Zobrazeno 1 - 10
of 32
pro vyhledávání: '"Fiorella Burgio"'
Publikováno v:
Universe, Vol 6, Iss 8, p 115 (2020)
We study the cooling of isolated neutron stars with particular regard to the importance of nuclear pairing gaps. A microscopic nuclear equation of state derived in the Brueckner-Hartree-Fock approach is used together with compatible neutron and proto
Externí odkaz:
https://doaj.org/article/2770861c154a4dd1b8c0f9554055bee1
The International Symposium on “Exotic States of Nuclear Matter” was a unique opportunity to review and discuss the many aspects of nuclear matter under extreme conditions and the corresponding possible exotic states like hyperonic matter, kaon c
Publikováno v:
Physical Review D. 103
We investigate radial oscillations of pure neutron stars and hybrid stars, employing equations of state of nuclear matter from Brueckner-Hartree-Fock theory, and of quark matter from the Dyson-Schwinger quark model, performing a Gibbs construction fo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6a1d0bad2249e7ac284462783f6f44eb
https://doi.org/10.1103/physrevd.103.103003
https://doi.org/10.1103/physrevd.103.103003
Publikováno v:
Symmetry, Vol 13, Iss 400, p 400 (2021)
Symmetry
Volume 13
Issue 3
Symmetry
Volume 13
Issue 3
Background: We analyze several constraints on the nuclear equation of state (EOS) currently available from neutron star (NS) observations and laboratory experiments and study the existence of possible correlations among properties of nuclear matter a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::801abb236d5f2b61152a81fe35c6331c
https://www.mdpi.com/2073-8994/13/3/400
https://www.mdpi.com/2073-8994/13/3/400
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
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instname
arXiv:1904.13060v2
We show that the pulsar mass depends on the environment, and that it decreases going towards the centre of the Milky Way. This is due to two combined effects, the capture and accumulation of self-interacting, non-annihilating
We show that the pulsar mass depends on the environment, and that it decreases going towards the centre of the Milky Way. This is due to two combined effects, the capture and accumulation of self-interacting, non-annihilating
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3ca21d30dd8fbed55ba3a468f51e1dbc
http://hdl.handle.net/20.500.11769/483988
http://hdl.handle.net/20.500.11769/483988
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
The European Physical Society Conference on High Energy Physics (EPS-HEP), 10-17 July 2019 Ghent, Belgium.
We discuss the formation of dark compact objects in a dark matter environment in view of the possible mass dependence of pulsars on the di
We discuss the formation of dark compact objects in a dark matter environment in view of the possible mass dependence of pulsars on the di
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::84ea10b489ecd8cb15356d841c83878b
Publikováno v:
Proceedings of XIII Quark Confinement and the Hadron Spectrum — PoS(Confinement2018).
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d102ede59ef51d732c937879ca5b5201
https://doi.org/10.22323/1.336.0203
https://doi.org/10.22323/1.336.0203
Autor:
Maksym Deliyergiyev, Antonino Del Popolo, Xiguo Lee, Fiorella Burgio, Morgan Le Delliou, Laura Tolos
We study the structure of compact objects that contain non-self annihilating, self-interacting dark matter admixed with ordinary matter made of neutron star and white dwarf materials. We extend the previous work Phys. Rev. D 92 123002 (2015) on these
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aca1519e544c853d285855c66c3c436f
http://hdl.handle.net/20.500.11769/363342
http://hdl.handle.net/20.500.11769/363342
Autor:
G. Fiorella Burgio, Isaac Vidaña
Publikováno v:
Universe, Vol 6, Iss 119, p 119 (2020)
Background. We investigate possible correlations between neutron star observables and properties of atomic nuclei. In particular, we explore how the tidal deformability of a 1.4 solar mass neutron star, M1.4, and the neutron-skin thickness of 48Ca an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f7c2fe524058c490dd176239b1400f59
https://doi.org/10.3390/universe6080119
https://doi.org/10.3390/universe6080119
Autor:
G. Fiorella Burgio, Anthea Fantina
Publikováno v:
The Physics and Astrophysics of Neutron Stars ISBN: 9783319976150
The Physics and Astrophysics of Neutron Stars
Luciano Rezzolla, Pierre Pizzochero, David Ian Jones, Nanda Rea, Isaac Vidaña. The Physics and Astrophysics of Neutron Stars, 457, Springer, pp.255-335, 2018, Astrophysics and Space Science Library, ⟨10.1007/978-3-319-97616-7_6⟩
The Physics and Astrophysics of Neutron Stars
Luciano Rezzolla, Pierre Pizzochero, David Ian Jones, Nanda Rea, Isaac Vidaña. The Physics and Astrophysics of Neutron Stars, 457, Springer, pp.255-335, 2018, Astrophysics and Space Science Library, ⟨10.1007/978-3-319-97616-7_6⟩
International audience; The equation of state (EoS) of hot and dense matter is a fundamental input to describe static and dynamical properties of neutron stars, core-collapse supernovae and binary compact-star mergers. We review the current status of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::647fac6d2fbc3f9884b0a77c58472555
https://doi.org/10.1007/978-3-319-97616-7_6
https://doi.org/10.1007/978-3-319-97616-7_6