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pro vyhledávání: '"Krastev, Plamen"'
Autor:
Krastev, Plamen G.
Understanding the equation of state of dense QCD matter remains a major challenge in both nuclear physics and astrophysics. Neutron star observations from electromagnetic and gravitational wave spectra provide critical insights into the behavior of d
Externí odkaz:
http://arxiv.org/abs/2303.17146
The Laser Interferometer Gravitational-Wave Observatory (LIGO) and Virgo Interferometer Collaborations have now detected all three classes of compact binary mergers: binary black hole (BBH), binary neutron star (BNS), and neutron star-black hole (NSB
Externí odkaz:
http://arxiv.org/abs/2210.15888
Autor:
Krastev, Plamen G.
Publikováno v:
Galaxies 2022, 10(1), 16
One of the most significant challenges involved in efforts to understand the equation of state of dense neutron-rich matter is the uncertain density dependence of the nuclear symmetry energy. Because of its broad impact, pinning down the density depe
Externí odkaz:
http://arxiv.org/abs/2112.04089
Autor:
Krastev, Plamen.
Thesis (Ph. D.)--University of Idaho, 2006.
"August, 2006." Includes bibliographical references (leaves 113-122). Also available online in PDF format.
"August, 2006." Includes bibliographical references (leaves 113-122). Also available online in PDF format.
Externí odkaz:
http://proquest.umi.com/pqdweb?did=1246570461&sid=1&Fmt=2&clientId=58634&RQT=309&VName=PQD
Publikováno v:
Phys. Lett. B 815, 136161 (2021)
One of the key challenges of real-time detection and parameter estimation of gravitational waves from compact binary mergers is the computational cost of conventional matched-filtering and Bayesian inference approaches. In particular, the application
Externí odkaz:
http://arxiv.org/abs/2012.13101
Autor:
Krastev, Plamen G.
Publikováno v:
Phys. Lett. B 803, 135330 (2020)
The groundbreaking discoveries of gravitational waves from binary black-hole mergers and, most recently, coalescing neutron stars started a new era of Multi-Messenger Astrophysics and revolutionized our understanding of the Cosmos. Machine learning t
Externí odkaz:
http://arxiv.org/abs/1908.03151
Publikováno v:
Euro. Phys. J. A 55: 117 (2019)
Determining the Equation of State (EOS) of dense neutron-rich nuclear matter is a shared goal of both nuclear physics and astrophysics. Except possible phase transitions, the density dependence of nuclear symmetry \esym is the most uncertain part of
Externí odkaz:
http://arxiv.org/abs/1905.13175
Autor:
Krastev, Plamen G., Li, Bao-An
Publikováno v:
J. Phys. G: Nucl. Part. Phys. 46 074001 (2019)
Applying an equation of state (EOS) with its symmetric nuclear matter (SNM) contribution and low-density symmetry energy $E_{sym}(\rho)$ constrained by heavy-ion reaction data, we calculate the dimensionless tidal deformability $\Lambda$ of neutron s
Externí odkaz:
http://arxiv.org/abs/1801.04620
Autor:
Krastev, Plamen G., Li, Bao-An
The recent direct detection of gravitational waves (GWs) from binary black hole mergers (2016, Phys. Rev. Lett. 116, no. 6, 061102; no. 24, 241103) opens up an entirely new non-electromagnetic window into the Universe making it possible to probe phys
Externí odkaz:
http://arxiv.org/abs/1607.05373
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