Zobrazeno 1 - 10
of 17
pro vyhledávání: '"Mateusz Cierniak"'
Publikováno v:
Particles, Vol 6, Iss 2, Pp 470-484 (2023)
In this study, we discuss how iterative solutions of QCD-inspired gap-equations at the finite chemical potential demonstrate domains of chaotic behavior as well as non-chaotic domains, which represent one or the other of the only two—usually distin
Externí odkaz:
https://doaj.org/article/d139c5638c87436689a47fbdcfa9e39c
Publikováno v:
Universe, Vol 5, Iss 8, p 186 (2019)
We construct a set of equations of state (EoS) of dense and hot matter with a 1st order phase transition from a hadronic system to a deconfined quark matter state. In this two-phase approach, hadrons are described using the relativistic mean field th
Externí odkaz:
https://doaj.org/article/758eefb53833475b86fbf56bde7828b4
Publikováno v:
Universe, Vol 4, Iss 2, p 30 (2018)
A commonly applied quark matter model in astrophysics is the thermodynamic bag model (tdBAG). The original MIT bag model approximates the effect of quark confinement, but does not explicitly account for the breaking of chiral symmetry, an important p
Externí odkaz:
https://doaj.org/article/25cc281c635a472fa1aa24bdcfca2170
Autor:
Noshad Khosravi Largani, Tobias Fischer, Armen Sedrakian, Mateusz Cierniak, David E Alvarez-Castillo, David B Blaschke
Publikováno v:
Web of Science
Several global parameters of compact stars are related via empirical relations, which are (nearly) independent of the underlying equation of state (EoS) of dense matter and, therefore, are said to be universal. We investigate the universality of rela
Autor:
Mateusz Cierniak, David Blaschke
Publikováno v:
The European Physical Journal Special Topics. 229:3663-3673
We show the existence and investigate the location of the special point (SP) in which hybrid neutron star mass-radius (M-R) curves have to cross each other when they belong to a class of hybrid equation of state (EoS) constructed with generic constan
Autor:
Mateusz Cierniak, David Blaschke
Publikováno v:
EPJ Web of Conferences, Vol 258, p 07009 (2022)
The special point is a feature unique to models of hybrid neutron stars. It represents a location on their mass--radius sequences that is insensitive to the phase transition density. We consider hybrid neutron stars with a core of deconfined quark ma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6d4338ec469b5e6200693efa3c982111
http://arxiv.org/abs/2112.09166
http://arxiv.org/abs/2112.09166
Autor:
David Blaschke, Mateusz Cierniak
We present a systematic investigation of the possible locations for the special point (SP), a unique feature of hybrid neutron stars in the mass-radius. The study is performed within the two-phase approach where the high-density (quark matter) phase
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::29aad75afe460e22f75aa9d045b1373f
Autor:
David Blaschke, Mateusz Cierniak
With the first multi-messenger observation of a binary neutron star merger (GW170817) new constraints became available for masses and radii of neutron stars. We introduce a class of hybrid EoS that fulfils all these constraints and predicts a region
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::163a931e319b134f78f80704cc541a2c
http://arxiv.org/abs/2012.15785
http://arxiv.org/abs/2012.15785
Autor:
Niels-Uwe F. Bastian, Nikolaos Stergioulas, David Blaschke, James A. Clark, Katerina Chatziioannou, Mateusz Cierniak, Tobias Fischer, Andreas Bauswein, Vimal Vijayan, Sebastian Blacker
Publikováno v:
Physical Review Letters
Physical review letters 125(14), 141103 (2020). doi:10.1103/PhysRevLett.125.141103
Physical review letters 125(14), 141103 (2020). doi:10.1103/PhysRevLett.125.141103
Using hydrodynamical simulations for a large set of high-density matter equations of state (EoSs) we systematically determine the threshold mass M_thres for prompt black-hole formation in equal-mass and asymmetric neutron star (NS) mergers. We devise
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4db5f681ea28ac9482cced459847861b
http://arxiv.org/abs/2004.00846
http://arxiv.org/abs/2004.00846
Autor:
David Blaschke, Tobias Fischer, Gerd Röpke, Stefan Typel, Mateusz Cierniak, Niels-Uwe F. Bastian, Matthias Hempel, Gabriel Martínez-Pinedo, William G. Newton, Thomas Klähn
In this review article we discuss selected developments regarding the role of the equation of state (EOS) in simulations of core-collapse supernovae. There are no first-principle calculations of the state of matter under supernova conditions since a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a7096ace6400bd400cf6e1fb4ea2c25e