Zobrazeno 1 - 10
of 5 350
pro vyhledávání: '"H, Dinh"'
Publikováno v:
A&A 687, A44 (2024)
Relating different global neutron-star (NS) properties, such as tidal deformability and radius, or mass and radius, requires an equation of state (EoS). Determining the NS EoS is therefore not only the science goal of a variety of observational proje
Externí odkaz:
http://arxiv.org/abs/2406.14906
Publikováno v:
Eur. Phys. J. A 59, 292 (2023)
Being born hot from core-collapse supernova, the crust of the proto-neutron star is expected to be made of a Coulomb liquid and composed of an ensemble of different nuclear species. In this work, we study the beta-equilibrated proto-neutron-star crus
Externí odkaz:
http://arxiv.org/abs/2309.01533
Publikováno v:
A&A 677, A174 (2023)
Proto-neutron stars (PNS) are born hot, with temperatures exceeding a few times $10^{10}$ K. In these conditions, the PNS crust is expected to be made of a Coulomb liquid composed of an ensemble of different nuclear species. We perform a study of the
Externí odkaz:
http://arxiv.org/abs/2309.01527
Akademický článek
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Publikováno v:
A&A 672, A160 (2023)
The crust of a neutron star is known to melt at a temperature that increases with increasing matter density, up to about $10^{10}$ K. At such high temperatures and beyond, the crustal ions are put into collective motion and the associated entropy con
Externí odkaz:
http://arxiv.org/abs/2304.01584
Autor:
Lan H. Dang, Khanh N. Thach, Yen T. Nguyen, Tuyen V. Nguyen, Ha H. Dinh, Loan T. Nguyen, Cuc T. Nguyen
Publikováno v:
Interdisciplinary Neurosurgery, Vol 37, Iss , Pp 101979- (2024)
Background and purpose: Minimally invasive surgery for ICH has shown a significantly improved functional outcome for selected ICH patients. This study aimed to evaluate the factors influencing the outcome of supratentorial ICH patients treated with s
Externí odkaz:
https://doaj.org/article/7ee0ebee23594291b0fb9f19974ed547
Publikováno v:
IL NUOVO CIMENTO 45 C (2022) 62
Exotic non-spherical configurations of nuclei, known as ``pasta" phases, are expected to be present at the bottom of the inner crust of a neutron star. We study the properties of these configurations in catalyzed neutron stars within a compressible l
Externí odkaz:
http://arxiv.org/abs/2206.07969
In the transition from nuclear matter to finite nuclei, complex finite-size effects which characterise open systems arise, in relation with either the nuclear surface or the bulk. In addition, the non-equilibrium character of the process, typical of
Externí odkaz:
http://arxiv.org/abs/2203.13736
Akademický článek
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Publikováno v:
Eur. Phys. J. A 57, 296 (2021)
Nuclear pasta, that is an inhomogeneous distribution of nuclear matter characterised by non-spherical clustered structures, is expected to occur in a narrow spatial region at the bottom of the inner crust of neutron stars, but the width of the pasta
Externí odkaz:
http://arxiv.org/abs/2111.04374