by the slope of the topography, that is, a topographic β plume. The entrainment-driven topographic β plume consists of a single gyre that is aligned along isobaths. The circulation is cyclonic within the upper ocean (water columns are stretched). The transport within one branch of the topographic β plume may exceed the entrainment flux by a factor of 2 or more. Overflows are likely to be baroclinically unstable, especially near the strait. This creates eddy variability in both the upper ocean and overflow layers and a flux of momentum and energy in the vertical. In the time mean, the eddies accompanying baroclinic instability set up a double-gyre circulation in the upper ocean, an eddy-driven topographic β plume. In regions where baroclinic instability is growing, the momentum flux from the overflow into the upper ocean acts as a drag on the overflow and causes the overflow to descend the slope at a steeper angle than what would arise from bottom friction alone. Numerical model experiments suggest that the Faroe Bank Channel overflow should be the most prominent example of an eddy-driven topographic β plume and that the resulting upper-layer transport should be comparable to that of the overflow. The overflow-layer eddies that accompany baroclinic instability are analogous to those observed in moored array data. In contrast, the upper layer of the Mediterranean overflow is likely to be dominated more by an entrainment-driven topographic β plume. The difference arises because entrainment occurs at a much shallower location for the Mediterranean case and the background potential vorticity gradient of the upper ocean is much larger.
    Description: SK’s support during the time of his Ph.D. research in the MIT/WHOI Joint Program was provided by the National Science Foundation through Grant OCE04-24741. JP and JY have also received support from the Climate Process Team on Gravity Current Entrainment, NSF Grant OCE-0611530. JY has also been supported by NSF Grant OCE-0351055.
    Keywords: Baroclinic flows ; Mass fluxes/transport ; Entrainment ; Topographic effects ; Potential vorticity
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  • 9
    Publication Date: 2022-05-25
    Description: Author Posting. © American Meteorological Society, 2013. This article is posted here by permission of American Meteorological Society for personal use, not for redistribution. The definitive version was published in Journal of Physical Oceanography 43 (2013): 766–789, doi:10.1175/JPO-D-12-0141.1.
    Description: Nonlinear energy transfers from the semidiurnal internal tide to high-mode, near-diurnal motions are documented near Kaena Ridge, Hawaii, an energetic generation site for the baroclinic tide. Data were collected aboard the Research Floating Instrument Platform (FLIP) over a 35-day period during the fall of 2002, as part of the Hawaii Ocean Mixing Experiment (HOME) Nearfield program. Energy transfer terms for a PSI resonant interaction at midlatitude are identified and compared to those for near-inertial PSI close to the M2 critical latitude. Bispectral techniques are used to demonstrate significant energy transfers in the Nearfield, between the low-mode M2 internal tide and subharmonic waves with frequencies near M2/2 and vertical wavelengths of O(120 m). A novel prefilter is used to test the PSI wavenumber resonance condition, which requires the subharmonic waves to propagate in opposite vertical directions. Depth–time maps of the interactions, formed by directly estimating the energy transfer terms, show that energy is transferred predominantly from the tide to subharmonic waves, but numerous reverse energy transfers are also found. A net forward energy transfer rate of 2 × 10−9 W kg−1 is found below 400 m. The suggestion is that the HOME observations of energy transfer from the tide to subharmonic waves represent a first step in the open-ocean energy cascade. Observed PSI transfer rates could account for a small but significant fraction of the turbulent dissipation of the tide within 60 km of Kaena Ridge. Further extrapolation suggests that integrated PSI energy transfers equatorward of the M2 critical latitude may be comparable to PSI energy transfers previously observed near 28.8°N.
    Description: This work was supported by the National Science Foundation and the Office of Naval Research.
    Description: 2013-10-01
    Keywords: Diapycnal mixing ; Energy transport ; Internal waves ; Nonlinear dynamics ; Topographic effects ; In situ oceanic observations
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  • 10
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    American Meteorological Society
    Publication Date: 2022-05-25
    Description: Author Posting. © American Meteorological Society, 2013. This article is posted here by permission of American Meteorological Society for personal use, not for redistribution. The definitive version was published in Journal of Physical Oceanography 43 (2013): 1398–1406, doi:10.1175/JPO-D-13-028.1.
    Description: An adiabatic, inertial, and quasigeostrophic model is used to discuss the interaction of surface Ekman transport with an island. The theory extends the recent work of Spall and Pedlosky to include an analytical and nonlinear model for the interaction. The presence of an island that interrupts a uniform Ekman layer transport raises interesting questions about the resulting circulation. The consequential upwelling around the island can lead to a local intake of fluid from the geostrophic region beneath the Ekman layer or to a more complex flow around the island in which the fluid entering the Ekman layer on one portion of the island's perimeter is replaced by a flow along the island's boundary from a downwelling region located elsewhere on the island. This becomes especially pertinent when the flow is quasigeostrophic and adiabatic. The oncoming geostrophic flow that balances the offshore Ekman flux is largely diverted around the island, and the Ekman flux is fed by a transfer of fluid from the western to the eastern side of the island. As opposed to the linear, dissipative model described earlier, this transfer takes place even in the absence of a topographic skirt around the island. The principal effect of topography in the inertial model is to introduce an asymmetry between the circulation on the northern and southern sides of the island. The quasigeostrophic model allows a simple solution to the model problem with topography and yet the resulting three-dimensional circulation is surprisingly complex with streamlines connecting each side of the island.
    Description: This research was supported in part by NSF Grant OCE Grant 0925061.
    Keywords: Baroclinic flows ; Large-scale motions ; Nonlinear dynamics ; Ocean circulation ; Ocean dynamics ; Topographic effects
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  • 11
    Publication Date: 2022-05-25
    Description: Author Posting. © American Meteorological Society, 2010. This article is posted here by permission of American Meteorological Society for personal use, not for redistribution. The definitive version was published in Journal of Physical Oceanography 40 (2010): 2679–2695, doi:10.1175/2010JPO4395.1.
    Description: Observations of stratification and currents between June 2007 and March 2009 reveal a strong overflow between 400- and 570-m depth from the Panay Strait into the Sulu Sea. The overflow water is derived from approximately 400 m deep in the South China Sea. Temporal mean velocity is greater than 0.75 m s−1 at 50 m above the 570-m Panay Sill. Empirical orthogonal function analysis of a mooring time series shows that the flow is dominated by the bottom overflow current with little seasonal variance. The overflow does not descend below 1250 m in the Sulu Sea but rather settles above high-salinity deep water derived from the Sulawesi Sea. The mean observed overflow transport at the sill is 0.32 × 106 m3 s−1. The observed transport was used to calculate a bulk diapycnal diffusivity of 4.4 × 10−4 m2 s−1 within the Sulu Sea slab (575–1250 m) ventilated from Panay Strait. Analysis of Froude number variation across the sill shows that the flow is hydraulically controlled. A suitable hydraulic control model shows overflow transport equivalent to the observed overflow. Thorpe-scale estimates show turbulent dissipation rates up to 5 × 10−7 W kg−1 just downstream of the supercritical to subcritical flow transition, suggesting a hydraulic jump downstream of the sill.
