Publicaciones (27) Publicaciones de Prasanta Char

2024

  1. 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

  1. Generalized description of neutron star matter with a nucleonic relativistic density functional

    Physical Review D, Vol. 108, Núm. 10

  2. Radial oscillations of neutron stars with antikaon condensate

    European Physical Journal A, Vol. 59, Núm. 9

  3. Stability and instability of strange dwarfs

    Astronomy and Astrophysics, Vol. 678

2022

  1. Speed of sound in dense matter and two families of compact stars

    Astronomy and Astrophysics, Vol. 660

2021

  1. 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

  2. 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

  1. A Bayesian Analysis on Neutron Stars within Relativistic Mean Field Models

    Particles, Vol. 3, Núm. 3, pp. 621-629

  2. Bayesian Inference of Dense Matter Equation of State within Relativistic Mean Field Models Using Astrophysical Measurements

    Astrophysical Journal, Vol. 897, Núm. 2

  3. Effect of superfluid matter of a neutron star on the tidal deformability

    Physical Review D, Vol. 101, Núm. 6

  4. Observed glitches in eight young pulsars

    Monthly Notices of the Royal Astronomical Society, Vol. 491, Núm. 3, pp. 3182-3191

  5. Role of antikaon condensation on the universality relations of hot and rapidly rotating neutron stars

    Journal of Physics: Conference Series

  6. Structure of Quark Star: A Comparative Analysis of Bayesian Inference and Neural Network Based Modeling

    Astrophysical Journal, Vol. 905, Núm. 1

2019

  1. Constraining Strangeness in Dense Matter with GW170817

    Astrophysical Journal, Vol. 877, Núm. 2

  2. Constraining the relativistic mean-field model equations of state with gravitational wave observations

    Physical Review C, Vol. 99, Núm. 5

  3. 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

  4. Properties of massive rotating protoneutron stars with hyperons: Structure and universality

    Journal of Physics G: Nuclear and Particle Physics, Vol. 46, Núm. 10

  5. Role of crustal physics in the tidal deformation of a neutron star

    Physical Review D, Vol. 100, Núm. 4

2018

  1. Glitch Behavior of Pulsars and Contribution from Neutron Star Crust

    Astrophysical Journal, Vol. 866, Núm. 2

  2. Hybrid Stars in the Light of GW170817

    Astrophysical Journal, Vol. 857, Núm. 1