Zobrazeno 1 - 10
of 20
pro vyhledávání: '"Pedro De La Torre Luque"'
Publikováno v:
The Astrophysical Journal Letters, Vol 973, Iss 1, p L6 (2024)
We explore the 511 keV emission associated with sub-GeV dark matter (DM) particles that can produce electron–positron pairs and form positronium after thermalizing. We use ∼16 yr of data from the Spectrometer on INTEGRAL to constrain DM propertie
Externí odkaz:
https://doaj.org/article/c99c53082de1498e918024adc2878f20
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 83, Iss 2, Pp 1-10 (2023)
Abstract The elusive nature of Dark Matter (DM) remains a mystery far from being solved. A vast effort is dedicated to search for signatures of feeble DM interactions with Standard Model particles. In this work, we explore the signatures of axion DM
Externí odkaz:
https://doaj.org/article/7dfbc3bb4de143febf6cdacdd1e06c81
Publikováno v:
The Astrophysical Journal, Vol 968, Iss 1, p 46 (2024)
We study sub-GeV dark matter (DM) particles that may annihilate or decay into Standard Model particles producing an exotic injection component in the Milky Way that leaves an imprint in both photon and cosmic-ray (CR) fluxes. Specifically, the DM par
Externí odkaz:
https://doaj.org/article/f32141bc072742dd88659e4d1b7f7b68
Publikováno v:
Proceedings of 7th Heidelberg International Symposium on High-Energy Gamma-Ray Astronomy — PoS(Gamma2022).
Publikováno v:
Proceedings of 27th European Cosmic Ray Symposium — PoS(ECRS).
Publikováno v:
Proceedings of 27th European Cosmic Ray Symposium — PoS(ECRS).
Publikováno v:
Proceedings of 27th European Cosmic Ray Symposium — PoS(ECRS).
Publikováno v:
Physical Review D. 106
TeV halos are regions of enhanced photon emissivity surrounding pulsars. While multiple sources have been discovered, a self-consistent explanation of their radial profile and spherically-symmetric morphology remains elusive due to the difficulty in
Autor:
Stefano Gabici, Daniele Gaggero, Ottavio Fornieri, Silvio Sergio Cerri, Pedro De la Torre Luque
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 502 (4), pp.5821-5838. ⟨10.1093/mnras/stab355⟩
Monthly Notices of the Royal Astronomical Society, 2021, 502 (4), pp.5821-5838. ⟨10.1093/mnras/stab355⟩
Monthly notices of the Royal Astronomical Society 502(4), 5821-5838 (2021). doi:10.1093/mnras/stab355
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 502 (4), pp.5821-5838. ⟨10.1093/mnras/stab355⟩
Monthly Notices of the Royal Astronomical Society, 2021, 502 (4), pp.5821-5838. ⟨10.1093/mnras/stab355⟩
Monthly notices of the Royal Astronomical Society 502(4), 5821-5838 (2021). doi:10.1093/mnras/stab355
Monthly notices of the Royal Astronomical Society 502(4), 5821 - 5838 (2021). doi:10.1093/mnras/stab355
We present a comprehensive study about the phenomenological implications of the theory describing Galactic cosmic ray scattering on to magnet
We present a comprehensive study about the phenomenological implications of the theory describing Galactic cosmic ray scattering on to magnet
Publikováno v:
Journal of Physics: Conference Series. 2429:012036
The Tibet ASγ experiment recently reported the observation of a diffuse gamma-ray emission from the Galactic plane with energy up to the PeV. This finding seems to be confirmed by LHAASO preliminary results. Both measurements provide the first evide