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Related papers: Shedding Light on Mirror Dark Matter Using CDEX

200 papers

Dark matter consisting of very light and very weakly interacting particles such as axions, axion-like particles and hidden photons could be detected using reflective surfaces. On such reflectors some of the dark matter particles are…

High Energy Physics - Phenomenology · Physics 2018-11-30 Joerg Jaeckel , Stefan Knirck

The MAgnetized Disk and Mirror Axion eXperiment (MADMAX) is a future experiment aiming to detect dark matter axions from the galactic halo by resonant conversion to photons in a strong magnetic field. It uses a stack of dielectric disks in…

High Energy Physics - Experiment · Physics 2025-01-09 Pascal Pralavorio

We search for the dark photon dark matter (DPDM) using a cryogenic millimeter-wave receiver. DPDM has a kinetic coupling with electromagnetic fields with a coupling constant of $\chi$, and is converted into ordinary photons at the surface…

We propose a novel direct detection concept to search for dark matter with 100~keV to 100~MeV masses. Such dark matter can scatter off molecules in a gas and transfer an $\mathcal{O}(1)$ fraction of its kinetic energy to excite a…

High Energy Physics - Phenomenology · Physics 2019-11-20 Rouven Essig , Jesús Pérez-Ríos , Harikrishnan Ramani , Oren Slone

We show that new physics can show up in dileptonic events through its radiative contributions to the dilepton invariant mass, leading to unique "monocline" features in $m_{\ell\ell}$, as well as the angular distribution of the leptons. We…

High Energy Physics - Phenomenology · Physics 2015-06-17 Wolfgang Altmannshofer , Patrick J. Fox , Roni Harnik , Graham D. Kribs , Nirmal Raj

Self-interacting dark matter (SIDM) is a simple and well-motivated scenario that could explain long-standing puzzles in structure formation on small scales. If the required self-interaction arises through a light mediator (with mass $\sim…

High Energy Physics - Phenomenology · Physics 2015-11-04 Eugenio Del Nobile , Manoj Kaplinghat , Hai-Bo Yu

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…

High Energy Physics - Phenomenology · Physics 2017-05-12 Matthew R. Buckley , David Feld

We study the kinetic decoupling of light (lesssim 10 GeV) magnetic dipole dark matter (DM). We find that present bounds from collider, direct DM searches, and structure formation allow magnetic dipole DM to remain in thermal equilibrium…

High Energy Physics - Phenomenology · Physics 2016-06-15 Paolo Gondolo , Kenji Kadota

We report results of a search for dark-matter-nucleon interactions via a dark mediator using optimized low-energy data from the PandaX-4T liquid xenon experiment. With the ionization-signal-only data and utilizing the Migdal effect, we set…

The dark rate of single-electrons emitted from a cathode of a multi-cathode counter may be interpreted as the effect from Hidden Photons (HPs) of Cold Dark Matter (CDM). As a tentative approach the measurements have been performed at…

Instrumentation and Detectors · Physics 2018-04-10 A. V. Kopylov , I. V. Orekhov , V. V. Petukhov

Dark matter may interact with the Standard Model through the kinetic mixing of dark photons, $A'$, with Standard Model photons. Such dark matter will accumulate in the Sun and annihilate into dark photons. The dark photons may then leave…

High Energy Physics - Phenomenology · Physics 2017-10-05 Jonathan L. Feng , Jordan Smolinsky , Philip Tanedo

Measurements in the radio regime embrace a number of effective approaches for WISP searches, often covering unique or highly complementary ranges of the parameter space compared to those explored in other research domains. These…

Instrumentation and Detectors · Physics 2013-09-19 Dieter Horns , Axel Lindner , Andrei Lobanov , Andreas Ringwald

Here we present world-leading sensitivity to light ($< 170$ MeV) dark matter (DM) using beam-dump experiments. Dark sector particles produced during pion decay at accelerator beam-dumps can be detected via scattering in neutrino detectors.…

High Energy Physics - Phenomenology · Physics 2023-09-14 Bhaskar Dutta , Wei-Chih Huang , Jayden L. Newstead

Mirror atoms are expected to be a significant component of the galactic dark matter halo if mirror matter is identified with the non-baryonic dark matter in the Universe. Mirror matter can interact with ordinary matter via gravity and via…

High Energy Physics - Phenomenology · Physics 2008-11-26 R. Foot

I point out that the sterile neutrinos suggested as candidates of "cool" Dark Matter will decay through their mixing with light neutrinos. This leads to an upper bound of about 200 keV on the mass of the sterile neutrinos, but might…

High Energy Physics - Phenomenology · Physics 2007-05-23 Manuel Drees

Motivated by various kinds of new physics models, a new light neutral vector boson (the dark photon) connected to the Standard Model of particle physics only through the kinetic mixing with the U(1)_Y factor has been studied extensively.…

High Energy Physics - Phenomenology · Physics 2014-02-03 Haipeng An , Maxim Pospelov , Josef Pradler

The direct detection rate for supersymmetric cold dark matter (CDM) particles is calculated for a number of suitable nuclear targets. Both the coherent and spin contributions are considered. By considering representative phenomenologically…

High Energy Physics - Phenomenology · Physics 2014-11-17 J. D. Vergados , T. S. Kosmas

Mirror matter type dark matter can exist on the Earth's surface, potentially in enhanced concentrations at various anomalous impact sites. Mirror matter fragments can draw in heat from the ordinary matter environment, radiate mirror photons…

Condensed Matter · Physics 2008-11-26 R. Foot , S. Mitra

This is the second paper of a series devoted to the study of the cosmological implications of the existence of mirror dark matter. The parallel hidden mirror world has the same microphysics as the observable one and couples the latter only…

Astrophysics · Physics 2008-11-26 P. Ciarcelluti