Probing the impact of WIMP dark matter on universal relations, GW170817 posterior, and radial oscillations
P Routaray, A Quddus, K Chakravarti… - Monthly Notices of the …, 2023 - academic.oup.com
In this study, we investigate the impact of weakly interacting massive particles (WIMPs) dark
matter (DM) on C–Λ universal relations, GW170817 posterior, and radial oscillations of …
matter (DM) on C–Λ universal relations, GW170817 posterior, and radial oscillations of …
The role of magnetar transient activity in time-domain and multimessenger astronomy
Time-domain and multimessenger astronomy (TDAMM) involves the study of transient and
time-variable phenomena across various wavelengths and messengers. The Astro2020 …
time-variable phenomena across various wavelengths and messengers. The Astro2020 …
Systematic analysis of the impacts of symmetry energy parameters on neutron star properties
The impacts of various symmetry energy parameters on the properties of neutron stars (NSs)
have been recently investigated, and the outcomes are at variance, as summarized in Table …
have been recently investigated, and the outcomes are at variance, as summarized in Table …
Constraining nuclear parameters using Gravitational waves from f-mode Oscillations in Neutron Stars
BK Pradhan, D Pathak, D Chatterjee - The Astrophysical Journal, 2023 - iopscience.iop.org
Gravitational waves (GWs) emanating from unstable quasi-normal modes in neutron stars
(NSs) could be accessible with the improved sensitivity of the current GW detectors or with …
(NSs) could be accessible with the improved sensitivity of the current GW detectors or with …
Impact of updated multipole Love numbers and -Love universal relations in the context of binary neutron stars
Neutron star (NS) equation of state (EoS) insensitive relations or universal relations (UR)
involving neutron star bulk properties play a crucial role in gravitational-wave astronomy …
involving neutron star bulk properties play a crucial role in gravitational-wave astronomy …
Investigating dark matter-admixed neutron stars with NITR equation of state in light of PSR J0952-0607
The fastest and heaviest pulsar, PSR J0952-0607, with a mass of M= 2.35±0.17 M⊙, has
recently been discovered in the disk of the Milky Way Galaxy. In response to this discovery, a …
recently been discovered in the disk of the Milky Way Galaxy. In response to this discovery, a …
Framework for phase transitions between the Maxwell and Gibbs constructions
C Constantinou, T Zhao, S Han, M Prakash - Physical Review D, 2023 - APS
By taking the nucleon-to-quark phase transition within a neutron star as an example, we
present a thermodynamically consistent method to calculate the equation of state of ambient …
present a thermodynamically consistent method to calculate the equation of state of ambient …
Establishing connection between neutron star properties and nuclear matter parameters through a comprehensive multivariate analysis
We have attempted to mitigate the challenge of connecting the neutron star (NS) properties
with the nuclear matter parameters that describe equations of state (EOSs). The efforts to …
with the nuclear matter parameters that describe equations of state (EOSs). The efforts to …
Mixed dark matter models for the peculiar compact object in remnant HESS and their implications for gravitational wave properties
B Hong, ZZ Ren - Physical Review D, 2024 - APS
A recent assessment of the central compact object in the supernova remnant HESS J 1731-
347 [Nat. Astron. 6, 1444 (2022) 2397-3366 10.1038/s41550-022-01800-1] reveals its …
347 [Nat. Astron. 6, 1444 (2022) 2397-3366 10.1038/s41550-022-01800-1] reveals its …
Frequencies of - and -oscillation modes in cold and hot compact stars
A large collection of equations of state (EOSs) built within the covariant density functional
theory of hadronic matter and allowing for density dependent couplings is employed to study …
theory of hadronic matter and allowing for density dependent couplings is employed to study …