    Description: This work was supported by the Office of Naval Research Grant N00014-09-1-0582 to Lamont-Doherty Earth Observatory of Columbia University; Grants ONR-13759000 and N00014-09-1-0582 to the Woods Hole Oceanographic Institution; Grant ONR-N00014-06-1-0690 to Scripps Institute of Oceanography; and a National Defense Science and Engineering Graduate Fellowship.
    Keywords: Transport ; Dynamics ; Topographic effects ; Currents ; Empirical orthogonal functions
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  • 12
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    Cambridge University Press
    Publication Date: 2022-05-25
    Description: Author Posting. © Cambridge University Press, 2013. This article is posted here by permission of Cambridge University Press for personal use, not for redistribution. The definitive version was published in Journal of Fluid Mechanics 726 (2013): 371-403, doi:10.1017/jfm.2013.231.
    Description: Nonlinear stratified spindown of an along-isobath current over an insulated slope is shown to develop asymmetries in the vertical circulation and vertical relative vorticity field. During spindown, cyclonic vorticity is weakened to a greater extent than anticyclonic vorticity near the boundary because of buoyancy advection. As a consequence, Ekman pumping is weakened over Ekman suction. Momentum advection can weaken Ekman pumping and strengthen Ekman suction. Time-dependent feedback between the geostrophic flow and the frictional secondary circulation induces asymmetry in cyclonic and anticyclonic vorticity away from the boundary. Buoyancy advection over a slope can modify the secondary circulation such that anticyclonic vorticity decays faster than cyclonic vorticity outside the boundary layer. In contrast, momentum advection can cause cyclonic vorticity to spin down faster than anticyclonic vorticity. A scaling and analytical solutions are derived for when buoyancy advection over a slope can have a more significant impact than momentum advection on these asymmetries. In order to test this scaling and analytical solutions, numerical experiments are run in which both buoyancy and momentum advection are active. These solutions are contrasted with homogeneous or stratified spindown over a flat bottom, in which momentum advection controls the asymmetries. These results are applied to ocean currents over continental shelves and slopes.
    Description: 2014-06-05
    Keywords: Geophysical flows ; Ocean circulation ; Topographic effects
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  • 13
    Publication Date: 2022-05-25
    Description: Author Posting. © American Meteorological Society, 2014. This article is posted here by permission of American Meteorological Society for personal use, not for redistribution. The definitive version was published in Journal of Physical Oceanography 44 (2014): 2938–2950, doi:10.1175/JPO-D-13-0201.1.
    Description: Direct observations in the Southern Ocean report enhanced internal wave activity and turbulence in a kilometer-thick layer above rough bottom topography collocated with the deep-reaching fronts of the Antarctic Circumpolar Current. Linear theory, corrected for finite-amplitude topography based on idealized, two-dimensional numerical simulations, has been recently used to estimate the global distribution of internal wave generation by oceanic currents and eddies. The global estimate shows that the topographic wave generation is a significant sink of energy for geostrophic flows and a source of energy for turbulent mixing in the deep ocean. However, comparison with recent observations from the Diapycnal and Isopycnal Mixing Experiment in the Southern Ocean shows that the linear theory predictions and idealized two-dimensional simulations grossly overestimate the observed levels of turbulent energy dissipation. This study presents two- and three-dimensional, realistic topography simulations of internal lee-wave generation from a steady flow interacting with topography with parameters typical of Drake Passage. The results demonstrate that internal wave generation at three-dimensional, finite bottom topography is reduced compared to the two-dimensional case. The reduction is primarily associated with finite-amplitude bottom topography effects that suppress vertical motions and thus reduce the amplitude of the internal waves radiated from topography. The implication of these results for the global lee-wave generation is discussed.
    Description: This research was supported by the National Science Foundation under Award CMG-1024198.
    Description: 2015-05-01
    Keywords: Circulation/ Dynamics ; Diapycnal mixing ; Internal waves ; Mixing ; Mountain waves ; Topographic effects ; Waves, oceanic
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  • 14
    Publication Date: 2022-05-26
    Description: Author Posting. © American Meteorological Society, 2014. This article is posted here by permission of American Meteorological Society for personal use, not for redistribution. The definitive version was published in Journal of Physical Oceanography 44 (2014): 834-849, doi:10.1175/JPO-D-13-0179.1.
    Description: A hydrostatic numerical model with alongshore-uniform barotropic M2 tidal boundary forcing and idealized shelfbreak canyon bathymetries is used to study internal-tide generation and onshore propagation. A control simulation with Mid-Atlantic Bight representative bathymetry is supported by other simulations that serve to identify specific processes. The canyons and adjacent slopes are transcritical in steepness with respect to M2 internal wave characteristics. Although the various canyons are symmetrical in structure, barotropic-to-baroclinic energy conversion rates Cυ are typically asymmetrical within them. The resulting onshore-propagating internal waves are the strongest along beams in the horizontal plane, with the stronger beam in the control simulation lying on the side with higher Cυ. Analysis of the simulation results suggests that the cross-canyon asymmetrical Cυ distributions are caused by multiple-scattering effects on one canyon side slope, because the phase variation in the spatially distributed internal-tide sources, governed by variations in the orientation of the bathymetry gradient vector, allows resonant internal-tide generation. A less complex, semianalytical, modal internal wave propagation model with sources placed along the critical-slope locus (where the M2 internal wave characteristic is tangent to the seabed) and variable source phasing is used to diagnose the physics of the horizontal beams of onshore internal wave radiation. Model analysis explains how the cross-canyon phase and amplitude variations in the locally generated internal tides affect parameters of the internal-tide beams. Under the assumption that strong internal tides on continental shelves evolve to include nonlinear wave trains, the asymmetrical internal-tide generation and beam radiation effects may lead to nonlinear internal waves and enhanced mixing occurring preferentially on one side of shelfbreak canyons, in the absence of other influencing factors.
    Description: All three authors were supported by Office of Naval Research (ONR) Grant N00014-11-1-0701. WGZ was additionally supported by the National Science Foundation (NSF) Grant OCE-1154575, and TFD was additionally supported by NSF Grant OCE-1060430.
    Description: 2014-09-01
    Keywords: Circulation/ Dynamics ; Baroclinic flows ; Internal waves ; Ocean circulation ; Topographic effects ; Waves, oceanic ; Models and modeling ; Numerical analysis/modeling
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  • 15
    ISSN: 0992-7689
    Keywords: Solar physics ; Astrophysics ; Astronomy ; Magnetic fields ; Space plasma physics ; Charged particle motion and acceleration
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract EISCAT observations of the interplanetary scintillation of a single source were made over an extended period of time, during which the orientation of the baselines between the two observing sites changed significantly. Assuming that maximum correlation between the scintillations observed at the two sites occurs when the projected baseline is parallel to the direction of plasma flow, this technique can be used to make a unique determination of the direction of the solar wind. In the past it has usually been assumed that the plasma flow is radial, but measurements of eleven sources using this technique have indicated conclusively that in at least six cases observed at mid or high heliocentric latitude there is a significant non-radial component directed in four cases towards the heliocentric equator and in two cases towards the pole.
