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Observing Supernova Neutrino Light Curves with Super-Kamiokande. V. Distance Estimation with Neutrinos
Published 2025-01-01Subjects: Get full text
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22
Intersections of ultracold atomic polarons and nuclear clusters: how is a chart of nuclides modified in dilute neutron matter?
Published 2024-02-01Subjects: Get full text
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23
Striking a Chord with Spectral Sirens: Multiple Features in the Compact Binary Population Correlate with H0
Published 2025-01-01Subjects: Get full text
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24
On the Use of Galaxy Catalogs in Gravitational-wave Parameter Estimation
Published 2025-01-01Subjects: Get full text
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25
A New X-Ray and Radio Burst Activity from the Magnetar SGR 1935+2154
Published 2025-01-01Subjects: Get full text
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26
Giant Hall Waves Launched by Superconducting Phase Transition in Pulsars
Published 2025-01-01Subjects: Get full text
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27
X-Ray Dips and Polarization Angle Swings in GX 13+1
Published 2025-01-01Subjects: Get full text
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28
Black Hole Supernovae, Their Equation of State Dependence, and Ejecta Composition
Published 2025-01-01Subjects: Get full text
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29
Imaging and Spectral Fitting of Bright Gamma-Ray Sources with the COSI Balloon Payload
Published 2025-01-01Subjects: Get full text
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30
Astrophysical Aspects of Neutrino Dynamics in Ultradegenerate Quark Gluon Plasma
Published 2017-01-01“…The cardinal focus of the present review is to explore the role of neutrinos originating from the ultradense core of neutron stars composed of quark gluon plasma in the astrophysical scenario. …”
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31
Strangeness in Astrophysics
Published 2025-01-01“…In this contribution the role of strangeness in astrophysics is discussed and, more precisely, strange hadronic matter in the interior of neutron stars. A special attention is payed to certain phenomena involving strange hadronic matter, such as the hyperon puzzle, kaon condensation and the thermal behaviour of hyperons in neutron star mergers.…”
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32
Can Effects of a Generalized Uncertainty Principle Appear in Compact Stars?
Published 2024-12-01“…The corresponding results for the equation of state and the mass-radius relation for neutron stars are in tune with recent observations with a maximum mass around 2.5 M<sub>⊙</sub> and radius close to 12 km. …”
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33
Dark I-Love-Q
Published 2025-02-01“…Abstract For neutron stars, there exist universal relations insensitive to the equation of states, the so called I-Love-Q relations, which show the connections among the moment of inertia, tidal Love number and quadrupole moment. …”
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34
Star shearing season: transient signals in wave-like dark matter experiments from black hole formation
Published 2025-02-01“…Abstract Ordinary matter coupled to light weakly interacting bosons can lead to the formation of a macroscopic bosonic field in the vicinity of large matter concentrations such as ordinary or neutron stars. When these objects are turned into black holes due to a supernova or a binary merger this “hair” could be “shorn” off. …”
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35
Strong-field QED effects on polarization states in dipole and quadrudipole pulsar emissions
Published 2024-12-01“…Abstract Highly magnetized neutron stars have quantum refraction effects on pulsar emission due to the non-linearity of the quantum electrodynamics (QED) action. …”
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36
Predicting Pulsars from Imbalanced Dataset with Hybrid Resampling Approach
Published 2021-01-01“…Pulsar stars, usually neutron stars, are spherical and compact objects containing a large quantity of mass. …”
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37
Kilonova/Macronova Emission from Compact Binary Mergers
Published 2016-01-01“…We review current understanding of kilonova/macronova emission from compact binary mergers (mergers of two neutron stars or a neutron star and a black hole). Kilonova/macronova is emission powered by radioactive decays of r-process nuclei and it is one of the most promising electromagnetic counterparts of gravitational wave sources. …”
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38
Aspects of rotating anisotropic dark energy stars
Published 2024-12-01“…We also find that the dimensionless quadrupole moments of anisotropic dark energy stars corresponding to the canonical mass $${\bar{q}}_{1.4}$$ q ¯ 1.4 have a similar range of values as that of isotropic neutron stars and strange stars.…”
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39
The stability of anisotropic compact stars influenced by dark matter under teleparallel gravity: an extended gravitational deformation approach
Published 2025-02-01“…To validate our findings, we compare our model predictions with observational constraints, including GW190814 (with a mass range of $$2.5-2.67 M_{\odot }$$ 2.5 - 2.67 M ⊙ ) and neutron stars (NSTRs) such as EXO 1785-248 [mass= $$1.3_{-0.2}^{+0.2}~M_{\odot }$$ 1 . 3 - 0.2 + 0.2 M ⊙ ], 4U 1608-52 [mass= $$1.74_{-0.14}^{+0.14}~M_{\odot }$$ 1 . 74 - 0.14 + 0.14 M ⊙ ], and PSR J0952-0607 [mass= $$2.35_{-0.17}^{+0.17}~M_{\odot }$$ 2 . 35 - 0.17 + 0.17 M ⊙ ]. …”
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40
Distinguishing Compact Objects in Extreme-Mass-Ratio Inspirals by Gravitational Waves
Published 2025-01-01“…Therefore, our findings suggest that it is possible to distinguish primordial black holes from white dwarfs, and, under certain conditions, neutron stars can also be differentiated from primordial black holes.…”
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