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Gamma-ray flux limits from nearby brown dwarfs: Implications for dark matter annihilating into long-lived mediators.

<!--HTML-->Brown dwarfs (BDs) are celestial objects representing the link between the least massive main-sequence stars and giant gas planets. I will present a recent analysis (Bhattacharjee et al.,2023) where consider a sample of nine nearby ($<$ 11 pc distance), cold and old BDs and look...

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Autor principal: BHATTACHARJEE, Pooja
Lenguaje:eng
Publicado: 2023
Materias:
Acceso en línea:http://cds.cern.ch/record/2860564
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author BHATTACHARJEE, Pooja
author_facet BHATTACHARJEE, Pooja
author_sort BHATTACHARJEE, Pooja
collection CERN
description <!--HTML-->Brown dwarfs (BDs) are celestial objects representing the link between the least massive main-sequence stars and giant gas planets. I will present a recent analysis (Bhattacharjee et al.,2023) where consider a sample of nine nearby ($<$ 11 pc distance), cold and old BDs and look for gamma-ray signal from the direction of these objects using 13 years of \textit{Fermi}-LAT data. In the absence of any gamma-ray excess, we set 95\% confidence level upper limits on the gamma-ray flux with a binned-likelihood approach. I will then show how this null result can be used to constrain particle dark matter (DM). If the DM of the universe is constituted of particles with non-negligible couplings to the standard model, BDs may efficiently accumulate them through scatterings. DM particles eventually thermalize and can annihilate into light, long-lived, mediators which later decay into photons outside the BD. Within this framework, we set a stacked upper limit on the DM-nucleon elastic scattering cross section at the level $\sim 10^{-38}$ cm$^{2}$ for DM masses below 10 GeV. Our limits are comparable to similar bounds from the capture of DM particles in celestial objects but have the advantage of covering a larger portion of the parameter space in mediator decay length and DM mass and being less affected by DM modeling uncertainties. Reference: Bhattacharjee et al.,2023 - ``Gamma-ray flux limits from brown dwarfs: Implications for dark matter annihilating into long-lived mediators'' -Pooja Bhattacharjee, Francesca Calore, and Pasquale Dario Serpico - Phys. Rev. D 107, 043012 – Published 10 February 2023
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spelling cern-28605642023-06-01T21:43:20Zhttp://cds.cern.ch/record/2860564engBHATTACHARJEE, PoojaGamma-ray flux limits from nearby brown dwarfs: Implications for dark matter annihilating into long-lived mediators.Third EuCAPT Annual SymposiumEucapt Conferences<!--HTML-->Brown dwarfs (BDs) are celestial objects representing the link between the least massive main-sequence stars and giant gas planets. I will present a recent analysis (Bhattacharjee et al.,2023) where consider a sample of nine nearby ($<$ 11 pc distance), cold and old BDs and look for gamma-ray signal from the direction of these objects using 13 years of \textit{Fermi}-LAT data. In the absence of any gamma-ray excess, we set 95\% confidence level upper limits on the gamma-ray flux with a binned-likelihood approach. I will then show how this null result can be used to constrain particle dark matter (DM). If the DM of the universe is constituted of particles with non-negligible couplings to the standard model, BDs may efficiently accumulate them through scatterings. DM particles eventually thermalize and can annihilate into light, long-lived, mediators which later decay into photons outside the BD. Within this framework, we set a stacked upper limit on the DM-nucleon elastic scattering cross section at the level $\sim 10^{-38}$ cm$^{2}$ for DM masses below 10 GeV. Our limits are comparable to similar bounds from the capture of DM particles in celestial objects but have the advantage of covering a larger portion of the parameter space in mediator decay length and DM mass and being less affected by DM modeling uncertainties. Reference: Bhattacharjee et al.,2023 - ``Gamma-ray flux limits from brown dwarfs: Implications for dark matter annihilating into long-lived mediators'' -Pooja Bhattacharjee, Francesca Calore, and Pasquale Dario Serpico - Phys. Rev. D 107, 043012 – Published 10 February 2023oai:cds.cern.ch:28605642023
spellingShingle Eucapt Conferences
BHATTACHARJEE, Pooja
Gamma-ray flux limits from nearby brown dwarfs: Implications for dark matter annihilating into long-lived mediators.
title Gamma-ray flux limits from nearby brown dwarfs: Implications for dark matter annihilating into long-lived mediators.
title_full Gamma-ray flux limits from nearby brown dwarfs: Implications for dark matter annihilating into long-lived mediators.
title_fullStr Gamma-ray flux limits from nearby brown dwarfs: Implications for dark matter annihilating into long-lived mediators.
title_full_unstemmed Gamma-ray flux limits from nearby brown dwarfs: Implications for dark matter annihilating into long-lived mediators.
title_short Gamma-ray flux limits from nearby brown dwarfs: Implications for dark matter annihilating into long-lived mediators.
title_sort gamma-ray flux limits from nearby brown dwarfs: implications for dark matter annihilating into long-lived mediators.
topic Eucapt Conferences
url http://cds.cern.ch/record/2860564
work_keys_str_mv AT bhattacharjeepooja gammarayfluxlimitsfromnearbybrowndwarfsimplicationsfordarkmatterannihilatingintolonglivedmediators
AT bhattacharjeepooja thirdeucaptannualsymposium