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Related papers: Ultralight Dark Matter -- A Novel proposal

200 papers

The mass of the dark matter particle is unknown, and may be as low as ~$10^{-22}$ eV. The lighter part of this range, below ~eV, is relatively unexplored both theoretically and experimentally but contains an array of natural dark matter…

High Energy Physics - Phenomenology · Physics 2016-04-27 Peter W. Graham , David E. Kaplan , Jeremy Mardon , Surjeet Rajendran , William A. Terrano

We propose that the ultralight dark matter (ULDM) model, in which dark matter particles have a tiny mass of $m=O(10^{-22})eV$, has characteristic scales for physical quantities of observed galaxies such as mass, size, acceleration, mass…

Astrophysics of Galaxies · Physics 2025-04-24 Jae-Weon Lee

There is a strong possibility that the particles making up the dark matter in the Universe have a mass below 1 eV and in many important situations exhibit a wave-like behavior. Amongst the candidates the axion stands out as particularly…

High Energy Physics - Phenomenology · Physics 2022-09-20 Joerg Jaeckel , Gray Rybka , Lindley Winslow

It has been proposed that an additional U(1) sector of hidden photons could account for the Dark Matter observed in the Universe. When passing through an interface of materials with different dielectric properties, hidden photons can give…

The nature of dark matter remains obscure in spite of decades of experimental efforts. The mass of dark matter candidates can span a wide range, and its coupling with the Standard Model sector remains uncertain. All these unknowns make the…

It is now widely accepted that most of mass--energy in the universe is unobserved except by its gravitational effects. Baryons make only about 4% of the total, with "dark matter" making up about 23% and the "dark energy" responsible for the…

Astrophysics · Physics 2007-05-23 Edward A. Baltz

This is a review on the brief history of the scalar field dark matter model also known as fuzzy dark matter, BEC dark matter, wave dark matter, or ultra-light axion. In this model ultra-light scalar dark matter particles with mass $m =…

Cosmology and Nongalactic Astrophysics · Physics 2018-01-24 Jae-Weon Lee

An ultralight scalar boson with mass $m_1 \simeq 10^{-22}$ eV is gaining credence as a Dark Matter (DM) candidate that explains the dark cores of dwarf galaxies as soliton waves. Such a boson is naturally interpreted as an axion generic in…

Astrophysics of Galaxies · Physics 2021-02-24 Hoang Nhan Luu , S. -H. Henry Tye , Tom Broadhurst

We discuss novel ways in which neutrino oscillation experiments can probe dark matter. In particular, we focus on interactions between neutrinos and ultra-light ("fuzzy") dark matter particles with masses of order $10^{-22}$ eV. It has been…

High Energy Physics - Phenomenology · Physics 2018-02-05 Vedran Brdar , Joachim Kopp , Jia Liu , Pascal Prass , Xiao-Ping Wang

In this letter, we propose a new model of fuzzy dark matter based on Stueckelberg theory. Dark matter is treated as a Bose-Einstein condensate of Stueckelberg particles and the resulting cosmological effects are analyzed. Fits are…

High Energy Physics - Phenomenology · Physics 2019-10-15 T. R. Govindarajan , Nikhil Kalyanapuram

Fuzzy Dark Matter (FDM) is one of the recent models for dark matter. According to this model, dark matter is made of very light scalar particles with considerable quantum mechanical effects on the galactic scale, which solves many problems…

Astrophysics of Galaxies · Physics 2020-05-13 Alireza Maleki , Shant Baghram , Sohrab Rahvar

Dark matter is one of the pillars of the current standard model of structure formation: it is assumed to constitute most of the matter in the Universe. However, it can so far only be probed indirectly through its gravitational effects, and…

We review dark matter (DM) candidates of a very low mass, appearing in the window below the traditional weakly-interacting massive particle $m_\chi \lesssim 10$ GeV and extending down to $m_\chi \gtrsim 1$ meV, somewhat below the mass limit…

High Energy Physics - Phenomenology · Physics 2025-02-25 Kathryn M. Zurek

We model the 21cm power spectrum across the Cosmic Dawn and the Epoch of Reionization (EoR) in fuzzy dark matter (FDM) cosmologies. The suppression of small mass halos in FDM models leads to a delay in the onset redshift of these epochs…

Cosmology and Nongalactic Astrophysics · Physics 2021-05-26 Dana Jones , Skyler Palatnick , Richard Chen , Angus Beane , Adam Lidz

In this article we address the mystery of dark matter. We expound the various evidences, astrophysical and cosmological, leading to hypothesize the existence of an invisible form of matter, whose attempts at detecting it have so far all…

General Relativity and Quantum Cosmology · Physics 2024-10-15 Sergio Luigi Cacciatori , Vittorio Gorini , Federico Re

Numerous observations point towards the existence of an unknown elementary particle with no electromagnetic interactions, a large population of which was presumably produced in the early stages of the history of the Universe. This so-called…

High Energy Physics - Phenomenology · Physics 2015-06-16 Alejandro Ibarra , David Tran , Christoph Weniger

Cold Dark Matter (CDM) models struggle to match the observations at galactic scales. The tension can be reduced either by dramatic baryonic feedback effects or by modifying the particle physics of CDM. Here, we consider an ultra-light…

Cosmology and Nongalactic Astrophysics · Physics 2016-07-27 Erminia Calabrese , David N. Spergel

We propose a new dark matter contender within the context of the so-called ``dark dimension'', an innovative 5-dimensional construct that has a compact space with characteristic length-scale in the micron range. The new dark matter…

High Energy Physics - Phenomenology · Physics 2024-03-19 Luis A. Anchordoqui , Ignatios Antoniadis , Dieter Lust

Using a single gravitational lens system observed at $\lesssim5$ milli-arcsecond resolution with very long baseline interferometry (VLBI), we place a lower bound on the mass of the fuzzy dark matter (FDM) particle, ruling out $m_\chi \leq…

Cosmology and Nongalactic Astrophysics · Physics 2023-06-28 Devon M. Powell , Simona Vegetti , J. P. McKean , Simon D. M. White , Elisa G. M. Ferreira , Simon May , Cristiana Spingola

Within the standard cosmological scenario the Universe is found to be filled by obscure components (dark matter and dark energy) for ~95% of its energy budget. In particular, almost all the matter content in the Universe is given by dark…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 Crescenzo Tortora , Philippe Jetzer , Nicola R. Napolitano