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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, with a weakly interacting massive particle (WIMP)…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Matthieu Vivier

The cold dark matter (CDM) cosmological model unambigously predicts that a large number of haloes should survive as subhaloes when they are accreted into a larger halo. The CDM model would be ruled out if such substructures were shown not…

Cosmology and Nongalactic Astrophysics · Physics 2016-04-27 Ran Li , Carlos S. Frenk , Shaun Cole , Liang Gao , Sownak Bose , Wojciech A. Hellwing

We study the possibility of testing a dark matter (DM) scenario embedded in a global lepton number symmetry $U(1)_L$ via gravitational waves (GW) and cosmic microwave background (CMB) observations. The spontaneous breaking of $U(1)_L$…

High Energy Physics - Phenomenology · Physics 2024-10-14 Debasish Borah , Nayan Das , Rishav Roshan

Dark Matter (DM) comprising particles in the mass range of a few MeV to GeV is waiting to be explored, given the many theoretical models accommodating cosmological abundance. We hereby propose an experiment with the LHC proton beam of 7 TeV…

High Energy Physics - Experiment · Physics 2016-09-04 Ashok Kumar , Archana Sharma

We study a minimally extended version of the Standard Model where baryon number is gauged with a $U(1)_B$ symmetry. This model can be made anomaly-free by adding a set of additional fermions. The lightest component of these fermions behaves…

High Energy Physics - Phenomenology · Physics 2025-08-26 Taramati , Lekhika Malhotra , Zafri A. Borboruah , Sudhanwa Patra

We propose a new extension of the Standard Model that incorporates a gauged \( U(1)_{\rm B-L} \) symmetry and the type-III seesaw mechanism to explain neutrino mass generation and provide a viable dark matter (DM) candidate. Unlike the…

High Energy Physics - Phenomenology · Physics 2026-01-27 Satyabrata Mahapatra , Partha Kumar Paul , Narendra Sahu , Prashant Shukla

Sterile neutrinos with the mass in the keV range are interesting warm dark matter (WDM) candidates. The restrictions on their parameters (mass and mixing angle) obtained by current X-ray missions (XMM-Newton or Chandra) can only be improved…

Astrophysics · Physics 2008-11-26 Alexey Boyarsky , Jan Willem den Herder , Andrey Neronov , Oleg Ruchayskiy

Since the pioneering detection of gravitational wave (GW) from a binary black hole merger by the LIGO-Virgo collaboration, GW has become a powerful probe for astrophysics and cosmology. If compact dark matter (DM) candidates, e.g.…

Cosmology and Nongalactic Astrophysics · Physics 2025-11-04 Xin-Yi Lin , Xi-Jing Wang , Huan Zhou , Zhengxiang Li , Kai Liao , Zong-Hong Zhu

We point out that current and planned telescopes have the potential of probing annihilating Dark Matter (DM) with a mass of O(100) TeV and beyond. As a target for such searches, we propose models where DM annihilates into lighter mediators,…

High Energy Physics - Phenomenology · Physics 2019-02-20 Marco Cirelli , Yann Gouttenoire , Kalliopi Petraki , Filippo Sala

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…

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

The precision measurements of the muon magnetic moment and the $W$ boson mass have sparked interest in the potential deviations from standard model (SM) predictions. While it may be premature to attribute any excesses in these precision…

High Energy Physics - Phenomenology · Physics 2026-01-05 Yi-Zhong Fan , Yao-Yu Li , Chih-Ting Lu , Xiao-Yi Luo , Tian-Peng Tang , Van Que Tran , Yue-Lin Sming Tsai

Ultralight Dark Matter (ULDM) offers an alternative to cold dark matter, characterized by wavelike behavior on galactic scales. This contribution summarizes our work~\cite{Blas:2024duy} on how solitonic cores induced by ULDM affect…

High Energy Astrophysical Phenomena · Physics 2025-03-07 Silvia Gasparotto

In a large class of scenarios, dark matter (DM) particles that belong to a multiplet of the standard model (SM) weak interactions are challenging to probe in direct detection experiments due to loop-suppressed cross-sections. Direct…

High Energy Physics - Phenomenology · Physics 2019-04-15 Tao Han , Satyanarayan Mukhopadhyay , Xing Wang

Some direct detection experiments have recently collected excess events that could be interpreted as a dark matter (DM) signal, pointing to particles in the $\sim$10 GeV mass range. We show that scenarios in which DM can self-annihilate…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Julien Lavalle

A new vector dark matter (DM) scenario in the context of the gauge-Higgs unification (GHU) is proposed. The DM particle is identified with an electric-charge neutral component in an $SU(2)_L$ doublet vector field with the same quantum…

High Energy Physics - Phenomenology · Physics 2018-10-31 Nobuhito Maru , Nobuchika Okada , Satomi Okada

The lightest neutralino, assumed to be the lightest supersymmetric particle, is proposed to be a dark matter (DM) candidate for the mass $\cal{O}$(100) GeV. Constraints from various direct dark matter detection experiments and Planck…

High Energy Physics - Phenomenology · Physics 2021-09-29 Monoranjan Guchait , Arnab Roy , Seema Sharma

Recent gravitational-wave (GW) observations offer a unique opportunity to probe the fundamental nature of compact objects. A growing body of research has focused on exploring the role of dark matter (DM) through the concept of DM-admixed…

General Relativity and Quantum Cosmology · Physics 2026-03-18 Rafael M. Santos , Rafael C. Nunes , Jaziel G. Coelho , Jose C. N. de Araujo

Supermassive black hole binaries source gravitational waves measured by Pulsar Timing Arrays. The frequency spectrum of this stochastic background is predicted more precisely than its amplitude. We argue that Dark Matter friction can…

Cosmology and Nongalactic Astrophysics · Physics 2023-07-04 Anish Ghoshal , Alessandro Strumia

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, with a weakly interacting massive particle (WIMP)…

High Energy Astrophysical Phenomena · Physics 2019-08-14 B. Zitzer

We consider an extended seesaw model which generates active neutrino masses via the usual type-I seesaw and leads to a large number of massless fermions as well as a sterile neutrino dark matter (DM) candidate in the $\mathcal{O}(10-100)…

High Energy Physics - Phenomenology · Physics 2025-04-22 Cristina Benso , Thomas Schwetz , Drona Vatsyayan