Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Rahul Somasundaram"'
Autor:
Peter T. H. Pang, Tim Dietrich, Michael W. Coughlin, Mattia Bulla, Ingo Tews, Mouza Almualla, Tyler Barna, Ramodgwendé Weizmann Kiendrebeogo, Nina Kunert, Gargi Mansingh, Brandon Reed, Niharika Sravan, Andrew Toivonen, Sarah Antier, Robert O. VandenBerg, Jack Heinzel, Vsevolod Nedora, Pouyan Salehi, Ritwik Sharma, Rahul Somasundaram, Chris Van Den Broeck
Publikováno v:
Nature Communications, Vol 14, Iss 1, Pp 1-13 (2023)
Abstract The multi-messenger detection of the gravitational-wave signal GW170817, the corresponding kilonova AT2017gfo and the short gamma-ray burst GRB170817A, as well as the observed afterglow has delivered a scientific breakthrough. For an accurat
Externí odkaz:
https://doaj.org/article/83e0219b0d0541b699d4f33d76fa54fd
Publikováno v:
The Astrophysical Journal Letters, Vol 962, Iss 1, p L3 (2024)
The equation of state (EOS) of dense strongly interacting matter can be probed by astrophysical observations of neutron stars (NS), such as X-ray detections of pulsars or the measurement of the tidal deformability of NSs during the inspiral stage of
Externí odkaz:
https://doaj.org/article/10169cb09ca240f8b37bb77865d423ab
Autor:
Brendan T. Reed, Rahul Somasundaram, Soumi De, Cassandra L. Armstrong, Pablo Giuliani, Collin Capano, Duncan A. Brown, Ingo Tews
Publikováno v:
The Astrophysical Journal, Vol 974, Iss 2, p 285 (2024)
Gravitational-wave observations of binary neutron-star (BNS) mergers have the potential to revolutionize our understanding of the nuclear equation of state (EOS) and the fundamental interactions that determine its properties. However, Bayesian parame
Externí odkaz:
https://doaj.org/article/ae4ca65748ef48dc8785b6682c81110f
Publikováno v:
Physical Review C. 105
A compressible liquid-drop model (CLDM) is used to correlate uncertainties associated with the properties of the neutron star (NS) crust with theoretical estimates of the uncertainties associated with the equation of state (EOS) of homogeneous neutro
Publikováno v:
The European Physical Journal A. 58
We explore three different classes of relativistic approaches applied to the description of dense nuclear matter: a Walecka-type relativistic mean field model (RMF), an extension including an effective chiral potential (RMF-C) and a further extension
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::49709eb6c9f5ff317c3d4f30f1a94a17
http://arxiv.org/abs/2109.05374
http://arxiv.org/abs/2109.05374
Publikováno v:
Physical Review D. 102
We study the weak decay of the ${\mathrm{\ensuremath{\Lambda}}}_{b}$ baryon into $J/\ensuremath{\psi}\ensuremath{\phi}\mathrm{\ensuremath{\Lambda}}$, a process that is particularly well suited to analyze the physics of some of the recently observed o