collaborators

7 papers

astro-ph.HE2026

Gravitational-Wave Signals for Supernova Explosions of Three-Dimensional Progenitors

Alessandro Lella, Giuseppe Lucente, Daniel Kresse +3

Core-collapse supernovae (SNe) are sources of gravitational waves (GWs) produced by hydrodynamical instabilities and highly time-dependent anisotropies of the neutrino radiation. I…

hep-ph2026

The COSMIC WISPers White Paper: The physics case for Weakly Interacting Slim Particles

Ariel Arza, Deniz Aybas, Shyam Balaji +124

Axions and other very weakly interacting slim particles (WISPs), with masses below 1 GeV, arise naturally in many extensions of the Standard Model of particle physics. In particula…

hep-ph2025

Detecting light axions from supernovae in nearby galaxies

Francesca Lecce, Alessandro Lella, Giuseppe Lucente +2

Axion-like particles (ALPs) coupled to nucleons can be efficiently produced in core-collapse supernovae (SNe) and then, if they couple to photons, convert into gamma rays in cosmic…

hep-ph2025

Probing axion-like particles with multimessenger observations of neutron star mergers

Francesca Lecce, Alessandro Lella, Giuseppe Lucente +4

Axion-like particles (ALPs) can be copiously produced in binary neutron star (BNS) mergers through nucleon-nucleon bremsstrahlung if the ALP-nucleon couplings are sizable…

hep-ph2025

NuSTAR bounds on radiatively decaying particles from M82

Francisco R. Candón, Damiano F. G. Fiorillo, Giuseppe Lucente +2

Axions and other putative feebly interacting particles (FIPs) with a mass of tens to several hundreds of keVs can be produced in stellar cores with a Lorentz boost factor $E_a/m_a\…

hep-ph2025

Exploring the Dark Universe: A European Strategy for Axions and other WISPs Discovery

Deniz Aybas, Francesca Calore, Michele Cicoli +17

Axions and other very weakly interacting slim (with 1 GeV) particles (WISPs) are a common feature of several extensions of the Standard Model of Particle Physics. The search…