output
19982026
most citedMeasurement of the permanent electric dipole moment of the neutron

619 citations

Showing 2025 · astro-ph.HEShow all

10 papers · 2 filters

astro-ph.HE2025

Nuclear parameter inference with semi-agnostic priors

Lami Suleiman, Anthea F. Fantina, Francesca Gulminelli +1

Radio pulsar timing, X-ray pulse profile modeling, and gravitational-wave detections of binary mergers involving at least one neutron star probe the properties of dense, neutron-ri…

astro-ph.HE2025

Optimizing the potential of KM3NeT in detecting core-collapse supernovae

KM3NeT Collaboration, O. Adriani, A. Albert +285

Core-collapse supernovae mark the end of life of massive stars. However, despite their importance in astrophysics, their underlying mechanisms remain unclear. Neutrinos that emerge…

astro-ph.HE2025★ 34 cited

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

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1783

We report the observation of gravitational waves from two binary black hole coalescences during the fourth observing run of the LIGO--Virgo--KAGRA detector network, GW241011 and GW…

astro-ph.HE2025

Constraining gamma-ray burst parameters with the first ultra-high energy neutrino event KM3-230213A

KM3NeT Collaboration, O. Adriani, A. Albert +278

Context: The detection of the highest energy neutrino observed to date by KM3NeT, with an estimated energy of 220 PeV, opens up new possibilities for the study and identification o…

astro-ph.HE2025★ 1 cited

Gravitational pulsars: correlations between the electromagnetic and the continuous gravitational wave signal

Marco Antonelli, Avishek Basu, Brynmor Haskell

Neutron stars emitting continuous gravitational waves may be regarded as gravitational pulsars, in the sense that it could be possible to track the evolution of their rotational pe…

astro-ph.HE2025★ 6 cited

Crust (Unified) Tool for Equation-of-state Reconstruction (CUTER) v2

P. J. Davis, H. Dinh Thi, A. F. Fantina +3

The equation of state (EoS) is a needed input to determine the neutron-star global properties and to relate them. It is thus important to provide consistent and unified EoSs to avo…