Articles Citing

Possible binary neutron star merger history of the primary of GW230529

Parthapratim Mahapatra ^1,2,*, Debatri Chattopadhyay ^2,3, Anuradha Gupta ⁴, Fabio Antonini ², Marc Favata ⁵, B. S. Sathyaprakash ^6,7, and K. G. Arun ¹

¹Chennai Mathematical Institute, Siruseri, 603103, India
²School of Physics and Astronomy, Cardiff University, Cardiff, CF24 3AA, United Kingdom
³Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA) and Department of Physics and Astronomy, Northwestern University, 1800 Sherman Ave, Evanston, Illinois 60201, USA
⁴Department of Physics and Astronomy, The University of Mississippi, University, Mississippi 38677, USA
⁵Department of Physics and Astronomy, Montclair State University, 1 Normal Avenue, Montclair, New Jersey 07043, USA
⁶Institute for Gravitation and the Cosmos, Department of Physics, Penn State University, University Park, Pennsylvania 16802, USA
⁷Department of Astronomy and Astrophysics, Penn State University, University Park, Pennsylvania 16802, USA

^*Contact author: MahapatraP@cardiff.ac.uk

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Articles Citing

Possible binary neutron star merger history of the primary of GW230529

Challenging a binary neutron star merger interpretation of GW230529

Impact of uncertainty in the compact binary population on source classification

Black-hole–neutron-star mergers: New numerical-relativity simulations and multipolar effective-one-body model with spin precession and eccentricity

On a local study of star boundaries

Characterizing Compact-object Binaries in the Lower Mass Gap with Gravitational Waves

Can Premature Collapse Form Black Holes in the Upper and Lower Mass Gaps?

Testing the nature of compact objects in the lower mass gap using gravitational wave observations

Distinguishing prompt-collapse binary neutron star mergers from binary black holes: Tidal effects and remnant properties

Identifying Proca-star mergers via consistent ultralight-boson mass estimates across gravitational-wave events

GW241011 and GW241110: Exploring Binary Formation and Fundamental Physics with Asymmetric, High-spin Black Hole Coalescences

First Eccentric Inspiral–Merger–Ringdown Analysis of Neutron Star–Black Hole Mergers

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