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  • 1
    Electronic Resource
    Electronic Resource
    Springer
    Il nuovo cimento della Società Italiana di Fisica 11 (1989), S. 303-319 
    ISSN: 0392-6737
    Keywords: Classical and semiclassical techniques ; Functional analytical methods
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Description / Table of Contents: Riassunto Si mostra come una descrizione funzionale del problema nucleare a molti corpi possa fornire uno schema unificato per trattare i vari aspetti del problema e stabilire ben definite procedure di approssimazione. Si considera in particolare l'approssimazione perturbativa e di campo medio per un'esatta lagrangiana bosonica effettiva, discutendo in quale modo possono essere ottenuti ben noti schemi di calcolo («hole-line expansion, RPA», ecc.) come sottoinsiemi di ordine definito in questi sviluppi. È poi presentata un'applicazione al calcolo della funzione di risposta elettromagnetica longitudinale con interazioneNπ. Si mostra come la dinamica pionica e le correlazioni a corta distanza contribuiscono all'ottenimento di un migliore accordo con i dati sperimentali.
    Abstract: Резюме Мы показнваем, как функциональный подход к ядерной провлеме многих тел может дать единую схему рассмотрения проблемы с многими гранями и установления хорошо опрелённых процедур приближения. В частности, мы рассматриваем пертурбационные приблизения и приближения среднего поля (петельное разложение) для эффективного бозонного Лагранжиана. Мы обсуждаем, как хорошо известные схемы вычисления могут быть получены, как подмножества определённых порядков в этих разложениях. Проводится вычисление функции продольного электромагнитного отклика в лучае простогоNπ взаимодействия. Мы показываем, как динамика пионов и короткодействующие корреляции способствуют получению лучшего согласия с экспериментальными данными.
    Notes: Summary We show how a functional approach to the nuclear many-body problem can provide a unified scheme to deal with the many facets of the problem and to establish well-defined procedures of approximation. We consider, in particular, the perturbative and the mean-field (loop expansion) approximations to an exact effective bosonic Lagrangian, discussing how well-known computational schemes (hole-line expansion, RPA, etc.) may be obtained as subsets of definite orders in these expansions. An application to the calculation of the longitudinal electromagnetic response function, with the simpleNπ interaction, is finally presented. We show how the pion dynamic and the short-range correlations cooperate to obtain a better agreement with experimental data.
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Amsterdam : Elsevier
    Nuclear Physics, Section A 487 (1988), S. 279-300 
    ISSN: 0375-9474
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Physics
    Type of Medium: Electronic Resource
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  • 3
    Electronic Resource
    Electronic Resource
    Amsterdam : Elsevier
    Annals of Physics 174 (1987), S. 131-168 
    ISSN: 0003-4916
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Physics
    Type of Medium: Electronic Resource
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  • 4
    Electronic Resource
    Electronic Resource
    Amsterdam : Elsevier
    Physics Letters B 246 (1990), S. 315-319 
    ISSN: 0370-2693
    Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002
    Topics: Physics
    Type of Medium: Electronic Resource
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  • 5
    Electronic Resource
    Electronic Resource
    Springer
    Few body systems 17 (1994), S. 21-61 
    ISSN: 1432-5411
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The connection between light-cone dynamics and field theory is analyzed in detail within the zero-range approximation, with particular attention to the so-called “angular condition”. New and detailed calculations for the elastic form factors of the deuteron are presented for the Bonn, Paris, Reid Soft-Core, Argonne V14 and one-pion-exchange potentials with various choices of the electromagnetic form factors of the nucleon.
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  • 6
    Electronic Resource
    Electronic Resource
    Springer
    The European physical journal 77 (1989), S. 491-495 
    ISSN: 1434-6036
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The dynamics of a quantum particle moving in a tight binding lattice and coupled to an ohmic heat bath is investigated. Imaginary-time functional integral methods are utilized to determine the self-energy of the velocity-velocity correlation function for weak damping and arbitrary temperatures. Recent results for the linear mobility atT=0 and high temperatures are confirmed and extended to intermediate temperatures. The dominant corrections to the zero temperature mobility are given in terms of a power law.
