Search Publications

Multimessenger search for electrophilic feebly interacting particles from supernovae
DOI: 10.1103/PhysRevD.109.103028 Bibcode: 2024PhRvD.109j3028L

Carenza, Pierluca; Balaji, Shyam; Luque, Pedro De la Torre

We study MeV-scale electrophilic feebly interacting particles (FIPs), that may be abundantly produced in supernova explosions, escape the star and decay into electrons and positrons. This exotic injection of leptons in the Milky Way leaves an imprint in both photon and cosmic ray fluxes. Specifically, positrons lose energy and annihilate almost at…

2024 Physical Review D
INTEGRAL XMM-Newton 15
Robust constraints on feebly interacting particles using XMM-Newton
DOI: 10.1103/PhysRevD.109.L101305 Bibcode: 2024PhRvD.109j1305L

Carenza, Pierluca; Balaji, Shyam; Luque, Pedro De la Torre

During galactic supernova (SN) explosions, a large amount of feebly interacting particles (FIPs) may be produced. In this work we analyze electrophilic FIPs with masses in the MeV-range that escape from SN and decay into electron-positron pairs, causing an exotic leptonic injection. This contribution adds up to known components, leading to an unex…

2024 Physical Review D
INTEGRAL XMM-Newton 14
Primordial black holes and scalar-induced gravitational waves from the polynomial attractor model
DOI: 10.1103/PhysRevD.109.103532 Bibcode: 2024PhRvD.109j3532W

Wang, Yue; Gong, Yungui; Wang, Zhongkai +1 more

Primordial black holes (PBHs) generated in the early Universe are considered as one of the candidates for dark matter. To produce PBHs with sufficient abundance, the primordial scalar power spectrum needs to be enhanced to the order of 0.01. Considering the third-order polynomial potential with polynomial attractors, we show that PBHs with a mass …

2024 Physical Review D
INTEGRAL 4
Constraining the low-energy cosmic ray flux in the center molecular zone from MeV nuclear deexcitation line observations
DOI: 10.1103/PhysRevD.110.063033 Bibcode: 2024PhRvD.110f3033L

Liu, Bing; Yang, Ruizhi

Low-energy cosmic rays (LECRs) dominate the ionization in dense regions of molecular clouds in which other ionizers such as UV or x-ray photons are effectively shielded. Thus, it was argued that the high ionization rate at the central molecular zone (CMZ) of our Galaxy is mainly caused by LECRs. However, the required LECR flux is orders of magnitu…

2024 Physical Review D
INTEGRAL 1
Precise measurement of pion-bump structure using future MeV gamma-ray detectors
DOI: 10.1103/PhysRevD.110.063026 Bibcode: 2024PhRvD.110f3026L

Liu, Jiahao; Liu, Bing; Yang, Ruizhi

The pion-bump structure in the γ-ray spectrum is a direct proof for the hadronic origin of the γ rays, and thus the decisive evidence for the acceleration of hadronic cosmic…

2024 Physical Review D
INTEGRAL 0
Constraints on the parameters of keV-scale mass annihilating dark matter obtained with SRG/ART-XC observations
DOI: 10.1103/PhysRevD.110.123026 Bibcode: 2024PhRvD.110l3026Z

Burenin, R. A.; Krivonos, R. A.; Zakharov, E. I. +2 more

In this paper we present new constraints on the velocity-independent cross section of keV-scale mass annihilating dark matter particles obtained with SRG/ART-XC after 4 full-sky surveys. These constraints are derived from observations of the Milky Way Halo, 33 Local Group spheroidal dwarf (dSph) galaxies and separately for the dSph galaxy Ursa Maj…

2024 Physical Review D
INTEGRAL 0