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In this work we have considered a minimal extension of Standard Model by a local $U(1)$ gauge group in order to accommodate a stable (fermionic) Dark Matter (DM) candidate. We have focussed on parameter regions where DM possesses adequate…

高能物理 - 唯象学 · 物理学 2021-01-08 Rahool Kumar Barman , Biplob Bhattacherjee , Arindam Chatterjee , Arghya Choudhury , Aritra Gupta

Weakly interacting massive particles (WIMPs) are one of the leading candidates for Dark Matter. So far we can use direct Dark Matter detection to estimate the mass of halo WIMPs only by fitting predicted recoil spectra to future…

高能物理 - 唯象学 · 物理学 2011-11-10 Chung-Lin Shan , Manuel Drees

We reassess the realistic discovery reach of Solar-System experiments for dark energy (DE) and dark matter (DM), making explicit the bridge from cosmology-level linear responses to local, screened residuals. In scalar-tensor frameworks with…

宇宙学与河外天体物理 · 物理学 2025-12-02 Slava G. Turyshev

Dark Matter experiments searching for Weakly interacting massive particles (WIMPs) primarily use nuclear recoils (NRs) in their attempt to detect WIMPs. Migdal-induced electronic recoils (ERs) provide additional sensitivity to light Dark…

高能物理 - 唯象学 · 物理学 2022-12-22 J. R. Angevaare , G. Bertone , A. P. Colijn , M. P. Decowski , B. J. Kavanagh

The Weak Equivalence Principle (WEP), stating that two bodies of different compositions and/or mass fall at the same rate in a gravitational field (universality of free fall), is at the very foundation of General Relativity. The MICROSCOPE…

In direct dark matter detection experiments, conventional elastic scattering of WIMPs results in exponentially falling recoil spectra. In contrast, theories of WIMPs with excited states can lead to nuclear recoil spectra that peak at finite…

高能物理 - 唯象学 · 物理学 2014-11-20 Rafael F. Lang , Neal Weiner

The mechanism behind Electroweak Symmetry Breaking (EWSB) and the nature of dark matter (DM) are currently among the most important issues in high energy physics. Since a natural dark matter candidate is a weakly interacting massive…

高能物理 - 唯象学 · 物理学 2008-11-26 Thomas Hambye , Michel H. G. Tytgat

In the cosmological paradigm, cold dark matter (DM) dominates the mass content of the Universe and is present at every scale. Candidates for DM include many extensions of the standard model, such as weakly interacting massive particles…

高能天体物理现象 · 物理学 2019-08-13 Benjamin Zitzer

Current cosmological models and data suggest the existence of a cold Dark Matter (DM) component, however the nature of DM particles remains unknown. A favored candidate for DM is a Weakly Interacting Massive Particle (WIMP) in the mass…

高能天体物理现象 · 物理学 2019-08-13 Benjamin Zitzer

We made global fits of the inert Higgs doublet model (IDM) in the light of collider and dark matter search limits and the requirement for a strongly first-order electroweak phase transition (EWPT). These show that there are still IDM…

高能物理 - 唯象学 · 物理学 2022-10-11 Shehu AbdusSalam , Leila Kalhor , Mohammad Mohammadidoust

Weak lensing provides a direct measure of the distribution of mass in the universe, and is therefore a uniquely powerful probe of dark matter. Weak lensing can also be used to measure the twin phenomenon of dark energy, via its effect upon…

天体物理学 · 物理学 2007-05-23 Richard Massey , Alexandre Refregier , Jason Rhodes

If dark matter (DM) simply consists in a scalar particle interacting dominantly with the Higgs boson, the ratio of its annihilation cross section ---which is relevant both for the relic abundance and indirect detection--- and its…

高能物理 - 唯象学 · 物理学 2014-11-20 Sarah Andreas , Chiara Arina , Thomas Hambye , Fu-Sin Ling , Michel H. G. Tytgat

Dark matter detectors built primarily to probe elastic scattering of WIMPs on nuclei are also precise probes of light, weakly coupled particles that may be absorbed by the detector material. In this paper, we derive constraints on the…

高能物理 - 唯象学 · 物理学 2015-07-23 Haipeng An , Maxim Pospelov , Josef Pradler , Adam Ritz

Weakly interacting massive particle (WIMP) is well known to be a good candidate for dark matter, and it is also predicted by many new physics models beyond the standard model at the TeV scale. We found that, if the WIMP is a vector particle…

高能物理 - 唯象学 · 物理学 2015-06-04 Tomohiro Abe , Mitsuru Kakizaki , Shigeki Matsumoto , Osamu Seto

Weakly Interacting Massive Particles (WIMPs) are among the main candidates for the relic dark matter (DM). The idea of the direct DM detection relies on elastic spin-dependent (SD) and spin-independent (SI) interaction of WIMPs with target…

高能物理 - 唯象学 · 物理学 2009-10-20 V. A. Bednyakov , H. V. Klapdor-Kleingrothaus

The Abnormally Weighting Energy (AWE) hypothesis consists of assuming that the dark sector of cosmology violates the weak equivalence principle (WEP) on cosmological scales, which implies a violation of the strong equivalence principle for…

天体物理学 · 物理学 2008-11-26 A. Fuzfa , J. -M. Alimi

Direct searches for WIMPs are sensitive to physics well below the weak scale. In the absence of light mediators, it is fruitful to apply an Effective Field Theory (EFT) approach accounting only for dark matter (DM) interactions with…

高能物理 - 唯象学 · 物理学 2015-04-21 Francesco D'Eramo , Massimiliano Procura

Dark matter is thought to make up most of the matter density of the Universe, yet its true nature remains uncertain. Among dark matter theories, Weakly Interacting Massive Particles (WIMPs) are a prominent candidate for dark matter because…

高能天体物理现象 · 物理学 2023-09-20 Micael Andrade , Aion Viana

Cosmology offers opportunities to test Dark Matter independently of its interactions with the Standard Model. We study the imprints of long-range forces acting solely in the dark sector on the distribution of galaxies, the so-called Large…

宇宙学与河外天体物理 · 物理学 2024-08-01 Salvatore Bottaro , Emanuele Castorina , Marco Costa , Diego Redigolo , Ennio Salvioni

Weakly Interacting Massive Particles (WIMPs) are one of the leading candidates for Dark Matter. Currently, the most promising method to detect WIMPs is the direct detection of the recoil energy deposited in a low-background laboratory…

天体物理学 · 物理学 2011-11-10 Chung-Lin Shan