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  • 16
    Electronic Resource
    Electronic Resource
    Springer
    Boundary layer meteorology 92 (1999), S. 145-162 
    ISSN: 1573-1472
    Keywords: Iceland ; Vatnajökull ; Low cloud ; Glacier wind ; Coastal winds ; Topographic effects
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract An impressive cloud wall has frequently been observed on the southern slopes of the Vatnajökull ice sheet, which is located in south-eastern Iceland. Its optical and dynamic features suggest a delicate balance of the atmospheric agents involved. This has been confirmed by a thorough analysis of a well documented event and by statistics covering a whole summer season. As an exemplary event, the regional development of the associated cloud has basically been documented with synchronous surface data along a suitable transect of the glacier. Data from tethered balloons, radiosoundings and routine synoptic data have also been exploited extensively. Cloud development was generally aided by a high moisture potential because of proximity to the open seas and the remnants of a frontal system. Furthermore the occurrence of the cloud phenomenon was associated with onshore (southerly) surface winds, assisting advection and lifting of the associated air masses above the slopes of the ice sheet. Northward protrusion of the associated cloud was apparently opposed by continuous katabatic winds and topographically induced lee effects.
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  • 17
    Publication Date: 2014-12-17
    Description: Author(s): Yun-He Li, Jing-Fei Zhang, and Xin Zhang Dark energy can modify the dynamics of dark matter if there exists a direct interaction between them. Thus, a measurement of the structure growth, e.g., redshift-space distortions (RSDs), can provide a powerful tool to constrain the interacting dark energy (IDE) models. For the widely studied Q=3βHρ ... [Phys. Rev. D 90, 123007] Published Tue Dec 16, 2014
    Keywords: Astrophysics
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  • 18
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    American Physical Society (APS)
    Publication Date: 2014-12-18
    Description: Author(s): Kiyotomo Ichiki One working hypothesis on which analyses of cosmological data are based is the zero ensemble mean hypothesis, which is related to the statistical homogeneity of cosmological perturbations. This hypothesis, however, should be tested by observational data in the current era of precision cosmology. Her... [Phys. Rev. D 90, 123008] Published Wed Dec 17, 2014
    Keywords: Astrophysics
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  • 19
    Publication Date: 2014-12-04
    Description: Author(s): Joohan Lee, James M. Overduin, Tae Hoon Lee, and Phillial Oh We present a simple cosmological model in which a single, nonminimally coupled scalar field with a quartic potential is responsible for both inflation at early times and acceleration at late times. Little or no fine tuning is needed to explain why the present density of dark energy is comparable to ... [Phys. Rev. D 90, 123003] Published Wed Dec 03, 2014
    Keywords: Astrophysics
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  • 20
    Publication Date: 2014-12-04
    Description: Author(s): José M. Torres, Miguel Alcubierre, Alberto Diez-Tejedor, and Darío Núñez We perform numerical evolutions of cosmological scenarios using a standard general relativistic code in spherical symmetry. We concentrate on two different situations: initial matter distributions that are homogeneous and isotropic, and perturbations to those that respect the spherical symmetry. As ... [Phys. Rev. D 90, 123002] Published Wed Dec 03, 2014
    Keywords: Astrophysics
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  • 21
    Publication Date: 2014-12-05
    Description: Author(s): Andreas Schärer, Raymond Angélil, Ruxandra Bondarescu, Philippe Jetzer, and Andrew Lundgren We compute the parametrized post-Newtonian (PPN) parameters γ and β for general scalar-tensor theories in the Einstein frame, which we compare to the existing PPN formulation in the Jordan frame for alternative theories of gravity. This computation is important for scalar-tensor theories that are ex... [Phys. Rev. D 90, 123005] Published Thu Dec 04, 2014
    Keywords: Astrophysics
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  • 22
    Publication Date: 2011-04-02
    Description: Author(s): F. Käppeler, R. Gallino, S. Bisterzo, and Wako Aoki Nucleosynthesis in the s process takes place in the He-burning layers of low-mass asymptotic giant branch (AGB) stars and during the He- and C-burning phases of massive stars. The s process contributes about half of the element abundances between Cu and Bi in solar system material. Depending on ste... [Rev. Mod. Phys. 83, 157] Published Fri Apr 01, 2011
    Keywords: Astrophysics
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  • 23
    Publication Date: 2014-01-15
    Description: Author(s): Apurba Kheto and Debades Bandyopadhyay We study the entrainment effect between superfluid neutrons and charge neutral fluid (called the proton fluid) which is made of protons and electrons in a neutron star interior within the two-fluid formalism and using a relativistic model where baryon-baryon interaction is mediated by the exchange o... [Phys. Rev. D 89, 023007] Published Tue Jan 14, 2014
    Keywords: Astrophysics
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  • 24
    Publication Date: 2014-01-15
    Description: Author(s): F. Y. Wang and Z. G. Dai The equation of state (EOS), w(z), is the most important parameter of dark energy. We reconstruct the evolution of this EOS in a model-independent way using the latest cosmic microwave background (CMB) data from Planck and other observations, such as type Ia supernovae, the baryonic acoustic oscilla... [Phys. Rev. D 89, 023004] Published Tue Jan 14, 2014
    Keywords: Astrophysics
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  • 25
    Publication Date: 2014-01-17
    Description: Author(s): Donghui Jeong, Jens Chluba, Liang Dai, Marc Kamionkowski, and Xin Wang Our motion relative to the cosmic microwave background (CMB) rest frame deflects light rays giving rise to shifts as large as ℓ→ℓ(1±β), where β=0.00123   is our velocity (in units of the speed of light) on measurements of CMB fluctuations. Here we present a novel harmonic-space approach to this CMB ... [Phys. Rev. D 89, 023003] Published Thu Jan 16, 2014
    Keywords: Astrophysics
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  • 26
    Publication Date: 2014-01-16
    Description: Author(s): Joshua S. Dillon, Adrian Liu, Christopher L. Williams, Jacqueline N. Hewitt, Max Tegmark, Edward H. Morgan, Alan M. Levine, Miguel F. Morales, Steven J. Tingay, Gianni Bernardi, Judd D. Bowman, Frank H. Briggs, Roger C. Cappallo, David Emrich, Daniel A. Mitchell, Divya Oberoi, Thiagaraj Prabu, Randall Wayth, and Rachel L. Webster We present techniques for bridging the gap between idealized inverse covariance weighted quadratic estimation of 21 cm power spectra and the real-world challenges presented universally by interferometric observation. By carefully evaluating various estimators and adapting our techniques for large bu... [Phys. Rev. D 89, 023002] Published Wed Jan 15, 2014
    Keywords: Astrophysics
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  • 27
    Publication Date: 2014-01-17
    Description: Author(s): Yi-Fu Cai, Wen Zhao, and Yang Zhang The hemispherical power asymmetry in the cosmic microwave background can be explained by the modulation of some primordial cosmological parameters, such as the sound speed of the inflaton. Inspired by new physics beyond the standard knowledge of particle cosmology, this sound speed modulation greatl... [Phys. Rev. D 89, 023005] Published Thu Jan 16, 2014
    Keywords: Astrophysics
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  • 28
