Zobrazeno 1 - 10
of 37
pro vyhledávání: '"Rana Nandi"'
Autor:
Sreemoyee Sarkar, Rana Nandi
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 84, Iss 9, Pp 1-14 (2024)
Abstract We examine bulk viscosity, taking into account trapped neutrinos in baryonic matter, in the context of binary neutron star mergers. Following the merging event, the binary star can yield a remnant compact object with densities up to 5 nuclea
Externí odkaz:
https://doaj.org/article/2d2cb39944424991a5c3ebd534faafed
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 82, Iss 6, Pp 1-8 (2022)
Abstract The occurrence of quark matter at the center of neutron stars is still in debate. This study defines some semi-empirical parameters that try to quantify the presence and the amount of quark matter at star interiors. We find that one needs un
Externí odkaz:
https://doaj.org/article/9a8efde1fd8248fe9c0690fdeff580d8
Publikováno v:
Universe, Vol 8, Iss 7, p 380 (2022)
The effect of isospin-dependent nuclear forces on the inner crust of neutron stars is modeled within the framework of Quantum Molecular Dynamics (QMD). To successfully control the density dependence of the symmetry energy of neutron-star matter below
Externí odkaz:
https://doaj.org/article/4b7340790af64dadb83bc8229bedd762
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 505:1600-1606
We show that the odds of the mass-gap (secondary) object in GW190814 being a neutron star (NS) improve if one allows for a stiff high-density equation of state (EoS) or a large spin. Since its mass is $\in (2.50,2.67) M_{\odot}$, establishing its tru
Autor:
Rana Nandi, Subrata Pal
Publikováno v:
The European Physical Journal Special Topics. 230:551-559
The detection of gravitational waves from GW170817 has provided a new opportunity to constrain the equation of state (EOS) of neutron stars. In this article, we investigate the possible existence of quarks inside the neutron star core in the context
Publikováno v:
Physical Review C. 104
In the present work we study the effects of strongly quantizing magnetic fields and finite temperature on the properties of inner crusts of hot neutron stars. In particular, we study the effects of Landau quantization of electrons on the composition
Publikováno v:
European Physical Journal
The occurrence of quark matter at the center of neutron stars is still in debate. This study defines some semi-empirical parameters that quantify the occurrence and the amount of quark matter at star interiors. These parameters show semi-universal re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9aca8d3ee40329cd3dd065481005218f
This article studies the maximum mass limit of the quark star formed after the shock-induced phase transition of a cold neutron star. By employing hadronic and quark equation of state that satisfies the current mass bound, we use combustion adiabat c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4bc748a59d2cd92ac392c01e8d0b013f
http://arxiv.org/abs/2012.04212
http://arxiv.org/abs/2012.04212
Autor:
Rana Nandi, P. K. Manoharan, Debades Bandhopadhay, Avishek Basu, Bhal Chandra Joshi, Dipankar Bhattacharya, Prasanta Char, M A Krishnakumar
The abrupt change in the pulse period of a pulsar is called a pulsar glitch. In this paper, we present eleven pulsar glitches detected using the Ooty Radio Telescope (ORT) and the upgraded Giant Metrewave Radio Telescope (uGMRT) in high cadence timin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4be4c480dac7a27524cf7a1df0c215a4
http://arxiv.org/abs/1911.04934
http://arxiv.org/abs/1911.04934
Publikováno v:
Physical Review C. 99
The first detection of gravitational waves from the binary neutron star merger event GW170817 has started to provide important new constraints on the nuclear equation of state at high density. The tidal deformability bound of GW170817 combined with t