    Type of Medium: Electronic Resource
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  • 7
    Publication Date: 1990-10-01
    Print ISSN: 0031-9007
    Electronic ISSN: 1079-7114
    Topics: Physics
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  • 8
    Publication Date: 2015-10-30
    Description: We present the first estimate of age, stellar metallicity and chemical abundance ratios, for an individual early-type galaxy at high-redshift ( z = 1.426) in the COSMOS (Cosmological Evolution Survey) field. Our analysis is based on observations obtained with the X-Shooter instrument at the Very Large Telescope (VLT), which cover the visual and near-infrared spectrum at high ( R 〉 5000) spectral resolution. We measure the values of several spectral absorptions tracing chemical species, in particular magnesium and iron, besides determining the age-sensitive D4000 break. We compare the measured indices to stellar population models, finding good agreement. We find that our target is an old ( t 〉 3 Gyr), high-metallicity ([ Z /H] 〉 0.5) galaxy which formed its stars at z form 〉5 within a short time-scale ~0.1 Gyr, as testified by the strong [α/Fe] ratio (〉0.4), and has passively evolved in the first 〉3–4 Gyr of its life. We have verified that this result is robust against the choice and number of fitted spectral features, and stellar population model. The result of an old age and high-metallicity has important implications for galaxy formation and evolution confirming an early and rapid formation of the most massive galaxies in the Universe.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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  • 9
    Publication Date: 2014-03-25
    Description: We present a high signal-to-noise ratio (S/N 〉 10) medium-resolution ( R  = 2000) Large Binocular Telescope/LUCIFER spectrum of the early-type galaxy (ETG) S2F1-142 at z ~= 1.4. By means of the CaT line at 8662 Å, we measured its redshift z  = 1.386 ± 0.001 and we estimated its velocity dispersion $\sigma _{v}=340^{-60}_{+120}$  km s –1 . Its corresponding virial mass is 3.9 10 11  M , compatible with the stellar mass estimates obtained assuming initial mass functions (IMFs) less dwarf rich than the Salpeter one. S2F1-142 is a compact galaxy with R e = 3.1 ± 0.2 kpc, i.e. an effective radius more than three times smaller than the average R e of ETGs with the same mass in the local Universe. At the same time, we found local and high-redshift galaxies with a similar mass content and similar effective radius confirming that it is fully consistent with the already available measures of R e and v both in the local and in the distant Universe. Considering the distribution of R e and v as a function of the stellar mass content of ETGs, both in the local and in the distant Universe, we noticed that the measured velocity dispersions of the more compact galaxies are on average slightly lower than expected on the basis of their compactness and the virial theorem, suggesting that (i) their dark matter content is lower than in the more diffuse galaxies and/or (ii) their luminosity profiles are steeper than in the more diffuse galaxies and/or (iii) their larger compactness is an apparent effect caused by the overestimate of their stellar mass content (due to bottom lighter IMF and/or systematic affecting the stellar mass estimates).
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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  • 10
    Publication Date: 2014-09-10
    Description: We present a spectroscopic analysis based on measurements of two mainly age-dependent spectrophotometric indices in the 4000 Å rest-frame region, i.e. H+K(Ca ii ) and 4000, for a sample of 15 early-type galaxies (ETGs) at 0.7 〈 z spec 〈 1.1, morphologically selected in the GOODS-South field. Ages derived from the two different indices by means of the comparison with stellar population synthesis models are not consistent with each other for at least nine galaxies (60 per cent of the sample), while for the remaining six galaxies, the ages derived from their global spectral energy distribution (SED) fitting are not consistent with those derived from the two indices. We then hypothesized that the stellar content of many galaxies is made of two stellar components with different ages. The double-component analysis, performed by taking into account both the index values and the observed SED, fully explains the observational data and improves the results of the standard one-component SED fitting in 9 out of the 15 objects, i.e. those for which the two indices point towards two different ages. In all of them, the bulk of the mass belongs to rather evolved stars, while a small mass fraction is many Gyr younger. In some cases, thanks to the sensitivity of the H+K(Ca ii ) index, we find that the minor younger component reveals signs of recent star formation. The distribution of the ages of the younger stellar components appears uniformly in time and this suggests that small amounts of star formation could be common during the evolution of high- z ETGs. We argue the possibility that these new star formation episodes could be frequently triggered by internal causes due to the presence of small gas reservoir.
    Print ISSN: 0035-8711
    Electronic ISSN: 1365-2966
    Topics: Physics
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