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The nature of dark matter remains one of the most profound mysteries in modern physics. In this work, we investigate the phenomenological implications of ultralight scalar dark matter (ULDM) coupled to neutrinos. We focus on a large…

高能物理 - 唯象学 · 物理学 2025-12-23 Luis A. Delgadillo , O. G. Miranda , Hiroshi Nunokawa

The dark matter conundrum stands out as one of the central challenges to understand in both particle physics and cosmology. The ultralight axion-like particle (UALP) is an appealing dark matter candidate that can be searched for in neutrino…

高能物理 - 唯象学 · 物理学 2024-12-13 Rubén Cordero , Luis A. Delgadillo

We discuss the use of atom interferometry as a tool to search for Dark Matter (DM) composed of ultra-light scalar fields. Previous work on ultra-light DM detection using accelerometers has considered the possibility of equivalence principle…

原子物理 · 物理学 2016-12-28 Andrew A. Geraci , Andrei Derevianko

Sterile neutrinos at the eV scale have long been studied in the context of anomalies in short baseline neutrino experiments. Their cosmology can be made compatible with our understanding of the early Universe provided the sterile neutrino…

高能物理 - 唯象学 · 物理学 2017-07-26 Francesco Capozzi , Ian M. Shoemaker , Luca Vecchi

Ultralight dark matter (ULDM), as a class of low mass (< 1 eV) dark matter (DM) candidates, is a compelling alternative to historically dominant models such as WIMPs and has recently gained significant attention in the scientific community.…

高能物理 - 唯象学 · 物理学 2024-11-22 Jordan Gué

Ultralight dark matter (ULDM) is one of the leading well-motivated dark matter candidates, predicted in many theories beyond the standard model of particle physics and cosmology. There have been increasing interests in searching for ULDM in…

高能物理 - 唯象学 · 物理学 2024-10-11 Jiang-Chuan Yu , Yan Cao , Yong Tang , Yue-Liang Wu

The European Spallation Source (ESS), currently finishing its construction, will soon provide the most intense neutron beams for multi-disciplinary science. At the same time, it will also produce a high-intensity neutrino flux with an…

高能物理 - 唯象学 · 物理学 2021-05-12 Ivan Esteban

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…

高能天体物理现象 · 物理学 2025-03-07 Silvia Gasparotto

We study the prospect of heavy singlet neutrinos as a dark matter (DM) candidate within a neutrinophilic U(1) model, where the Standard Model (SM) is extended with a U(1) gauge symmetry, and neutrino mass and oscillation parameters are…

高能物理 - 唯象学 · 物理学 2024-05-27 Waleed Abdallah , Anjan Kumar Barik , Santosh Kumar Rai , Tousik Samui

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…

高能物理 - 唯象学 · 物理学 2021-03-24 Yohei Ema , Filippo Sala , Ryosuke Sato

If neutrinos get mass through the exchange of lepton mediators, as in seesaw schemes, the neutrino appearance probabilities in oscillation experiments are modified due to effective nonunitarity of the lepton mixing matrix. This also leads…

高能物理 - 唯象学 · 物理学 2022-11-02 Sabya Sachi Chatterjee , O. G. Miranda , M. Tórtola , J. W. F. Valle

In this thesis, we investigate the possibility that dark matter consists of ultra light spin-zero particles with mass $m \sim 10^{-22}\ \text{eV}$. We focus on the role of self-interactions, assuming all other non-gravitational couplings to…

宇宙学与河外天体物理 · 物理学 2026-01-01 Bihag Dave

The scattering of neutrinos off dark matter can induce time delays in their propagation compared to that of photons, which would wash out correlations between ultra-high-energy neutrinos and electromagnetic observations of their sources -…

高能物理 - 唯象学 · 物理学 2019-09-11 Seth Koren

In this work, we study the propagation of high energy neutrinos produced in extragalactic sources including the effect of a possible interaction with ultralight axion-like particles (UALP) with a mass $m_a\sim 10^{-22} {\rm eV}$ as the…

高能物理 - 唯象学 · 物理学 2022-04-20 Matías M. Reynoso , Oscar A. Sampayo , Agustín M. Carulli

The upcoming European Spallation Source (ESS) will soon provide the most intense neutrino source in the world. We propose the Search for Hidden Neutrinos at the ESS (SHiNESS) experiment, highlighting its unique opportunities to search for…

高能物理 - 实验 · 物理学 2025-05-28 Stefano Roberto Soleti , Pilar Coloma , Juan Jose Gómez Cadenas , Anatael Cabrera

Next-generation ultra-high-energy (UHE) neutrino telescopes, presently under planning, will have the potential to probe the decay of heavy dark matter (DM) into UHE neutrinos, with energies in excess of $10^7$~GeV. Yet, this potential may…

高能天体物理现象 · 物理学 2023-12-13 Damiano F. G. Fiorillo , Victor Valera , Mauricio Bustamante , Walter Winter

Sub-GeV thermal dark matter weakly interacting with the Standard Model through vector-portal mediators provides a well-motivated and predictive framework that remains challenging to probe with conventional direct detection experiments.…

高能物理 - 唯象学 · 物理学 2026-03-23 D. Aristizabal Sierra , V. De Romeri , D. K. Papoulias , G. Sanchez Garcia

The effects of scalar and pseudoscalar ultralight bosonic dark matter (UBDM) were searched for by comparing the frequency of a quartz oscillator to that of a hyperfine-structure transition in $^{87}$Rb, and an electronic transition in…

We propose to search for (ultra)-light scalar dark matter (DM) using synchrotron radiation based M\"ossbauer spectroscopy technique. Such DM induces temporal variation in various fundamental constants, which in turn causes time modulation…

高能物理 - 唯象学 · 物理学 2024-08-12 Abhishek Banerjee

We consider optical fibers as detectors for scalar ultralight dark matter (UDM) and propose using a fiber-based interferometer to search for scalar UDM with particle mass in the range $10^{-17} - 10^{-13}$ eV/$c^2$ $\left(10^{-3}- 10 \text{…

高能物理 - 唯象学 · 物理学 2023-05-22 J. Manley , R. Stump , R. Petery , and S. Singh
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