    Publication Date: 2014-05-06
    Description: Author(s): A. Neronov, D. Semikoz, and C. Tchernin We present a self-consistent interpretation of the very high-energy neutrino signal from the direction of the inner Galaxy, which is a part of the astronomical neutrino signal reported by IceCube. We demonstrate that an estimate of the neutrino flux in the E〉100  TeV energy range lies at the high... [Phys. Rev. D 89, 103002] Published Mon May 05, 2014
    Keywords: Astrophysics
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  • 29
    Publication Date: 2014-05-06
    Description: Author(s): Andrew M. Taylor, Stefano Gabici, and Felix Aharonian Recent IceCube results suggest that the first detection of very high energy astrophysical neutrinos have been accomplished. We consider these results at face value in a Galactic origin context. Emission scenarios from both the Fermi bubble and broader halo region are considered. We motivate that suc... [Phys. Rev. D 89, 103003] Published Mon May 05, 2014
    Keywords: Astrophysics
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  • 30
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    American Physical Society (APS)
    Publication Date: 2014-03-20
    Description: Author(s): Ue-Li Pen and Pengjie Zhang We consider the generic scenario of dark energy that arises through the latent heat of a hidden sector first-order cosmological phase transition. This field could account for the extra radiation degree of freedom suggested by the CMB. We present the bubble nucleation solution for the viscous limit. ... [Phys. Rev. D 89, 063009] Published Wed Mar 19, 2014
    Keywords: Astrophysics
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  • 31
    Publication Date: 2014-05-01
    Description: Author(s): M. C. Ferreira, O. Frigola, C. J. A. P. Martins, A. M. R. V. L. Monteiro, and J. Solà We test the consistency of several independent astrophysical measurements of fundamental dimensionless constants. In particular, we compare direct measurements of the fine-structure constant α and the proton-to-electron mass ratio μ=mp/me (mostly in the optical/ultraviolet) with combined measurement... [Phys. Rev. D 89, 083011] Published Wed Apr 30, 2014
    Keywords: Astrophysics
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  • 32
    Publication Date: 2014-04-25
    Description: Author(s): Yun-He Li and Xin Zhang Dark energy might interact with cold dark matter in a direct, nongravitational way. However, the usual interacting dark energy models (with constant w) suffer from some catastrophic difficulties. For example, the Q∝ρc model leads to an early-time large-scale instability, and the Q∝ρde model gives ri... [Phys. Rev. D 89, 083009] Published Thu Apr 24, 2014
    Keywords: Astrophysics
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  • 33
    Publication Date: 2014-01-25
    Description: Author(s): Jeremiah Birrell, Cheng-Tao Yang, Pisin Chen, and Johann Rafelski We perform a model independent study of the neutrino momentum distribution at freeze-out, treating the freeze-out temperature as a free parameter. Our results imply that measurement of neutrino reheating, as characterized by the measurement of the effective number of neutrinos Nν, amounts to the det... [Phys. Rev. D 89, 023008] Published Fri Jan 24, 2014
    Keywords: Astrophysics
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  • 34
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    American Physical Society (APS)
    Publication Date: 2014-02-22
    Description: Author(s): Mohammed Mia By considering fluxes on D7 branes and explicitly computing their backreaction on the geometry with and without a black hole, we show how the UV divergence of the Klebanov-Strassler model can be regulated. Using the form of the metric and fluxes in the extremal and nonextremal limits, we compute the... [Phys. Rev. D 89, 043010] Published Fri Feb 21, 2014
    Keywords: Astrophysics
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  • 35
    Publication Date: 2014-02-22
    Description: Author(s): Benjamin D. Lackey, Koutarou Kyutoku, Masaru Shibata, Patrick R. Brady, and John L. Friedman Information about the neutron-star equation of state is encoded in the waveform of a black hole-neutron star system through tidal interactions and the possible tidal disruption of the neutron star. During the inspiral this information depends on the tidal deformability Λ of the neutron star, and we ... [Phys. Rev. D 89, 043009] Published Fri Feb 21, 2014
    Keywords: Astrophysics
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  • 36
    Publication Date: 2014-02-25
    Description: Author(s): Ilias Cholis and Dan Hooper The rapid rise in the cosmic ray positron fraction above 10 GeV, as measured by PAMELA and AMS, suggests the existence of nearby primary sources of high energy positrons, such as pulsars or annihilating/decaying dark matter. In contrast, the spectrum of secondary positrons produced through the colli... [Phys. Rev. D 89, 043013] Published Mon Feb 24, 2014
    Keywords: Astrophysics
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  • 37
    Publication Date: 2014-02-25
    Description: Author(s): Kohta Murase, Basudeb Dasgupta, and Todd A. Thompson Rotating and magnetized protoneutron stars may drive relativistic magnetocentrifugally accelerated winds as they cool immediately after core collapse. The wind fluid near the star is composed of neutrons and protons, and the neutrons become relativistic while collisionally coupled with the ions. Her... [Phys. Rev. D 89, 043012] Published Mon Feb 24, 2014
    Keywords: Astrophysics
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  • 38
    Publication Date: 2014-03-26
    Description: Author(s): Eric Thrane and Michael Coughlin The problem of searching for unmodeled gravitational-wave bursts can be thought of as a pattern recognition problem: how to find statistically significant clusters in spectrograms of strain power when the precise signal morphology is unknown. In a previous publication, we showed how “seedless cluste... [Phys. Rev. D 89, 063012] Published Tue Mar 25, 2014
    Keywords: Astrophysics
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  • 39
    Publication Date: 2014-03-27
    Description: Author(s): Suvodip Mukherjee and Tarun Souradeep Although theoretically expected to be statistically isotropic (SI), the observed cosmic microwave background (CMB) temperature and polarization field would exhibit SI violation due to various inevitable effects like weak lensing, Doppler boost, and practical limitations of observations like noncircu... [Phys. Rev. D 89, 063013] Published Wed Mar 26, 2014
    Keywords: Astrophysics
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  • 40
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    American Physical Society (APS)
    Publication Date: 2014-04-01
    Description: Author(s): Rongjia Yang We investigate the growth of the large-scale structure in the superfluid Chaplygin gas (SCG) model. Both linear and nonlinear growth, such as σ8 and the skewness S3, are discussed. We find the growth factor of SCG reduces to the Einstein–de Sitter case at early times while it differs from the cosmol... [Phys. Rev. D 89, 063014] Published Mon Mar 31, 2014
    Keywords: Astrophysics
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  • 41
    Publication Date: 2014-04-03
    Description: Author(s): Kenny C. Y. Ng, Ranjan Laha, Sheldon Campbell, Shunsaku Horiuchi, Basudeb Dasgupta, Kohta Murase, and John F. Beacom The extragalactic dark matter (DM) annihilation signal depends on the product of the clumping factor, ⟨δ2⟩, and the velocity-weighted annihilation cross section, σv. This “clumping factor–σv” degeneracy can be broken by comparing DM annihilation signals from multiple sources. In particular, one can ... [Phys. Rev. D 89, 083001] Published Wed Apr 02, 2014
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  • 42
    Publication Date: 2014-04-04
