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  • 1
    Publication Date: 2015-09-11
    Description: Hydrodynamical simulations of galaxy formation such as the Illustris simulations have progressed to a state where they approximately reproduce the observed stellar mass function from high to low redshift. This in principle allows self-consistent models of reionization that exploit the accurate representation of the diffuse gas distribution together with the realistic growth of galaxies provided by these simulations, within a representative cosmological volume. In this work, we apply and compare two radiative transfer algorithms implemented in a GPU-accelerated code to the 106.5-Mpc-wide volume of Illustris in post-processing in order to investigate the reionization transition predicted by this model. We find that the first generation of galaxies formed by Illustris is just about able to reionize the universe by redshift z  ~ 7, provided quite optimistic assumptions about the escape fraction and the resolution limitations are made. Our most optimistic model finds an optical depth of ~= 0.065, which is in very good agreement with recent Planck 2015 determinations. Furthermore, we show that moment-based approaches for radiative transfer with the M1 closure give broadly consistent results with our angular-resolved radiative transfer scheme. In our favoured fiducial model, 20 per cent of the hydrogen is reionized by redshift z  = 9.20, and this rapidly climbs to 80 per cent by redshift z  = 6.92. It then takes until z  = 6.24 before 99 per cent of the hydrogen is ionized. On average, reionization proceeds ‘inside-out’ in our models, with a size distribution of reionized bubbles that progressively features regions of ever larger size while the abundance of small bubbles stays fairly constant.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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  • 2
    Publication Date: 2015-09-27
    Description: Hydrodynamical simulations of galaxy formation such as the Illustris simulations have progressed to a state where they approximately reproduce the observed stellar mass function from high to low redshift. This in principle allows self-consistent models of reionization that exploit the accurate representation of the diffuse gas distribution together with the realistic growth of galaxies provided by these simulations, within a representative cosmological volume. In this work, we apply and compare two radiative transfer algorithms implemented in a GPU-accelerated code to the 106.5-Mpc-wide volume of Illustris in post-processing in order to investigate the reionization transition predicted by this model. We find that the first generation of galaxies formed by Illustris is just about able to reionize the universe by redshift z  ~ 7, provided quite optimistic assumptions about the escape fraction and the resolution limitations are made. Our most optimistic model finds an optical depth of ~= 0.065, which is in very good agreement with recent Planck 2015 determinations. Furthermore, we show that moment-based approaches for radiative transfer with the M1 closure give broadly consistent results with our angular-resolved radiative transfer scheme. In our favoured fiducial model, 20 per cent of the hydrogen is reionized by redshift z  = 9.20, and this rapidly climbs to 80 per cent by redshift z  = 6.92. It then takes until z  = 6.24 before 99 per cent of the hydrogen is ionized. On average, reionization proceeds ‘inside-out’ in our models, with a size distribution of reionized bubbles that progressively features regions of ever larger size while the abundance of small bubbles stays fairly constant.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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  • 3
    Publication Date: 2014-09-26
    Description: We present an overview of galaxy evolution across cosmic time in the Illustris simulation. Illustris is an N -body/hydrodynamical simulation that evolves 2 1820 3 resolution elements in a (106.5 Mpc) 3 box from cosmological initial conditions down to z  = 0 using the arepo moving-mesh code. The simulation uses a state-of-the-art set of physical models for galaxy formation that was tuned to reproduce the z  = 0 stellar mass function and the history of the cosmic star formation rate density. We find that Illustris successfully reproduces a plethora of observations of galaxy populations at various redshifts, for which no tuning was performed, and provide predictions for future observations. In particular, we discuss (a) the buildup of galactic mass, showing stellar mass functions and the relations between stellar mass and halo mass from z  = 7 to 0, (b) galaxy number density profiles around massive central galaxies out to z  = 4, (c) the gas and total baryon content of both galaxies and their haloes for different redshifts, and as a function of mass and radius, and (d) the evolution of galaxy specific star formation rates up to z  = 8. In addition, we (i) present a qualitative analysis of galaxy morphologies from z  = 5 to 0, for the stellar as well as the gaseous components, and their appearance in Hubble Space Telescope mock observations, (ii) follow galaxies selected at z  = 2 to their z  = 0 descendants, and quantify their growth and merger histories, and (iii) track massive z  = 0 galaxies to high redshift and study their joint evolution in star formation activity and compactness. We conclude with a discussion of several disagreements with observations, and lay out possible directions for future research.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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  • 4
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 184 (1959), S. 44-45 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] From the data of Opik3 one finds that a particle-size distribution peaking in the fractional mm. range, as observed for Worzel's ash, could indeed be obtained by ablation of mm.- to cm.-sized particles. However, a cometary or asteroidal origin of the ash is unlikely for a number of reasons. If the ...
