Prasanta
Char
Publicacións (27) Publicacións de Prasanta Char
2024
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Observation of Gravitational Waves from the Coalescence of a 2.5–4.5Me Compact Object and a Neutron Star
Astrophysical Journal Letters, Vol. 970, Núm. 2
2023
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Generalized description of neutron star matter with a nucleonic relativistic density functional
Physical Review D, Vol. 108, Núm. 10
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Radial oscillations of neutron stars with antikaon condensate
European Physical Journal A, Vol. 59, Núm. 9
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Stability and instability of strange dwarfs
Astronomy and Astrophysics, Vol. 678
2022
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Speed of sound in dense matter and two families of compact stars
Astronomy and Astrophysics, Vol. 660
2021
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GW190814: On the properties of the secondary component of the binary
Monthly Notices of the Royal Astronomical Society, Vol. 505, Núm. 2, pp. 1600-1606
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Towards mitigation of apparent tension between nuclear physics and astrophysical observations by improved modeling of neutron star matter
Physical Review D, Vol. 103, Núm. 10
2020
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A Bayesian Analysis on Neutron Stars within Relativistic Mean Field Models
Particles, Vol. 3, Núm. 3, pp. 621-629
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Bayesian Inference of Dense Matter Equation of State within Relativistic Mean Field Models Using Astrophysical Measurements
Astrophysical Journal, Vol. 897, Núm. 2
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Effect of superfluid matter of a neutron star on the tidal deformability
Physical Review D, Vol. 101, Núm. 6
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Observed glitches in eight young pulsars
Monthly Notices of the Royal Astronomical Society, Vol. 491, Núm. 3, pp. 3182-3191
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Role of antikaon condensation on the universality relations of hot and rapidly rotating neutron stars
Journal of Physics: Conference Series
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Structure of Quark Star: A Comparative Analysis of Bayesian Inference and Neural Network Based Modeling
Astrophysical Journal, Vol. 905, Núm. 1
2019
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Constraining Strangeness in Dense Matter with GW170817
Astrophysical Journal, Vol. 877, Núm. 2
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Constraining the relativistic mean-field model equations of state with gravitational wave observations
Physical Review C, Vol. 99, Núm. 5
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How to Test the Two-Families Scenario
XIAMEN-CUSTIPEN WORKSHOP ON THE EQUATION OF STATE OF DENSE NEUTRON-RICH MATTER IN THE ERA OF GRAVITATIONAL WAVE ASTRONOMY
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Properties of massive rotating protoneutron stars with hyperons: Structure and universality
Journal of Physics G: Nuclear and Particle Physics, Vol. 46, Núm. 10
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Role of crustal physics in the tidal deformation of a neutron star
Physical Review D, Vol. 100, Núm. 4
2018
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Glitch Behavior of Pulsars and Contribution from Neutron Star Crust
Astrophysical Journal, Vol. 866, Núm. 2
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Hybrid Stars in the Light of GW170817
Astrophysical Journal, Vol. 857, Núm. 1