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The sensitivity of direct detection of dark matter (DM) approaches the so-called neutrino floor below which it is hard to disentangle the DM candidate from the background neutrino. In this work we consider the scenario that no DM signals…

高能物理 - 唯象学 · 物理学 2020-12-02 Qing-Hong Cao , An-Kang Wei , Qian-Fei Xiang

We determine the prospects for direct and indirect detection of thermal relic neutralinos in supersymmetric theories with multi-TeV squarks and sleptons. We consider the concrete example of the focus point region of minimal supergravity,…

高能物理 - 唯象学 · 物理学 2014-10-01 Patrick Draper , Jonathan Feng , Philipp Kant , Stefano Profumo , David Sanford

Mirror dark matter offers a framework to explain the existing dark matter direct detection experiments. Here we confront this theory with the most recent experimental data, paying attention to the various known systematic uncertainties, in…

高能物理 - 唯象学 · 物理学 2010-11-11 R. Foot

In most models of the dark sector, dark matter is charged under some new symmetry to make it stable. We explore the possibility that not just dark matter, but also the force carrier connecting it to the visible sector is charged under this…

高能物理 - 唯象学 · 物理学 2015-06-19 David Curtin , Yuhsin Tsai

Effective contact operators provide the simplest parameterization of dark matter searches at colliders. However, light mediator can significantly change the sensitivity and search strategies. Considering simple models of mediators is an…

高能物理 - 唯象学 · 物理学 2014-06-25 Haipeng An , Lian-Tao Wang , Hao Zhang

The complementarity between dark matter searches at colliders and in underground laboratories is an extraordinarily powerful tool in the quest for dark matter. In the vast majority of the analyses conducted so far these dark matter…

高能物理 - 唯象学 · 物理学 2013-04-24 Giorgio Arcadi , Riccardo Catena , Piero Ullio

We study a minimal model with an imposed $\mathbb{Z}_2$ symmetry incorporating two singlet fermions and a singlet scalar which communicate with the SM particles through a scalar-Higgs portal. We probe regions in the parameter space where…

高能物理 - 唯象学 · 物理学 2026-04-10 Karim Ghorbani

Higgs-portal effective field theories are widely used as benchmarks in order to interpret collider and astroparticle searches for dark matter (DM) particles. To assess the validity of these effective models, it is important to confront them…

高能物理 - 唯象学 · 物理学 2021-08-18 Giorgio Arcadi , Abdelhak Djouadi , Marumi Kado

Direct detection experiments for light (sub-GeV) dark matter are making enormous leaps in reaching previously unexplored theory space. The need for accurate characterizations of target responses has led to a growing interplay between…

高能物理 - 唯象学 · 物理学 2022-03-16 Andrea Mitridate , Tanner Trickle , Zhengkang Zhang , Kathryn M. Zurek

We present an undated comprehensive analysis for the simplest dark matter model in which a real singlet scalar with a $Z_2$ symmetry is introduced to extend the standard model. According to the observed dark matter abundance, we predict the…

高能物理 - 唯象学 · 物理学 2010-11-17 Wan-Lei Guo , Yue-Liang Wu

Direct detection of dark matter (DM) requires an interaction of dark matter particles with nucleons. The same interaction can lead to dark matter pair production at a hadron collider, and with the addition of initial state radiation this…

高能物理 - 唯象学 · 物理学 2011-01-05 Yang Bai , Patrick J. Fox , Roni Harnik

Dark matter (DM) is currently searched for with a variety of detection strategies. Accelerator searches are particularly promising, but even if Weakly Interacting Massive Particles (WIMPs) are found at the Large Hadron Collider (LHC), it…

高能物理 - 唯象学 · 物理学 2010-10-13 Gianfranco Bertone , David G. Cerdeno , Mattia Fornasa , Roberto Ruiz de Austri , Roberto Trotta

We study a Dark Matter (DM) model in which the dominant coupling to the standard model occurs through a neutrino-DM-scalar coupling. The new singlet scalar will generically have couplings to nuclei/electrons arising from renormalizable…

高能物理 - 唯象学 · 物理学 2020-07-22 Nicholas Hurtado , Hana Mir , Ian M. Shoemaker , Eli Welch , Jason Wyenberg

Any form of dark matter which was in thermal equilibrium with the Standard Model in the early Universe must have some annihilation mechanism in order to avoid overclosure. In general, such models are now constrained by the negative…

高能物理 - 唯象学 · 物理学 2017-05-12 Matthew R. Buckley , David Feld

We consider a spin~-~3/2 fermionic dark matter candidate (DM) interacting with Standard Model fermions through a vector mediator in the $s$-channel. We find that for pure vector couplings almost the entire parameter space of the DM and…

高能物理 - 唯象学 · 物理学 2016-12-26 Mohammed Omer Khojali , Ashok Goyal , Mukesh Kumar , Alan S. Cornell

We analyze future direct data matter detection experiments using Effective Field Theory (EFT) operators with light, $\lesssim 100$ MeV mass mediators. We compare the nuclear recoil energy spectra from these operators to the predicted high…

高能物理 - 唯象学 · 物理学 2017-03-29 James B. Dent , Bhaskar Dutta , Jayden L. Newstead , Louis E. Strigari

Several direct detection experiments, including recently CDMS-II, have reported signals consistent with 5 to 10 GeV dark matter (DM) that appear to be in tension with null results from XENON and LUX experiments; these indicate a careful…

宇宙学与河外天体物理 · 物理学 2014-03-10 Yao-Yuan Mao , Louis E. Strigari , Risa H. Wechsler

Using the existing simplified model framework, we build several dark matter models which have suppressed spin-independent scattering cross section. We show that the scattering cross section can vanish due to interference effects with models…

高能物理 - 唯象学 · 物理学 2017-05-30 Arghya Choudhury , Kamila Kowalska , Leszek Roszkowski , Enrico Maria Sessolo , Andrew J. Williams

The scattering of dark matter particles off nuclei in direct detection experiments can be described in terms of a multidimensional effective field theory (EFT). A new systematic analysis technique is developed using the EFT approach and…

宇宙学与河外天体物理 · 物理学 2017-04-26 H. E. Rogers , D. G. Cerdeno , P. Cushman , F. Livet , V. Mandic

We point out a serendipitous link between warm dark matter (WDM) models for structure formation on the one hand and the high sensitivity energy range (1-10 keV) for x-ray photon detection on the Chandra and XMM-Newton observatories on the…

天体物理学 · 物理学 2009-07-09 K. Abazajian , G. M. Fuller , W. H. Tucker