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    Springer
    Fish physiology and biochemistry 10 (1992), S. 23-34 
    ISSN: 1573-5168
    Keywords: Protein synthesis ; liver ; trout ; Oncorhynchus mykiss ; feeding
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology
    Notes: Abstract The response of protein synthesis in the liver of the rainbow trout to feeding and fasting was investigated in 3 experiments. In the first experiment, the fractional rate of protein synthesis (k s ), %/day) appeared to cycle with daily feeding events being increased by 46%, 123%, and 72% at 1.5h, 3h, and 6h, after a meal. In Experiment 2, liver protein synthesis fell progressively with fasting to a basal level at 4d which was only 20% of the value at 3h after feeding. Liver weight (hepatosomatic index, HSI, % body weight), total RNA and total protein also fell gradually. Between 4d and 6d, both the RNA/protein ratio and the rate of protein synthesis were significantly increased (11% and 74%). At this time, however, there was also a large loss of liver protein suggesting a concomitant increase in protein breakdown. In the last experiment, when trout were pre-fed a low ration (0.6%/d for 2 wks, LR group), the HSI and liver total RNA and protein were largely unaffected by the 6d fast (i.e., relative to the body weight). In this group, however, protein synthesis at 3h was significantly higher than in fish pre-fed a high ration (1.5%/d, HR group). In addition, at 6d after feeding, protein synthesis had increased back to fed levels in the LR group only. It is concluded that protein synthesis in the liver of the trout is influenced both by feeding events and by ration size and also by the degree to which the trout is fasted.
    Type of Medium: Electronic Resource
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  • 6
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    In:  Science, Jena, Physica-Verlag, vol. 298, no. 5596, pp. 1219-1221, pp. L24313, (ISSN: 1340-4202)
    Publication Date: 2002
    Keywords: Seismology ; China ; Plate tectonics ; Subduction zone ; Receiver functions
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  • 7
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    Am. Geophys. Un.
    In:  Bull., Polar Proj. OP-O3A4, Continental Lithosphere: Deep Seismic Reflections, Washington, D.C., Am. Geophys. Un., vol. 22, no. Subvol. a, pp. 377-382, (ISBN 0080419208)
    Publication Date: 1991
    Keywords: Deep seismic sounding (espec. cont. crust) ; Earth model, also for more shallow analyses ! ; GeodesyY ; Plate tectonics ; Review article ; Meissner ; Duerbaum ; Durbaum
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  • 8
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    In:  Bull. Seism. Soc. Am., Tokyo, Railway Tech. Res. Inst., vol. 80, no. 4, pp. 395-410, pp. L06615, (ISSN: 1340-4202)
    Publication Date: 1990
    Keywords: Seismology ; AUD ; Hypocenter determination ; Travel time ; BSSA
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  • 9
    Publication Date: 2015-11-26
    Description: Author(s): Bryan Kaufman, Pran Nath, Brent D. Nelson, and Andrew B. Spisak Light stops consistent with the Higgs boson mass of ∼ 126     GeV are investigated within the framework of minimal supergravity. It is shown that models with light stops which are also consistent with the thermal relic density constraints require stop coannihilation with the neutralino LSP. The analysis… [Phys. Rev. D 92, 095021] Published Mon Nov 23, 2015
    Keywords: Beyond the Standard Model
    Print ISSN: 0556-2821
    Electronic ISSN: 1089-4918
    Topics: Physics
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  • 10
    Publication Date: 2015-06-02
    Description: Author(s): Erik D. Nelson and Nick V. Grishin Protein evolution is frequently explored using minimalist polymer models, however, little attention has been given to the problem of structural drift, or diffusion. Here, we study neutral evolution of small protein motifs using an off-lattice heteropolymer model in which individual monomers interact... [Phys. Rev. E 91, 060701(R)] Published Mon Jun 01, 2015
    Keywords: Biological Physics
    Print ISSN: 1539-3755
    Electronic ISSN: 1550-2376
    Topics: Physics
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