English
Related papers

Related papers: Testing Light Dark Matter Coannihilation With Fixe…

200 papers

We provide a simple model of vector dark matter (DM) which can realize the recently proposed freeze-out mechanism with catalyzed annihilation. In our setup, a vector DM field $X_\mu$ and a catalyst field $C_\mu$ is unified by an SU(2)$_D$…

High Energy Physics - Phenomenology · Physics 2022-01-24 Chengfeng Cai , Hong-Hao Zhang

Some extensions of the Standard Model provide Dark Matter candidate particles with sub-GeV mass. These Light Dark Matter particles have been considered for example in Warm Dark Matter scenarios (e.g. the keV scale sterile neutrino, axino or…

We propose a new strategy to directly detect light particle dark matter that has long-ranged interactions with ordinary matter. The approach involves distorting the local flow of dark matter with time-varying fields and measuring these…

High Energy Physics - Phenomenology · Physics 2020-01-08 Asher Berlin , Raffaele Tito D'Agnolo , Sebastian A. R. Ellis , Philip Schuster , Natalia Toro

We use Super-K data to place new strong limits on interactions of sub-GeV Dark Matter (DM) with nuclei, that rely on the DM flux inevitably induced by cosmic-ray upscatterings. We derive analogous sensitivities at Hyper-K and DUNE and…

High Energy Physics - Phenomenology · Physics 2021-03-24 Yohei Ema , Filippo Sala , Ryosuke Sato

Dark matter (DM) is added to the Froggatt-Nielsen (FN) mechanism, and conditions for its successful freezeout identified. Requesting the FN scale $\Lambda_{\text{FN}}$ to be the cutoff of the theory renders freezeout scenarios surprisingly…

High Energy Physics - Phenomenology · Physics 2017-10-04 Carlos Alvarado , Fatemeh Elahi , Nirmal Raj

Searches for dark matter (DM) have not provided any solid evidence for the existence of weakly interacting massive particles in the GeV-TeV mass range. Coincidentally, the scale of new physics is being pushed by collider searches well…

High Energy Astrophysical Phenomena · Physics 2022-07-06 A. Albert , S. Alves , M. Andre , M. Anghinolfi , G. Anton , M. Ardid , S. Ardid , J. -J. Aubert , J. Aublin , B. Baret , S. Basa , B. Belhorma , M. Bendahman , F. Benfenati , V. Bertin , S. Biagi , M. Bissinger , J. Boumaaza , M. Bouta , M. C. Bouwhuis , H. Branzas , R. Bruijn , J. Brunner , J. Busto , B. Caiffi , D. Calvo , A. Capone , L. Caramete , J. Carr , V. Carretero , S. Celli , M. Chabab , T. N. Chau , R. Cherkaoui El Moursli , T. Chiarusi , M. Circella , A. Coleiro , R. Coniglione , P. Coyle , A. Creusot , A. F. Diaz , G. de Wasseige , C. Distefano , I. Di Palma , A. Domi , C. Donzaud , D. Dornic , D. Drouhin , T. Eberl , T. van Eeden , D. van Eijk , N. El Khayati , A. Enzenhoefer , P. Fermani , G. Ferrara , F. Filippini , L. Fusco , Y. Gatelet , P. Gay , H. Glotin , R. Gozzini , R. Gracia Ruiz , K. Graf , C. Guidi , S. Hallmann , H. van Haren , A. J. Heijboer , Y. Hello , J. J. Hernandez-Rey , J. Hoessl , J. Hofestaedt , F. Huang , G. Illuminati , C. W. James , B. Jisse-Jung , M. de Jong , P. de Jong , M. Kadler , O. Kalekin , U. Katz , N. R. Khan-Chowdhury , A. Kouchner , I. Kreykenbohm , V. Kulikovskiy , C. Lagunas Gualda , R. Lahmann , R. Le Breton , S. LeStum , D. Lefevre , E. Leonora , G. Levi , M. Lincetto , D. Lopez-Coto , S. Loucatos , L. Maderer , J. Manczak , M. Marcelin , A. Margiotta , A. Marinelli , J. A. Martinez-Mora , B. Martino , K. Melis , P. Migliozzi , A. Moussa , R. Muller , L. Nauta , S. Navas , E. Nezri , B. O Fearraigh , A. Paun , G. E. Pavalas , C. Pellegrino , M. Perrin-Terrin , V. Pestel , P. Piattelli , C. Pieterse , C. Poire , V. Popa , T. Pradier , N. Randazzo , D. Real , S. Reck , G. Riccobene , A. Romanov , F. Sala , A. Sanchez-Losa , F. Salesa Greus , D. F. E. Samtleben , M. Sanguineti , P. Sapienza , J. Schnabel , J. Schumann , F. Schuessler , J. Seneca , M. Spurio , Th. Stolarczyk , M. Taiuti , Y. Tayalati , S. J. Tingay , B. Vallage , V. Van Elewyck , F. Versari , S. Viola , D. Vivolo , J. Wilms , S. Zavatarelli , A. Zegarelli , J. D. Zornoza , J. Zuniga

