Fits to the Fermi-LAT GeV excess with right-handed sneutrino dark matter: Implications for direct and indirect dark matter searches and the LHC

被引:40
|
作者
Cerdeno, D. G. [1 ]
Peiro, M. [2 ,3 ]
Robles, S. [2 ,3 ]
机构
[1] Univ Durham, Inst Particle Phys Phenomenol, Dept Phys, Durham DH1 3LE, England
[2] Univ Autonoma Madrid, CSIC, Inst Fis Teor, E-28049 Madrid, Spain
[3] Univ Autonoma Madrid, Dept Fis Teor, E-28049 Madrid, Spain
来源
PHYSICAL REVIEW D | 2015年 / 91卷 / 12期
关键词
COGENT; DAMA;
D O I
10.1103/PhysRevD.91.123530
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show that the right-handed (RH) sneutrino in the next-to-minimal supersymmetric standard model can account for the observed excess in the Fermi- LAT spectrum of gamma rays from the Galactic center, while fulfilling all the current experimental constraints from the LHC as well as from direct and indirect dark matter searches. We have explored the parameter space of this scenario, computed the gamma-ray spectrum for each phenomenologically viable solution and then performed a chi(2) fit to the excess. Unlike previous studies based on model- independent interpretations, we have taken into account the full annihilation spectrum, without assuming pure annihilation channels. Furthermore, we have incorporated limits from direct detection experiments, LHC bounds and also the constraints from Fermi- LAT on dwarf spheroidal galaxies and gamma- ray spectral lines. In addition, we have estimated the effect of the most recent Fermi- LAT reprocessed data (pass 8). In general, we obtain good fits to the Galactic center excess (GCE) when the RH sneutrino annihilates mainly into pairs of light singlet like scalar or pseudoscalar Higgs bosons that subsequently decay in flight, producing four-body final states and spectral features that improve the goodness of the fit at large energies. The best fit (chi(2) = 20.8) corresponds to a RH sneutrino with a mass of 64 GeV which annihilates preferentially into a pair of light singlet like pseudoscalar Higgs bosons (with masses of order 60 GeV). Besides, we have analyzed other channels that also provide good fits to the excess. Finally, we discuss the implications for direct and indirect detection searches paying special attention to the possible appearance of gamma- ray spectral features in near future Fermi- LAT analyses, as well as deviations from the Standard Model- like Higgs properties at the LHC. Remarkably, many of the scenarios that fit the GCE can also be probed by these other complementary techniques.
引用
收藏
页数:12
相关论文
共 50 条
  • [21] Right-handed sneutrino dark matter and big-bang nucleosynthesis
    Ishiwata, Koji
    Kawasaki, Masahiro
    Kohri, Kazunori
    Moroi, Takeo
    PHYSICS LETTERS B, 2010, 689 (4-5) : 163 - 168
  • [22] Right-handed sneutrino dark matter in supersymmetric B − L model
    Shaaban Khalil
    Hiroshi Okada
    Takashi Toma
    Journal of High Energy Physics, 2011
  • [23] Gravitino dark matter with weak-scale right-handed sneutrino
    Ishiwata, Koji
    Matsumoto, Shigeki
    Moroi, Takeo
    PHYSICAL REVIEW D, 2008, 77 (03):
  • [24] Fitting the Fermi-LAT GeV excess: On the importance of including the propagation of electrons from dark matter
    Lacroix, Thomas
    Baehm, Celine
    Silk, Joseph
    PHYSICAL REVIEW D, 2014, 90 (04):
  • [25] Implications of the Fermi-LAT Pass 8 Galactic Center excess on supersymmetric dark matter
    Achterberg, Abraham
    van Beekveld, Melissa
    Caron, Sascha
    Gomez-Vargas, German A.
    Hendriks, Luc
    Ruiz de Austri, Roberto
    JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2017, (12):
  • [26] The Fermi-LAT Galactic Center Excess: Evidence of Annihilating Dark Matter?
    Murgia, Simona
    ANNUAL REVIEW OF NUCLEAR AND PARTICLE SCIENCE, VOL 70, 2020, 70 : 455 - 483
  • [27] 130 GeV fingerprint of right-handed neutrino dark matter
    Bergstrom, Lars
    PHYSICAL REVIEW D, 2012, 86 (10):
  • [28] Right-handed sneutrino and gravitino multicomponent dark matter in light of neutrino detectors
    Kim, Jong Soo
    Lopez-Fogliani, Daniel E.
    Perez, Andres D.
    Ruiz de Austri, Roberto
    JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2023, (04):
  • [29] The right-handed sneutrino as thermal dark matter in U(1) extensions of the MSSM
    Belanger, G.
    Da Silva, J.
    Pukhov, A.
    JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2011, (12):
  • [30] Indirect detection of Dirac right-handed neutrino dark matter
    Hooper, D
    Servant, G
    ASTROPARTICLE PHYSICS, 2005, 24 (03) : 231 - 246