activity
20152023
most citedScience with e-ASTROGAM (A space mission for MeV-GeV gamma-ray astrophysics)

253 citations · 405 across the 11 of their papers we have counts for

collaborators

12 papers

hep-ph2023★ 18 cited

Constraints from the duration of supernova neutrino burst on on-shell light gauge boson production by neutrinos

David G. Cerdeño, Marina Cermeño, Yasaman Farzan

In this article, we study the on-shell production of low-mass vector mediators from neutrino-antineutrino coalescence in the core of proto-neutron stars. Taking into account the ra…

hep-ph2022★ 12 cited

Signatures of leptophilic t-channel dark matter from active galactic nuclei

Marina Cermeño, Céline Degrande, Luca Mantani

In this work, we study indirect photon signatures of leptophilic dark matter (DM) coming from Centaurus A, where a DM density spike is believed to have survived to date contrary to…

hep-ph2021★ 1 cited

Searching for Dark Matter with circularly polarised photons from the Galactic Centre

Marina Cermeño, Céline Degrande, Luca Mantani

Conventional indirect dark matter (DM) searches look for an excess in the electromagnetic emission from the sky that cannot be attributed to known astrophysical sources, but its po…

hep-ph2021★ 14 cited

Medium effects in supernovae constraints on light mediators

David G. Cerdeño, Marina Cermeño, M. Ángeles Pérez-García +1

In this article, we reevaluate supernovae (SN) constraints on the diffusion time of neutrinos for a family of extensions of the Standard Model that incorporate new light scalar and…

hep-ph2021

Circular polarisation of gamma rays as a probe of dark matter interactions with cosmic ray electrons

Marina Cermeño, Céline Degrande, Luca Mantani

Conventional indirect dark matter (DM) searches look for an excess in the electromagnetic emission from the sky that cannot be attributed to known astrophysical sources. Here, we a…

astro-ph.SR2018★ 6 cited

Modified Gravity at Astrophysical Scales

M. Cermeño, J. Carro, A. L. Maroto +1

Using a perturbative approach we solve stellar structure equations for low-density (solar-type) stars whose interior is described with a polytropic equation of state in scenarios i…

hep-ph2018★ 24 cited

Gamma rays from dark mediators in white dwarfs

M. Cermeño, M. Angeles Pérez-García

We consider self-annihilation of dark matter, , into metastable mediators, , and their subsequent decay into photons inside white dwarfs. We focus on reactions of the type $χ…

astro-ph.HE2017★ 253 cited

Science with e-ASTROGAM (A space mission for MeV-GeV gamma-ray astrophysics)

A. De Angelis, V. Tatischeff, I. A. Grenier +248

e-ASTROGAM (enhanced ASTROGAM) is a breakthrough Observatory space mission, with a detector composed by a Silicon tracker, a calorimeter, and an anticoincidence system, dedicated t…

astro-ph.HE2017★ 27 cited

Fermionic Light Dark Matter particles and the New Physics of Neutron Stars

M. Cermeño, M. Ángeles Pérez-García, Joseph Silk

Dark Matter constitutes most of the matter in the presently accepted cosmological model for our Universe. The extreme conditions of ordinary baryonic matter, namely high density an…

hep-ph2017★ 13 cited

Enhanced neutrino emissivities in pseudoscalar-mediated Dark Matter annihilation in Neutron Stars

M. Cermeño, M. A. Pérez-García, R. A. Lineros

We calculate neutrino emissivities from self-annihilating dark matter () in the dense and hot stellar interior of a (proto)neutron star. Using a model where dark matter interact…

astro-ph.HE2016★ 25 cited

Light dark matter scattering in outer neutron star crusts

Marina Cermeño, M. Ángeles Pérez-García, Joseph Silk

We calculate for the first time the phonon excitation rate in the outer crust of a neutron star due to scattering from light dark matter (LDM) particles gravitationally boosted int…

hep-ph2015★ 12 cited

Diffusion of dark matter in a hot and dense nuclear environment

Marina Cermeño, M. Ángeles Pérez-García, Joseph Silk

We calculate the mean free path in a hot and dense nuclear environment for a fermionic dark matter particle candidate in the GeV mass range interacting with nucleons via scal…