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most citedDo Finite Density Effects Jeopardize Axion Nucleophobia in Supernovae?

7 citations · 10 across the 10 of their papers we have counts for

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hep-ph2026

How invisible can QCD axions be? From Supernova emission to Cherenkov signals

Luca Di Luzio, Vincenzo Fiorentino, Maurizio Giannotti +2

We investigate the scenario of maximally invisible axions, namely QCD axions whose interactions with matter arise exclusively from the irreducible coupling to gluons responsible fo…

hep-ph2026

Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades

Víctor Fonoll, Maurizio Giannotti, Giuseppe Lucente

Weakly interacting slim particles (WISPs) can be produced in stars through the conversion of non-thermal photons generated in nuclear reactions. Previous studies have generally tre…

hep-ph2026★ 1 cited

Axions at the meV Crossroads: Theory, Cosmology, Astrophysics, and Experiments

Michele Cicoli, Francesco D'Eramo, Luca Di Luzio +18

The meV mass range has emerged as a focal point in axion physics, where advances in theory, cosmology, astrophysics, and experimental techniques converge. Axions in this mass range…

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★ 2 cited

Fresh look at the diffuse ALP background from supernovae

Francisco R. Candón, Sougata Ganguly, Maurizio Giannotti +3

Protoneutron stars, highly compact objects formed in the core of exploding supernovae (SNe), are powerful sources of axion-like particles (ALPs). In the SN core, ALPs are dominantl…

hep-ph2024

Axion-induced pair production: a new strategy for axion detection

Fernando Arias-Aragón, Maurizio Giannotti, Giovanni Grilli di Cortona +1

We revisit and update the axion-induced pair production process in a nuclear electric field mediated by the axion-electron coupling, $a+{{}^{A}_{Z}X} \rightarrow {{}^{A}_{Z}X} + e^…

hep-ph2024★ 7 cited

Do Finite Density Effects Jeopardize Axion Nucleophobia in Supernovae?

Luca Di Luzio, Vincenzo Fiorentino, Maurizio Giannotti +2

Nucleophobic axion models, wherein axion couplings to both protons and neutrons are simultaneously suppressed, can relax the stringent constraints from SN 1987A. However, it remain…