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We study the gravitational collapse of axion dark matter fluctuations in the post-inflationary scenario, so-called axion miniclusters, with N-body simulations. Largely confirming theoretical expectations, overdensities begin to collapse in…

宇宙学与河外天体物理 · 物理学 2020-07-22 Benedikt Eggemeier , Javier Redondo , Klaus Dolag , Jens C. Niemeyer , Alejandro Vaquero

Dark matter as scalar particles consisting of multiple species is well motivated in string theory where axion fields are ubiquitous. A two-field fuzzy dark matter (FDM) model features two species of ultralight axion particles with different…

宇宙学与河外天体物理 · 物理学 2024-02-01 Hoang Nhan Luu , Philip Mocz , Mark Vogelsberger , Simon May , Josh Borrow , S. -H. Henry Tye , Tom Broadhurst

We derive from first principles equations for bosonic, non-relativistic and self-interacting dark matter which can include both a condensed, low momentum "fuzzy" component and one with higher momenta that may be approximated as a collection…

宇宙学与河外天体物理 · 物理学 2023-09-21 Nick P. Proukakis , Gerasimos Rigopoulos , Alex Soto

The cosmic large-scale structures of the Universe are mainly the result of the gravitational instability of initially small density fluctuations in the dark-matter distribution. Dark matter appears to be initially cold and behaves as a…

宇宙学与河外天体物理 · 物理学 2021-11-09 Cornelius Rampf

Self-gravitating bosonic fields can support stable and localised field configurations. For real fields, these solutions oscillate in time and are known as oscillatons. The density profile is static, and is soliton. Such solitons should be…

宇宙学与河外天体物理 · 物理学 2015-06-18 David J. E. Marsh , Ana-Roxana Pop

We investigate the effect of self-interactions on the shape and oscillations of the solitonic core profile of condensed fuzzy dark matter systems without the backdrop of a halo, revealing universal features in terms of an appropriately…

宇宙学与河外天体物理 · 物理学 2025-02-26 Milos Indjin , I-Kang Liu , Nick P. Proukakis , Gerasimos Rigopoulos

We initiate a systematic study of the perturbative nonlinear dynamics of cosmological fluctuations in dark sectors comprising a fraction of non-cold dark matter, for example ultra-light axions or light thermal relics. These mixed dark…

宇宙学与河外天体物理 · 物理学 2026-02-02 Francesco Verdiani , Emanuele Castorina , Ennio Salvioni , Emiliano Sefusatti

The subjects of this thesis are the invisible axion and the more general family of axion-like particles. The invisible axion is a hypothetical elementary particle and a cold dark matter candidate. I present an improved computation of the…

宇宙学与河外天体物理 · 物理学 2011-11-23 Luca Visinelli

Non-relativistic QCD axions or axion-like particles are among the most popular candidates for cold Dark Matter (DM) in the universe. We proposed to detect axion-like DM, using linearly polarized pulsar light as a probe. Because of…

宇宙学与河外天体物理 · 物理学 2020-03-18 Tao Liu , George Smoot , Yue Zhao

One of the challenging questions in cosmology is the nature of dark matter particles. Fuzzy Dark Matter (FDM) is one of the candidates which is made of very light ($m_{FDM}\simeq 10^{-22}-10^{-21}$ eV) bosonic particles with no…

宇宙学与河外天体物理 · 物理学 2020-01-22 Alireza Maleki , Shant Baghram , Sohrab Rahvar

We report on a search for ultra-low-mass axion-like dark matter by analysing the ratio of the spin-precession frequencies of stored ultracold neutrons and $^{199}$Hg atoms for an axion-induced oscillating electric dipole moment of the…

高能物理 - 实验 · 物理学 2018-05-28 N. J. Ayres

We study fuzzy axion dark matter in type IIB string theory, for axions descending from the Ramond-Ramond four-form in compactifications on orientifolds of Calabi-Yau hypersurfaces. Such models can be tested by cosmological measurements if a…

Existence of dark matter indicates the presence of unknown fundamental laws of nature. Ultralight axion-like particles are well-motivated dark matter candidates, emerging naturally from theories of physics at ultrahigh energies. We report…

高能物理 - 实验 · 物理学 2021-01-11 Alexander V. Gramolin , Deniz Aybas , Dorian Johnson , Janos Adam , Alexander O. Sushkov

Axion-like dark matter whose symmetry breaking occurs after the end of inflation predicts enhanced primordial density fluctuations at small scales. This leads to dense axion minihalos (or miniclusters) forming early in the history of the…

高能物理 - 唯象学 · 物理学 2023-11-28 Patrick J. Fox , Neal Weiner , Huangyu Xiao

We revisit the generation of dark matter isocurvature perturbations in the curvaton model in greater detail, both analytically and numerically. As concrete examples, we investigate the cases of thermally decoupled dark matter and axionic…

宇宙学与河外天体物理 · 物理学 2018-01-10 Naoya Kitajima , David Langlois , Tomo Takahashi , Shuichiro Yokoyama

The velocity distribution of cold dark matter within galaxies is expected to exhibit ultra-fine-grained substructure as a result of the many foldings of an initially smooth phase-space sheet under gravity. The innumerable folds of this…

高能物理 - 唯象学 · 物理学 2025-09-19 Ciaran A. J. O'Hare , Giovanni Pierobon

We present an in-depth exploration of the phenomenon of dynamical friction in a universe where the dark matter is composed entirely of so-called Fuzzy Dark Matter (FDM), ultralight bosons of mass $m\sim\mathcal{O}(10^{-22})\,$eV. We review…

宇宙学与河外天体物理 · 物理学 2020-01-15 Lachlan Lancaster , Cara Giovanetti , Philip Mocz , Yonatan Kahn , Mariangela Lisanti , David N. Spergel

We extend our previous work (Proukakis {\em et al.}, Phys.~Rev.~D~108,~083513 (2023)) on the dynamics of bosonic, non-relativistic and self-interacting dark matter that simultaneously contains both a ``fuzzy'' low-momentum component and one…

宇宙学与河外天体物理 · 物理学 2024-12-18 Nick P. Proukakis , Gerasimos Rigopoulos , Alex Soto

We consider the production of axion dark matter through the misalignment mechanism in the context of a nonstandard cosmological history involving early matter domination by a scalar field with a time-dependent decay rate. In cases where the…

高能物理 - 唯象学 · 物理学 2023-05-24 Paola Arias , Nicolás Bernal , Jacek K. Osiński , Leszek Roszkowski

AI super-resolution, combining deep learning and N-body simulations has been shown to successfully reproduce the large scale structure and halo abundances in the Lambda Cold Dark Matter cosmological model. Here, we extend its use to models…

宇宙学与河外天体物理 · 物理学 2023-08-16 Meris Sipp , Patrick LaChance , Rupert Croft , Yueying Ni , Tiziana Di Matteo