Zobrazeno 1 - 10
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pro vyhledávání: '"Constantinou C"'
Autor:
Miglior, F., author, Pinotti, L., author, Boyle, L., author, Kenny, D., author, Lee, M., author, De Marchi, M., author, Cadavez, V.A.P., author, Millet, S., author, Evans, R., author, Veldkamp, T., author, Pastell, M., author, Pollott, G., author, Spoolder, H., author, Tzamaloukas, O., author, Neofytou, M.C., author, Constantinou, C., author, Symeou, S., author, Sparaggis, D., author, Miltiadou, D., author
Publikováno v:
Book of Abstracts of the 73rd Annual Meeting of the European Federation of Animal Science. :362-362
In this work, we examine in detail the difference between constraining the electric charge fraction and isospin fraction when calculating the deconfinement phase transition in the presence of net strangeness. We present relations among charge and iso
Externí odkaz:
http://arxiv.org/abs/2010.00996
Publikováno v:
Phys. Rev. D 102, 076016 (2020)
We investigate the phase transition from hadron to quark matter in the general case without the assumption of chemical equilibrium. The effects of net strangeness on charge and isospin fractions, chemical potentials, and temperature are studied in th
Externí odkaz:
http://arxiv.org/abs/2004.03039
Akademický článek
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Publikováno v:
Phys. Rev. D 100, 103022 (2019)
Neutron star interiors provide the opportunity to probe properties of cold dense matter in the QCD phase diagram. Utilizing models of dense matter in accord with nuclear systematics at nuclear densities, we investigate the compatibility of deconfined
Externí odkaz:
http://arxiv.org/abs/1906.04095
Publikováno v:
Phys. Rev. C 100, 025803 (2019)
Differences in the equation of state (EOS) of dense matter translate into differences in astrophysical simulations and their multi-messenger signatures. Thus, extending the number of EOSs for astrophysical simulations allows us to probe the effect of
Externí odkaz:
http://arxiv.org/abs/1901.09652
The influence of thermal fluctuations on fermion pairing is investigated using a semiclassical treatment of fluctuations. When the average pairing gaps along with those differing by one standard deviation are used, the characteristic discontinuity of
Externí odkaz:
http://arxiv.org/abs/1812.09988
In this work, we study matter in the cores of proto-neutron stars, focusing on the impact of their composition on the stellar structure. We begin by examining the effects of finite temperature (through a fixed entropy per baryon) and lepton fraction
Externí odkaz:
http://arxiv.org/abs/1812.08157
In simulations of binary neutron star mergers, the dense matter equation of state (EOS) is required over wide ranges of density and temperature as well as under conditions in which neutrinos are trapped, and the effects of magnetic fields and rotatio
Externí odkaz:
http://arxiv.org/abs/1809.08126
Publikováno v:
Phys. Rev. C 97, 064324 (2018)
Exploiting the similarity between the bunched single-particle energy levels of nuclei and of random distributions around the Fermi surface, pairing properties of the latter are calculated to establish statistically-based bounds on the basic character
Externí odkaz:
http://arxiv.org/abs/1705.09351