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Resonant amplification of multimessenger emission in rotating stellar core collapse

Marco Cusinato1,*, Martin Obergaulinger1,2,†, Miguel Á. Aloy1,2,‡, and José A. Font1,2

  • *Contact author: marco.cusinato@uv.es
  • †Contact author: martin.obergaulinger@uv.es
  • ‡Contact author: miguel.a.aloy@uv.es

Toward more realistic machine-learning inference of the dense-matter equation of state from supernova gravitational waves

A. Akhmetali, Y. S. Abylkairov, M. Zaidyn, A. Sakan, A. Zhunuskanov, N. Ussipov, J. A. Font, A. Torres-Forné, and E. Abdikamalov

Phys. Rev. D 114 023053 (2026)

Parameter estimation horizon of core-collapse supernovae with current and next-generation gravitational-wave detectors

A. Akhmetali, Y. S. Abylkairov, D. Orel, S. Nunes, A. Sakan, A. Zhunuskanov, M. Zaidyn, N. Ussipov, J. A. Font, and E. Abdikamalov

Phys. Rev. D 114 043035 (2026)

Trends in gravitational wave emission in axisymmetric simulations of rotating core-collapse supernovae

Bailey Sykes and Bernhard Müller

Phys. Rev. D 113 103049 (2026)

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