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Published in 2017 at "Astronomische Nachrichten"
DOI: 10.1002/asna.201713441
Abstract: Although the detailed structure of neutron stars remains unknown, their equilibrium temperatures lie well below the Fermi temperature of dense nuclear matter, suggesting that the nucleons in the stars' core form Cooper pairs and exhibit…
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Keywords:
star cores;
fluxtube dynamics;
dynamics neutron;
neutron star ... See more keywords
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Published in 2019 at "Astronomische Nachrichten"
DOI: 10.1002/asna.201913579
Abstract: Since 2013 the mass of pulsar PSR J0348+0432 ($M = 2.01\,M_{\odot}$) has provided a tight constraint on neutron star equation of state. However, a number of different analyses of the recently detected BNS merger (GW170817)…
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Keywords:
matter light;
mass;
neutron star;
star matter ... See more keywords
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Published in 2024 at "Astronomische Nachrichten"
DOI: 10.1002/asna.20240096
Abstract: We model the duration of the propeller stage in wide binary systems with neutron stars and calculate the time of accretion onset for various propeller models. We apply our modeling to the symbiotic X‐ray binary…
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Keywords:
neutron star;
propeller stage;
propeller;
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Published in 2024 at "Astronomische Nachrichten"
DOI: 10.1002/asna.20240098
Abstract: A0538‐66 is a neutron star/Be x‐ray binary located in the Large Magellanic Cloud and, since its discovery in the 70s, it showed a peculiar behavior that makes it a unique object in the high‐mass x‐ray…
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Keywords:
ray binary;
neutron star;
xmm newton;
newton observations ... See more keywords
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Published in 2025 at "Astronomische Nachrichten"
DOI: 10.1002/asna.20240150
Abstract: To model the structure of neutron stars (NSs) theoretically, it is common to consider layers with different density regimes. Matching the equation of state (EoS) for the crust and core and obtaining a suitable description…
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Keywords:
crust core;
crust;
neutron star;
interpolation ... See more keywords
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Published in 2024 at "Contributions to Plasma Physics"
DOI: 10.1002/ctpp.202400004
Abstract: Crystallization of dense matter in neutron star crusts and white dwarf cores may be similar to epitaxial crystal growth in terrestrial laboratories. However, in stellar crystals, the spacing between horizontal planes has to gradually increase…
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Keywords:
crusts white;
star crusts;
dwarf cores;
neutron star ... See more keywords
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Published in 2017 at "Journal of High Energy Physics"
DOI: 10.1007/jhep06(2018)036
Abstract: A bstractIn certain models of a QCD axion, finite density corrections to the axion potential can result in the axion being sourced by large dense objects. There are a variety of ways to test this…
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Keywords:
inspirals stellar;
axions neutron;
probing axions;
axion ... See more keywords
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Published in 2020 at "Astrophysics and Space Science"
DOI: 10.1007/s10509-020-3745-3
Abstract: The results of the investigation of the core-envelope model presented in Negi et al. (Gen. Relativ. Gravit. 22:735, 1990 ) have been discussed in view of the reference (Negi et al. in Gen. Relativ. Gravit.…
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Keywords:
relativ gravit;
gen relativ;
negi gen;
neutron star ... See more keywords
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Published in 2024 at "Astrophysics and Space Science"
DOI: 10.1007/s10509-024-04281-y
Abstract: Neutron star low-mass X-ray binaries accrete via Roche-lobe overflow from a stellar companion that is ≲ 1 M⊙. The accretion disk in these systems can be externally illuminated by X-rays that are reprocessed by the…
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Keywords:
neutron star;
low mass;
star low;
mass ray ... See more keywords
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Published in 2020 at "General Relativity and Gravitation"
DOI: 10.1007/s10714-020-02714-x
Abstract: The first multimessenger observation of a binary neutron star (BNS) merger in August 2017 demonstrated the huge scientific potential of these extraordinary events. This breakthrough led to a number of discoveries and provided the best…
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Keywords:
magnetic fields;
neutron star;
binary neutron;
merger ... See more keywords
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Published in 2017 at "Journal of Astrophysics and Astronomy"
DOI: 10.1007/s12036-017-9473-6
Abstract: G. Srinivasan et al. (1990) proposed a simple and elegant explanation for the reduction of the neutron star magnetic dipole moment during binary evolution leading to low mass X-ray binaries and eventually to millisecond pulsars:…
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Keywords:
evolution;
neutron star;
flux vortex;
vortex pinning ... See more keywords