    Description: Author(s): Zacharias Roupas, Minos Axenides, George Georgiou, and Emmanuel N. Saridakis A self-gravitating gas in the Newtonian limit is studied in the presence of dark energy with a linear and constant equation of state. Entropy extremization associates to the isothermal Boltzmann distribution an effective density that includes “dark energy particles”—which either strengthen or weaken... [Phys. Rev. D 89, 083002] Published Thu Apr 03, 2014
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  • 43
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    Publication Date: 2011-09-08
    Description: Author(s): Antoine Letessier-Selvon and Todor Stanev The discovery of cosmic rays - charged particles that originate outside the solar system - was made almost 100 years ago. Today the cosmic ray energy spectrum is known to extend more than 14 orders of magnitude, from 10 (6) to above 10 (20)   eV . Nevertheless, after decades of research the physics behi... [Rev. Mod. Phys. 83, 907] Published Wed Sep 07, 2011
    Keywords: Astrophysics
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  • 44
    Publication Date: 2011-09-30
    Description: Author(s): N. Prantzos, C. Boehm, A. M. Bykov, R. Diehl, K. Ferrière, N. Guessoum, P. Jean, J. Knoedlseder, A. Marcowith, I. V. Moskalenko, A. Strong, and G. Weidenspointner The first gamma-ray line ever detected from outside the Solar System witnesses electron-positron annihilation in the Galaxy. Its true origin is still not understood but after 30 years of research, gamma-ray observatories revealed a strong concentration of the emission towards the galactic bulge with... [Rev. Mod. Phys. 83, 1001] Published Thu Sep 29, 2011
    Keywords: Astrophysics
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  • 45
    Publication Date: 2012-01-18
    Description: Author(s): André Maeder and Georges Meynet How does rotation change the evolution, end stages, and stellar winds as well as types of supernovae explosions? This question is not only of importance for the fate of individual stars in galaxies, but also for the populations of blue and red supergiants, Wolf-Rayet stars, the progenitors of supern... [Rev. Mod. Phys. 84, 25] Published Tue Jan 17, 2012
    Keywords: Astrophysics
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  • 46
    Publication Date: 2014-09-23
    Description: Author(s): Tamal Sarkar, Shubhrangshu Ghosh, and Arunava Bhadra The late time accelerated expansion of the Universe demands that even in local galactic scales it is desirable to study astrophysical phenomena, particularly relativistic accretion related phenomena in massive galaxies or in galaxy mergers and the dynamics of the kiloparsecs-scale structure and beyo... [Phys. Rev. D 90, 063008] Published Mon Sep 22, 2014
    Keywords: Astrophysics
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  • 47
    Publication Date: 2014-10-02
    Description: Author(s): Jian-hua Gao, Bin Qi, and Shou-Yu Wang In the framework of relativistic ideal hydrodynamics, we study the production mechanism for vorticity and magnetic field in relativistic ideal fluids. It is demonstrated that in the uncharged fluids the thermal vorticity will always satisfy the Kelvin’s theorem and the circulation must be conserved.... [Phys. Rev. D 90, 083001] Published Wed Oct 01, 2014
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  • 48
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    American Physical Society (APS)
    Publication Date: 2014-10-07
    Description: Author(s): M. Kachelrieß and S. Ostapchenko We calculate the neutrino yield from collisions of cosmic ray (CR) nuclei with gas using the event generator QGSJET-II. We present first the general characteristics and numerical results for the neutrino yield assuming power-law fluxes for the primary CR nuclei. Then we use three parametrizations fo... [Phys. Rev. D 90, 083002] Published Mon Oct 06, 2014
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  • 49
    Publication Date: 2014-08-30
    Description: Author(s): Jannis Bielefeld, Robert R. Caldwell, and Eric V. Linder The dark sector of the Universe need not be completely separable into distinct dark matter and dark energy components. We consider a model of early dark energy in which the dark energy mimics a dark matter component in both evolution and perturbations at early times. Barotropic aether dark energy sc... [Phys. Rev. D 90, 043015] Published Fri Aug 29, 2014
    Keywords: Astrophysics
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  • 50
    Publication Date: 2014-10-30
    Description: Author(s): Shuo Cao and Zong-Hong Zhu Using relatively complete observational data concerning four angular diameter distance (ADD) measurements and combined SN+GRB observations representing current luminosity distance (LD) data, this paper investigates the compatibility of these two cosmological distances considering three classes of da... [Phys. Rev. D 90, 083006] Published Wed Oct 29, 2014
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  • 51
    Publication Date: 2014-08-26
    Description: Author(s): Sheila Dwyer and Stefan W. Ballmer Radiative losses have traditionally been neglected in the calculation of thermal noise of transmissive optical elements because for the most commonly used geometries they are small compared to losses due to thermal conduction. We explore the use of such transmissive optical elements in extremely noi... [Phys. Rev. D 90, 043013] Published Mon Aug 25, 2014
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  • 52
    Publication Date: 2014-08-28
    Description: Author(s): Peter L. Gonthier, Matthew G. Baring, Matthew T. Eiles, Zorawar Wadiasingh, Caitlin A. Taylor, and Catherine J. Fitch The quantum electrodynamical (QED) process of Compton scattering in strong magnetic fields is commonly invoked in atmospheric and inner magnetospheric models of x-ray and soft gamma-ray emission in high-field pulsars and magnetars. A major influence of the field is to introduce resonances at the cyc... [Phys. Rev. D 90, 043014] Published Wed Aug 27, 2014
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  • 53
    Publication Date: 2014-09-17
    Description: Author(s): Yun-He Li, Jing-Fei Zhang, and Xin Zhang Dark energy might directly interact with cold dark matter. However, in such a scenario, an early-time large-scale instability occurs occasionally, which may be due to the incorrect treatment for the pressure perturbation of dark energy as a nonadiabatic fluid. To avoid this nonphysical instability, ... [Phys. Rev. D 90, 063005] Published Tue Sep 16, 2014
    Keywords: Astrophysics
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  • 54
    Publication Date: 2014-09-24
    Description: Author(s): Kent Yagi, Leo C. Stein, George Pappas, Nicolás Yunes, and Theocharis A. Apostolatos Black holes are said to have no hair because all of their multipole moments can be expressed in terms of just their mass, charge and spin angular momentum. The recent discovery of approximately equation-of-state-independent relations among certain multipole moments in neutron stars suggests that the... [Phys. Rev. D 90, 063010] Published Tue Sep 23, 2014
    Keywords: Astrophysics
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  • 55
    Publication Date: 2014-09-24
    Description: Author(s): Amol V. Patwardhan and George M. Fuller We show that a particular class of postrecombination phase transitions in the vacuum can lead to localized overdense regions on relatively small scales, roughly 106 to 1010M⊙, potentially interesting for the origin of large black hole seeds and for dwarf galaxy evolution. Our study suggests that thi... [Phys. Rev. D 90, 063009] Published Tue Sep 23, 2014
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  • 56
    Publication Date: 2014-08-22
    Description: Author(s): Cynthia Keeler, Finn Larsen, and Pedro Lisbão By means of a new efficient method for computing the one-loop corrections to the entropy of supersymmetric four-dimensional black holes, the logarithmic correction to the Bekenstein-Hawking area law is found. [Phys. Rev. D 90, 043011] Published Thu Aug 21, 2014
