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Physical Review D

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Phys. Rev. D (2)

Articles Citing

Orbital eccentricity can make neutron star $g$ -mode resonances observable with current gravitational-wave detectors

János Takátsy ^1,2,*, Lorenz Zwick^2,3, Pankaj Saini ^2,3, and Johan Samsing^2,3

¹Institut für Physik und Astronomie, Universität Potsdam, Haus 28, Karl-Liebknecht-Straße 24-25, Potsdam, Germany
²Niels Bohr International Academy, The Niels Bohr Institute, Blegdamsvej 17, DK-2100, Copenhagen, Denmark
³Center of Gravity, Niels Bohr Institute, Blegdamsvej 17, 2100 Copenhagen, Denmark

^*Contact author: janos.takatsy@uni-potsdam.de

Reaction-constrained composition g -modes in neutron stars with antikaon condensates, hyperons, and Δ(1232) resonances

Prashant Thakur and Ishfaq Ahmad Rather

Phys. Rev. D 114 083034 (2026)

Identifiability of g mode resonances in eccentric binary neutron stars with multidetector observations

Mengfei Sun, Jie Wu, Qianning Hu, Jin Li, Nan Yang, Xianghe Ma, Borui Wang, Minghui Zhang, and Yuanhong Zhong

Phys. Rev. D 114 103011 (2026)

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ISSN 2470-0029 (online), 2470-0010 (print).

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