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相关论文: Indirect Detection of Little Higgs Dark Matter

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The introduction of T parity dramatically improves the consistency of Little Higgs models with precision electroweak data, and renders the lightest T-odd particle (LTP) stable. In the Littlest Higgs model with T parity, the LTP is typically…

高能物理 - 唯象学 · 物理学 2012-02-06 Andreas Birkedal , Andrew Noble , Maxim Perelstein , Andrew Spray

We examine the status of dark matter (heavy photon) in the littlest Higgs model with T-parity (LHT) in light of the new results from the LHC Higgs search, the Planck dark matter relic density and the XENON100 limit on the dark matter…

高能物理 - 唯象学 · 物理学 2013-12-30 Lei Wang , Jin Min Yang , Jingya Zhu

Little Higgs models may provide a viable alternative to supersymmetry as an extension of the Standard Model. After the introduction of a discrete $Z_2$ symmetry, dubbed T-parity into Little Higgs models they also contain a promising dark…

高能物理 - 唯象学 · 物理学 2009-03-30 Pat Kalyniak , Dmitriy Tseliakhovich

Following previous study, in the Littlest Higgs model (LHM), the heavy photon is supposed to be a possible dark matter candidate and its relic abundance of the heavy photon is estimated in terms of the Boltzman-Lee-Weinberg time-evolution…

高能物理 - 唯象学 · 物理学 2009-01-01 Qing-Peng Qiao , Jian Tang , Xue-Qian Li

Dark matter candidates arising in models of particle physics incorporating weak scale supersymmetry may produce detectable signals through their annihilation into neutrinos, photons, or positrons. A large number of relevant experiments are…

天体物理学 · 物理学 2009-10-09 Jonathan L. Feng , Konstantin T. Matchev , Frank Wilczek

High energy neutrinos are produced by the annihilation of dark matter particles in our galaxy. These are presently searched for with large area, deep underground neutrino telescopes. Cold dark matter particles, trapped inside the sun, are…

高能物理 - 唯象学 · 物理学 2009-09-25 F. Halzen , J. E. Jacobsen

Considerable efforts have been dedicated to discovering a dark photon via the decay of the Higgs boson to a photon and an invisible particle. A subject that is still mostly unexplored is which properties of the dark photon could be measured…

高能物理 - 唯象学 · 物理学 2022-05-11 Hugues Beauchesne , Cheng-Wei Chiang

One way to unambiguously confirm the existence of particle dark matter and determine its mass would be to detect its annihilation into monochromatic gamma-rays in upcoming telescopes. One of the most minimal models for dark matter is the…

天体物理学 · 物理学 2008-11-26 Michael Gustafsson , Erik Lundstrom , Lars Bergstrom , Joakim Edsjo

Weakly interacting massive particles (WIMPs) are among the favored candidates for cold dark matter in the universe. The phenomenology of supersymmetric WIMPs has been quite developed during recent years. However, there are other…

高能物理 - 唯象学 · 物理学 2009-11-07 E. A. Baltz , L. Bergstrom

Recently, Weinberg proposed a Higgs portal model with a spontaneously broken global $U(1)$ symmetry in which Goldstone bosons may be masquerading as fractional cosmic neutrinos. We extend the model by gauging the $U(1)$ symmetry. This gives…

高能物理 - 唯象学 · 物理学 2015-06-19 Kin-Wang Ng , Huitzu Tu , Tzu-Chiang Yuan

Giving up the assumption of the gaugino mass unification at the GUT scale, the latest LEP and Tevatron data still allow the lightest supersymmetric Higgs to have a large branching fraction into invisible neutralinos. Such a Higgs may be…

高能物理 - 唯象学 · 物理学 2009-11-07 G. Belanger , F. Boudjema , A. Cottrant , R. M. Godbole , A. Semenov

It was recently argued by Hooper and Goodenough [arXiv:1010.2752] that the excess gamma ray emission from within 1-2 degrees of the galactic center can be well-described by annihilation of ~8 GeV dark matter particles into tau pairs. I show…

高能物理 - 唯象学 · 物理学 2011-03-21 Heather E. Logan

High energy particles are produced by the annihilation of dark matter particles in our galaxy. These are presently searched for using balloon-borne antiproton and positron detectors and large area, deep underground neutrino telescopes. Dark…

高能物理 - 唯象学 · 物理学 2016-09-01 F. Halzen , J. E Jacobsen

We investigate the signatures of neutrinos produced in the annihilation of WIMP dark matter in the Earth, the Sun and at the Galactic centre within the framework of the Inert Doublet Model and extensions. We consider a dark matter…

高能物理 - 唯象学 · 物理学 2010-01-05 Sarah Andreas , Michel H. G. Tytgat , Quentin Swillens

Dark Matter (DM), arising from an Inert Higgs Doublet, may either be light, below the $W$ mass, or heavy, above about 525 GeV. While the light region may soon be excluded, the heavy region is known to be very difficult to probe with either…

高能物理 - 唯象学 · 物理学 2015-07-31 Venus Keus , Stephen F. King , Stefano Moretti , Dorota Sokolowska

This is a short review of the framework proposed in \cite{Goh:2009wg} which gives rise to indirect Dark Matter (DM) signals explaining the recent cosmic-ray anomalies and links cosmic-ray signals of DM to LHC signals of a leptonic Higgs…

高能物理 - 唯象学 · 物理学 2015-05-14 Piyush Kumar

A search for a dark photon, a new light neutral particle, which decays promptly into collimated pairs of electrons or muons is presented. The search targets dark photons resulting from the exotic decay of the Standard Model Higgs boson,…

高能物理 - 实验 · 物理学 2025-03-27 ATLAS Collaboration

In the Next-to-Minimal Supersymmetric Standard Model, neutralino dark matter can annihilate into a pair of photons through the exchange of a CP-odd Higgs boson in the s-channel. The CP-odd Higgs boson couples to two photons through a loop…

高能物理 - 唯象学 · 物理学 2015-06-05 Debottam Das , Ulrich Ellwanger , Pantelis Mitropoulos

The extremely large hierarchy observed in the fermion mass spectrum remains as one of the most puzzling and unresolved issues in particle physics. In a recent proposal, however, it was demonstrated that by introducing one Higgs doublet (or…

高能物理 - 唯象学 · 物理学 2008-05-27 C. B. Jackson

Next-to-Minimal Supersymmetric Standard Model neutralino dark matter candidates in the (1-15) GeV range are found with a Markov Chain Monte Carlo scanning code. A very light, singlet-like Higgs and/or CP-odd Higgs is needed in order to…

高能物理 - 唯象学 · 物理学 2012-04-19 Daniel Albornoz Vásquez
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