    Keywords: Astrophysics
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  • 57
    Publication Date: 2014-08-22
    Description: Author(s): Ken’ichiro Nakazato A new cellular automaton (CA) model is presented for the self-organized criticality (SOC) in recurrent bursts of soft gamma repeaters (SGRs), which are interpreted as avalanches of reconnection in the magnetosphere of neutron stars. The nodes of a regular dodecahedron and a truncated icosahedron are... [Phys. Rev. D 90, 043010] Published Thu Aug 21, 2014
    Keywords: Astrophysics
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  • 58
    Publication Date: 2014-09-25
    Description: Author(s): Y. Bai, A. J. Barger, V. Barger, R. Lu, A. D. Peterson, and J. Salvado We investigate whether a subset of high-energy events observed by IceCube may be due to neutrinos from Sagittarius A*. We check both spatial and temporal coincidences of IceCube events with other transient activities of Sagittarius A*. Among the seven IceCube shower events nearest to the Galactic ce... [Phys. Rev. D 90, 063012] Published Wed Sep 24, 2014
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  • 59
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    Publication Date: 2014-09-26
    Description: Author(s): Peng-Cheng Chu, Lie-Wen Chen, and Xin Wang Within the confined isospin- and density-dependent mass model, we study the properties of strange quark matter (SQM) and quark stars (QSs) in strong magnetic fields. The equation of state of SQM under a constant magnetic field is obtained self-consistently and the pressure perpendicular to the magne... [Phys. Rev. D 90, 063013] Published Thu Sep 25, 2014
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  • 60
    Publication Date: 2014-09-25
    Description: Author(s): Yanbei Chen, Linqing Wen, and Yiqiu Ma Extra-galactic sources of photons have been used to constrain space-time quantum fluctuations in the Universe. In these proposals, the fundamental “fuzziness” of distance caused by space-time quantum fluctuations has been directly identified with fluctuations in optical paths. Phase-front corrugatio... [Phys. Rev. D 90, 063011] Published Wed Sep 24, 2014
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  • 61
    Publication Date: 2014-11-25
    Description: Author(s): Guido W. Pettinari, Christian Fidler, Robert Crittenden, Kazuya Koyama, Antony Lewis, and David Wands We compute the cosmic microwave background (CMB) bispectrum induced by the evolution of the primordial density perturbations, including for the first time both temperature and polarization using a second-order Boltzmann code. We show that including polarization can increase the signal-to-noise by a ... [Phys. Rev. D 90, 103010] Published Mon Nov 24, 2014
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  • 62
    Publication Date: 2014-12-02
    Description: Author(s): Torsten Bringmann, Martin Vollmann, and Christoph Weniger The apparent gamma-ray excess in the Galactic center region and inner Galaxy has attracted considerable interest, notably because both its spectrum and its radial distribution are consistent with an interpretation in terms of annihilating dark matter particles with a mass of about 10–40 GeV. We conf... [Phys. Rev. D 90, 123001] Published Mon Dec 01, 2014
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  • 63
    Publication Date: 2014-09-03
    Description: Author(s): Mikhail E. Gusakov, Andrey I. Chugunov, and Elena M. Kantor In a previous paper [M. E. Gusakov, A. I. Chugunov, and E. M. Kantor, Phys. Rev. Lett. 112 , 151101 (2014)], we introduced a new scenario that explains the existence of rapidly rotating warm neutron stars (NSs) observed in low-mass x-ray binaries (LMXBs). Here it is described in more detail. The scen... [Phys. Rev. D 90, 063001] Published Tue Sep 02, 2014
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  • 64
    Publication Date: 2014-09-11
    Description: Author(s): G. Mazzolo, F. Salemi, M. Drago, V. Necula, C. Pankow, G. A. Prodi, V. Re, V. Tiwari, G. Vedovato, I. Yakushin, and S. Klimenko We estimated the sensitivity of the upcoming advanced ground-based gravitational-wave observatories (the LIGO, Virgo, and KAGRA interferometers) to coalescing intermediate mass black hole binaries (IMBHB). We added waveforms modeling the gravitational radiation emitted by IMBHBs to simulated data fr... [Phys. Rev. D 90, 063002] Published Wed Sep 10, 2014
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  • 65
    Publication Date: 2014-09-11
    Description: Author(s): W. F. Kao and Ing-Chen Lin We will study the cosmological evolutions of a Weyl-invariant de Rham, Gabadadze, and Tolley (dRGT) massive gravity theory with a general fiducial metric. In the unitary gauge, this model is equivalent to a massive gauge field coupled to the dRGT massive gravity model. The massive gravity terms will... [Phys. Rev. D 90, 063003] Published Wed Sep 10, 2014
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  • 66
    Publication Date: 2014-09-12
    Description: Author(s): Bohdan Novosyadlyj, Yurij Kulinich, and Maksym Tsizh We study the dynamical properties and space distribution of dark energy in the weak and strong gravitational fields caused by inhomogeneities of matter in the static world of galaxies and clusters. We show that the dark energy in the weak gravitational fields of matter density perturbations can cond... [Phys. Rev. D 90, 063004] Published Thu Sep 11, 2014
    Keywords: Astrophysics
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  • 67
    Publication Date: 2014-12-04
    Description: Author(s): Leandro Beraldo e Silva, Marcos Lima, Laerte Sodré, and Jérôme Perez We propose an association between the phase-space mixing level of a self-gravitating system and the indistinguishability of its constituents (stars or dark matter particles). This represents a refinement in the study of systems exhibiting incomplete violent relaxation. Within a combinatorial analysi... [Phys. Rev. D 90, 123004] Published Wed Dec 03, 2014
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  • 68
    Publication Date: 2014-12-17
    Description: Author(s): Matthew D. Kistler, Todor Stanev, and Hasan Yüksel The IceCube experiment recently detected the first flux of high-energy neutrinos in excess of atmospheric backgrounds. We examine whether these neutrinos originate from within the same extragalactic sources as ultrahigh energy cosmic rays. Starting from rather general assumptions about spectra and f... [Phys. Rev. D 90, 123006] Published Tue Dec 16, 2014
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  • 69
    Publication Date: 2014-10-15
    Description: Author(s): Tina Kahniashvili, Yurii Maravin, George Lavrelashvili, and Arthur Kosowsky If a primordial magnetic field in the Universe has nonzero helicity, the violation of parity symmetry results in nonzero correlations between cosmic microwave background temperature and B-mode polarization. In this paper we derive approximations to the relevant microwave background power spectra ari... [Phys. Rev. D 90, 083004] Published Tue Oct 14, 2014
    Keywords: Astrophysics
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  • 70
    Publication Date: 2014-10-15
    Description: Author(s): Hayato Shimabukuro, Kiyotomo Ichiki, Susumu Inoue, and Shuichiro Yokoyama Although the cosmological paradigm based on cold dark matter and adiabatic, nearly scale-invariant primordial fluctuations is consistent with a wide variety of existing observations, it has yet to be sufficiently tested on scales smaller than those of massive galaxies, and various alternatives have ... [Phys. Rev. D 90, 083003] Published Tue Oct 14, 2014
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  • 71
    Publication Date: 2014-10-15