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…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Benjamin Zitzer

DarkSHINE is an electron fixed target experiment under proposal that aims to probe light dark matter in the MeV-GeV mass range via the invisible decay of dark photons, leveraging the High repetition rate 8 GeV electron beam from the…

High Energy Physics - Experiment · Physics 2025-12-16 Haijun Yang

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…

High Energy Physics - Phenomenology · Physics 2020-12-02 Qing-Hong Cao , An-Kang Wei , Qian-Fei Xiang

We reappraise the viability of asymmetric dark matter (ADM) realized as a Dirac fermion coupling dominantly to the Standard Model fermions. Treating the interactions of such a DM particle with quarks/leptons in an effective-interactions…

High Energy Physics - Phenomenology · Physics 2024-07-19 Arnab Roy , Basudeb Dasgupta , Monoranjan Guchait

Direct detection experiments are the only way to obtain indisputable evidence of the existence of dark matter (DM) in the form of a particle. These experiments have been used to probe many extensions of the Standard Model (SM) that provide…

High Energy Physics - Phenomenology · Physics 2022-08-03 Seraina Glaus , Margarete Mühlleitner , Jonas Müller , Shruti Patel , Rui Santos

The dark photon is a new hypothetical gauge boson arising in extensions of the Standard Model, and constitutes a compelling dark matter candidate. As dark photon dark matter (DPDM), it can interact with electromagnetic fields via kinetic…

High Energy Astrophysical Phenomena · Physics 2026-02-26 Júlia G. Mamprim , Aion Viana , Vitor de Souza

We study dark matter (DM) models in which there are two dark sector particles, $\chi_1$ and $\chi_2$, of near mass. In such models, co-annihilation of $\chi_1$ and $\chi_2$ may be the dominant process controlling the DM relic density during…

High Energy Physics - Phenomenology · Physics 2014-07-02 Nicole F. Bell , Yi Cai , Anibal D. Medina

Astrophysical and cosmological observations strongly suggest the existence of Dark Matter\,(DM). Experiments at the Large Hadron Collider\,(LHC) have the potential to probe the particle nature of the DM. In the present work, we investigate…

High Energy Physics - Phenomenology · Physics 2025-04-18 Sweta Baradia , Sanchari Bhattacharyya , Anindya Datta , Suchandra Dutta , Suvankar Roy Chowdhury , Subir Sarkar

Driven by the null results in the searches for dark matter, the field of direct dark matter detection is constantly evolving to push new frontiers. Ultimately, a vast parameter space for dark matter masses below a few GeV is yet to be…

High Energy Physics - Experiment · Physics 2025-12-18 Melih Solmaz

In light of recent DAMIC-M results, we present the status of thermal-relic dark matter $\chi$ coupled to a kinetically-mixed dark photon $A^\prime$. In the predictive "direct annihilation" regime, $m_{A'} > m_\chi$, the relic abundance…

High Energy Physics - Phenomenology · Physics 2025-05-08 Gordan Krnjaic

Up to now searches for Dark Matter (DM) detection have not been successful, either because our paradigm in how DM signals should look like are wrong or the detector sensitivity is still too low in spite of the large progress made in recent…

High Energy Physics - Phenomenology · Physics 2017-12-20 Wim de Boer

We explore simplified models of mixed dark matter (DM), defined here to be a stable relic composed of a singlet and an electroweak charged state. Our setup describes a broad spectrum of thermal DM candidates that can naturally accommodate…

High Energy Physics - Phenomenology · Physics 2014-02-12 Clifford Cheung , David Sanford

Dark matter (DM) could be a relic of freeze-in through a light mediator, where the DM is produced by extremely feeble, IR-dominated processes in the thermal Standard Model plasma. In the simplest viable models with the DM mass below the MeV…

Cosmology and Nongalactic Astrophysics · Physics 2021-09-15 Cora Dvorkin , Tongyan Lin , Katelin Schutz

We present Self-Destructing Dark Matter (SDDM), a new class of dark matter models which are detectable in large neutrino detectors. In this class of models, a component of dark matter can transition from a long-lived state to a short-lived…

High Energy Physics - Phenomenology · Physics 2019-07-04 Yuval Grossman , Roni Harnik , Ofri Telem , Yue Zhang
‹ Prev 1 4 5 6 7 8 10 Next ›