Zobrazeno 1 - 10
of 67
pro vyhledávání: '"velocity: acoustic"'
Publikováno v:
Journal of High Energy Physics
Journal of high energy physics 08(8), 302 (2022). doi:10.1007/JHEP08(2022)302
Journal of high energy physics 08(8), 302 (2022). doi:10.1007/JHEP08(2022)302
Journal of high energy physics 08(8), 302 (2022). doi:10.1007/JHEP08(2022)302
The energy budget for gravitational waves of a cosmological first order phase transitions depends on the speed of sound in the thermal plasma in both phases around the
The energy budget for gravitational waves of a cosmological first order phase transitions depends on the speed of sound in the thermal plasma in both phases around the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::76075f95cba03f058562041d6ed98cb6
http://arxiv.org/abs/2206.01130
http://arxiv.org/abs/2206.01130
Autor:
Chavanis, Pierre-Henri
Publikováno v:
Phys.Rev.D
Phys.Rev.D, 2022, 106 (6), pp.063525. ⟨10.1103/PhysRevD.106.063525⟩
Phys.Rev.D, 2022, 106 (6), pp.063525. ⟨10.1103/PhysRevD.106.063525⟩
International audience; We introduce a new logotropic model based on a complex scalar field with a logarithmic potential that unifies dark matter and dark energy. The scalar field satisfies a nonlinear wave equation generalizing the Klein-Gordon equa
Autor:
Rho, Mannque
The answer is found in the way the hidden scale symmetry involving a dilaton emerges in strong nuclear correlations in nuclear matter. It is suggested that the same mechanism is at the origin at higher densities of the sound speed converging in the c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c905590b13a6886675c155c6eac8245d
http://arxiv.org/abs/2204.08190
http://arxiv.org/abs/2204.08190
Publikováno v:
Physical review / D 105(5), 054011 (2022). doi:10.1103/PhysRevD.105.054011
Physical Review
Physical Review
We extend the effective dynamical quasiparticle model (DQPM) - constructed for the description of non-perturbative QCD phenomena of the strongly interacting quark-gluon plasma (QGP) - to large baryon chemical potentials, $\mu_B$, including a critical
Autor:
Renaux-Petel, Sébastien
Publikováno v:
European Physical Society Conference on High Energy Physics 2021
European Physical Society Conference on High Energy Physics 2021, Jul 2021, Online, Germany
proceedings of the European Physical Society Conference on High Energy Physics
Proceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2021)
European Physical Society Conference on High Energy Physics 2021, Jul 2021, Online, Germany
proceedings of the European Physical Society Conference on High Energy Physics
Proceedings of The European Physical Society Conference on High Energy Physics — PoS(EPS-HEP2021)
A new class of inflationary attractors characterized by a strongly non-geodesic motion has been discovered and explored in the past few years. I describe how they naturally arise in negatively curved field space, allowing to inflate on potentials tha
Publikováno v:
Journal of cosmology and astroparticle physics 04(04), 010 (2022). doi:10.1088/1475-7516/2022/04/010
Journal of cosmology and astroparticle physics 04(04), 010 (2022). doi:10.1088/1475-7516/2022/04/010
We revisit the computation of bubble wall friction during a cosmological first-order phase transition, using an extended fluid Ansatz to solve t
We revisit the computation of bubble wall friction during a cosmological first-order phase transition, using an extended fluid Ansatz to solve t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::750e148633099f3916f7bddd07f7adcb
https://bib-pubdb1.desy.de/record/478391
https://bib-pubdb1.desy.de/record/478391
The energy budget for gravitational waves of a cosmological first order phase transitions depends on the speed of sound in the thermal plasma in both phases around the bubble wall. Working in the real-singlet augmented Standard Model, which admits a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fa6641e9e026ced62da348e54aad6364
Publikováno v:
Mod.Phys.Lett.A
Mod.Phys.Lett.A, 2022, 37 (03), pp.2230003. ⟨10.1142/S0217732322300038⟩
Mod.Phys.Lett.A, 2022, 37 (03), pp.2230003. ⟨10.1142/S0217732322300038⟩
We review how the "cusp" predicted in the nuclear symmetry energy generated by a topology change at density $n_{1/2}\gsim 2 n_0$ can have a surprising consequence, so far unrecognized in nuclear physics and astrophysics communities, on the structure
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d56f3ca67d8a7c03ecd023ff6f5b20c6
https://hal.science/hal-03287208
https://hal.science/hal-03287208
Publikováno v:
Universe; Volume 8; Issue 9; Pages: 468
We propose a new class of cosmological unified dark sector models called "{\em Generalized Logotropic Models}". They depend on a free parameter $n$. The original logotropic model [P.H. Chavanis, Eur. Phys. J. Plus {\bf 130}, 130 (2015)] is a special
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bcf60f31f68a2b325c3ec3e2631bc5b9
http://arxiv.org/abs/2112.13318
http://arxiv.org/abs/2112.13318
Publikováno v:
Journal of High Energy Physics, Vol 2021, Iss 11, Pp 1-16 (2021)
Journal of High Energy Physics
JHEP
JHEP, 2021, 11, pp.063. ⟨10.1007/JHEP11(2021)063⟩
Journal of High Energy Physics
JHEP
JHEP, 2021, 11, pp.063. ⟨10.1007/JHEP11(2021)063⟩
Gravitinos can inherit a non-relativistic dispersion relation while propagating in a background breaking both supersymmetry and Lorentz symmetry spontaneously. This is because the longitudinal mode velocity is controlled by the sound speed in the bac