    Description: Author(s): M. Coughlin, E. Thrane, and N. Christensen Compact binary coalescences are a promising source of gravitational waves for second-generation interferometric gravitational-wave detectors. Although matched filtering is the optimal search method for well-modeled systems, alternative detection strategies can be used to guard against theoretical er... [Phys. Rev. D 90, 083005] Published Tue Oct 14, 2014
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  • 72
    Publication Date: 2014-05-20
    Description: Author(s): Soumyajit Bose, Anindya Sengupta, and Arnab K. Ray We subject the stationary solutions of inviscid and axially symmetric rotational accretion to a time-dependent radial perturbation, which includes nonlinearity to any arbitrary order. Regardless of the order of nonlinearity, the equation of the perturbation bears a form that is similar to the metric... [Phys. Rev. D 89, 103011] Published Mon May 19, 2014
    Keywords: Astrophysics
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  • 73
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    Publication Date: 2014-05-21
    Description: Author(s): Massimo Giovannini This paper investigates the Faraday effect as a different source of B-mode polarization. The E-mode polarization is Faraday rotated provided a stochastic large-scale magnetic field is present prior to photon decoupling. In the first part of the paper we discuss the case where the tensor modes of the... [Phys. Rev. D 89, 103010] Published Tue May 20, 2014
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  • 74
    Publication Date: 2014-06-02
    Description: Author(s): Rajaram Nityananda and Sushan Konar We show that recently proposed white dwarf models with masses well in excess of the Chandrasekhar limit, based on modifying the equation of state by a superstrong magnetic field in the center, are very far from equilibrium because of the neglect of Lorentz forces. An upper bound on the central magne... [Phys. Rev. D 89, 103017] Published Fri May 30, 2014
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  • 75
    Publication Date: 2014-06-21
    Description: Author(s): Dipongkar Talukder, Eric Thrane, Sukanta Bose, and Tania Regimbau Galactic neutron stars are a promising source of gravitational waves in the analysis band of detectors such as Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo. Previous searches for gravitational waves from neutron stars have focused on the detection of individual neutron stars,... [Phys. Rev. D 89, 123008] Published Fri Jun 20, 2014
    Keywords: Astrophysics
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  • 76
    Publication Date: 2014-07-18
    Description: Author(s): Huan Yang and Marc Casals In this paper we study wave propagation and scattering near a black hole. In particular, we assume a coherent emission source near the black hole and investigate the wavefront distortion as seen by a distant observer. By ignoring the spin nature of the electromagnetic radiation we model it by a comp... [Phys. Rev. D 90, 023014] Published Thu Jul 17, 2014
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  • 77
    Publication Date: 2014-07-12
    Description: Author(s): Markus Ahlers and Kohta Murase The IceCube Collaboration has recently reported evidence for a high-energy extraterrestrial neutrino flux. During two years of operation 28 events with energies between 30 TeV and 1.2 PeV were observed while only 10.6 events were expected from conventional atmospheric backgrounds. The hadronic inter... [Phys. Rev. D 90, 023010] Published Fri Jul 11, 2014
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  • 78
    Publication Date: 2014-07-12
    Description: Author(s): Victor I. Denisov, Vladimir A. Sokolov, and Mikhail I. Vasili’ev The motion of x-ray and gamma-ray pulses in the magnetic field of the pulsar, taking into account the nonlinearity of electrodynamics in a vacuum, is calculated. It is shown that in these conditions, each pulse propagates in the form of two orthogonally polarized normal waves with different speeds. ... [Phys. Rev. D 90, 023011] Published Fri Jul 11, 2014
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  • 79
    Publication Date: 2014-07-12
    Description: Author(s): Domenico Sapone, Elisabetta Majerotto, and Savvas Nesseris We test the FLRW cosmology by reconstructing in a model-independent way both the Hubble parameter H(z) and the comoving distance D(z) via the most recent Hubble and Supernovae Ia data. In particular we use data binning with direct error propagation, the principal component analysis, the genetic algo... [Phys. Rev. D 90, 023012] Published Fri Jul 11, 2014
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  • 80
    Publication Date: 2014-07-12
    Description: Author(s): E. Thrane, N. Christensen, R. M. S. Schofield, and A. Effler One of the key science goals of advanced gravitational-wave detectors is to observe a stochastic gravitational-wave background. However, recent work demonstrates that correlated magnetic fields from Schumann resonances can produce correlated strain noise over global distances, potentially limiting t... [Phys. Rev. D 90, 023013] Published Fri Jul 11, 2014
    Keywords: Astrophysics
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  • 81
    Publication Date: 2014-02-19
    Description: Author(s): Michele Maggiore We discuss the cosmological consequences of a model based on a nonlocal infrared modification of Einstein equations. We find that the model generates a dynamical dark energy that can account for the presently observed value of ΩDE, without introducing a cosmological constant. Tuning a free mass para... [Phys. Rev. D 89, 043008] Published Tue Feb 18, 2014
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  • 82
    Publication Date: 2014-02-19
    Description: Author(s): Ariadna Montiel, Ruth Lazkoz, Irene Sendra, Celia Escamilla-Rivera, and Vincenzo Salzano In this work we present a nonparametric approach, which works on minimal assumptions, to reconstruct the cosmic expansion of the Universe. We propose to combine a locally weighted scatterplot smoothing method and a simulation-extrapolation method. The first one (LOESS) is a nonparametric approach th... [Phys. Rev. D 89, 043007] Published Tue Feb 18, 2014
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  • 83
    Publication Date: 2014-02-19
    Description: Author(s): Xiang-Nan Zhou, Xiao-Long Du, Ke Yang, and Yu-Xiao Liu Recently, a novel kind of scalar wigs around Schwarzschild black holes—scalar dynamical resonance states—was introduced in [Phys. Rev. D 84 , 083008 (2011)] and [Phys. Rev. Lett. 109 , 081102 (2012)]. In this paper, we investigate the existence and evolution of Dirac dynamical resonance states. First,... [Phys. Rev. D 89, 043006] Published Tue Feb 18, 2014
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  • 84
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    Publication Date: 2014-02-21
    Description: Author(s): Kent Yagi Gravitational-wave observations in the near future may allow us to measure tidal deformabilities of neutron stars, which leads us to the understanding of physics at nuclear density. In principle, the gravitational waveform depends on various tidal parameters, which correlate strongly. Therefore, it ... [Phys. Rev. D 89, 043011] Published Thu Feb 20, 2014
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  • 85
    Publication Date: 2014-03-21
    Description: Author(s): Seokcheon Lee, Guo-Chin Liu, and Kin-Wang Ng We study the imprint of a coupling of scalar dark energy to a photon on the cosmic microwave background polarization. Both the time-evolving field value and the perturbation of the scalar induce B-mode polarization. For a wide range of scalar dark energy models allowed by current observational data,... [Phys. Rev. D 89, 063010] Published Thu Mar 20, 2014
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  • 86
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    Publication Date: 2014-03-25
    Description: Author(s): Vincent Poitras According to a generalization of black hole thermodynamics to a cosmological framework, it is possible to define a temperature for the cosmological horizon. The hypothesis of thermal equilibrium between the dark energy and the horizon has been considered by many authors. We find the restrictions imp... [Phys. Rev. D 89, 063011] Published Mon Mar 24, 2014
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  • 87
    Publication Date: 2014-05-02
    Description: Author(s): Jacques M. Wagstaff, Robi Banerjee, Dominik Schleicher, and Günter Sigl In this paper we show that the Universe is already strongly magnetized at very early epochs during cosmic evolution. Our calculations are based on the efficient amplification of weak magnetic seed fields, which are unavoidably present in the early Universe, by the turbulent small-scale dynamo. We id... [Phys. Rev. D 89, 103001] Published Thu May 01, 2014
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  • 88
    Publication Date: 2014-05-01
    Description: Author(s): Andrew Pontzen I discuss fluctuations in the neutral hydrogen density of the z≈2.3 intergalactic medium and show that their relation to cosmic overdensity is strongly scale dependent. This behavior arises from a linearized version of the well-known “proximity effect,” in which bright sources suppress atomic hydrog... [Phys. Rev. D 89, 083010] Published Wed Apr 30, 2014
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  • 89
    Publication Date: 2014-05-01
    Description: Author(s): Esteban Calzetta and Alejandra Kandus We study the possibility that primordial magnetic fields generated in the transition between inflation and reheating posses magnetic helicity, HM. The fields are induced by stochastic currents of scalar charged particles created during the mentioned transition. We estimate the rms value of the induc... [Phys. Rev. D 89, 083012] Published Wed Apr 30, 2014
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  • 90
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    Publication Date: 2014-07-02
    Description: Author(s): Alessandro Manzotti, Wayne Hu, and Aurélien Benoit-Lévy Lensing of the cosmic microwave background by modes that are larger than the size of the survey dilates intrinsic scales in the temperature and polarization fields and coherently shifts their observed power spectra with respect to the ensemble or all-sky mean. The effect can be simply encapsulated a... [Phys. Rev. D 90, 023003] Published Tue Jul 01, 2014
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  • 91
    Publication Date: 2014-07-02
    Description: Author(s): S.-C. Su, Eugene A. Lim, and E. P. S. Shellard We study cosmological perturbations by solving the governing Boltzmann and Einstein field equations up to second order and calculate the corresponding CMB bispectrum during recombination. We include all the second-order Liouville and collision terms, truncating the multipole hierarchy at l=10, consi... [Phys. Rev. D 90, 023004] Published Tue Jul 01, 2014
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  • 92
    Publication Date: 2014-07-02
    Description: Author(s): A. Bauswein, N. Stergioulas, and H.-T. Janka We present a novel method for revealing the equation of state of high-density neutron star matter through gravitational waves emitted during the postmerger phase of a binary neutron star system. The method relies on a small number of detections of the peak frequency in the postmerger phase for binar... [Phys. Rev. D 90, 023002] Published Tue Jul 01, 2014
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  • 93
    Publication Date: 2014-07-02
    Description: Author(s): Dai G. Yamazaki, Motohiko Kusakabe, Toshitaka Kajino, Grant. J. Mathews, and Myung-Ki Cheoun The Li7 abundance calculated in BBN with the baryon-to-photon ratio fixed from fits to the CMB power spectrum is inconsistent with the observed lithium abundances on the surface of metal-poor halo stars. Previous cosmological solutions proposed to resolve this Li7 problem include photon cooling (pos... [Phys. Rev. D 90, 023001] Published Tue Jul 01, 2014
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  • 94
    Publication Date: 2014-06-21
    Description: Author(s): S.-C. Su and Eugene A. Lim The Planck mission has conclusively detected lensing of the cosmic microwave background (CMB) radiation from foreground sources to an overall significance of greater than 25σ [1]. The high precision of this measurement motivates the development of a more complete formulation of the calculation of th... [Phys. Rev. D 89, 123006] Published Fri Jun 20, 2014
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  • 95
    Publication Date: 2014-07-01
    Description: Author(s): Justin P. DeAndrea and Kevin M. Alexander We model the supermassive Galactic center of the Milky Way Galaxy as a strongly naked singularity lens described by the Janis–Newman–Winicour metric. This metric has an ordinary mass and massless scalar charge parameters. For very accurate results, we use the Virbhadra–Ellis lens equation for comput... [Phys. Rev. D 89, 123012] Published Mon Jun 30, 2014
    Keywords: Astrophysics
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  • 96
    Publication Date: 2014-03-18
    Description: Author(s): Hajime Takami, Koutarou Kyutoku, and Kunihito Ioka We study high-energy emission from the mergers of neutron star binaries as electromagnetic counterparts to gravitational waves aside from short gamma-ray bursts. The mergers entail significant mass ejection, which interacts with the surrounding medium to produce similar but brighter remnants than su... [Phys. Rev. D 89, 063006] Published Mon Mar 17, 2014
    Keywords: Astrophysics
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  • 97
    Publication Date: 2014-03-18
    Description: Author(s): Ranjan Laha and John F. Beacom Detecting supernova νe is essential for testing supernova and neutrino physics, but the yields are small and the backgrounds from other channels large, e.g., ∼ 102 and ∼ 104 events, respectively, in Super-Kamiokande. We develop a new way to isolate supernova νe, using gadolinium-loaded water Cherenk... [Phys. Rev. D 89, 063007] Published Mon Mar 17, 2014
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  • 98
    Publication Date: 2014-03-19
    Description: Author(s): H. F. Gruetjen and E. P. S. Shellard Strong foreground contamination in high resolution CMB data requires masking which introduces statistical anisotropies and renders a full maximum likelihood analysis numerically intractable. Standard analysis methods like the pseudo-Cl framework lead to information loss due to estimator suboptimalit... [Phys. Rev. D 89, 063008] Published Tue Mar 18, 2014
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  • 99
    Publication Date: 2014-04-05
    Description: Author(s): Luis A. Anchordoqui, Haim Goldberg, Morgan H. Lynch, Angela V. Olinto, Thomas C. Paul, and Thomas J. Weiler Very recently the IceCube Collaboration has reported an observation of 28 neutrino candidates with energies between 50 TeV and 2 PeV, constituting a 4.1σ excess compared to the atmospheric background. In this article we investigate the compatibility between the data and a hypothesized unbroken power... [Phys. Rev. D 89, 083003] Published Fri Apr 04, 2014
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  • 100
    Publication Date: 2014-04-18
    Description: Author(s): Juan Barranco, Argelia Bernal, Juan Carlos Degollado, Alberto Diez-Tejedor, Miguel Megevand, Miguel Alcubierre, Darío Núñez, and Olivier Sarbach Using the Green’s function representation technique, the late time behavior of localized scalar field distributions on Schwarzschild spacetimes is studied. Assuming arbitrary initial data we perform a spectral analysis, computing the amplitude of each excited quasibound mode without the necessity of... [Phys. Rev. D 89, 083006] Published Thu Apr 17, 2014
    Keywords: Astrophysics
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