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相关论文: Late Time Magnetogenesis from Ultralight Scalar Da…

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We propose a mechanism for the generation of magnetic fields on cosmological scales that is operative after recombination. An essential ingredient is an instability (of parametric resonance type) of the electromagnetic field driven by an…

高能物理 - 唯象学 · 物理学 2025-02-27 Robert Brandenberger , Jürg Fröhlich , Hao Jiao

We discuss the possibility that dark matter is made of a new complex massive vector field with a global $U(1)$-symmetry. The field interacts with the Standard Model via coupling to the gauge field of the hypercharge group. We study…

高能物理 - 唯象学 · 物理学 2020-04-30 Emin Nugaev , Andrey Shkerin

Oscillating ultra-light scalar fields are a natural explanation for the dark matter in our universe, as long as a mechanism, often called a misalignment mechanism, exists to explain the amplitude of the scalar oscillations. If the dark…

高能物理 - 唯象学 · 物理学 2026-04-01 Clare Burrage , Sergio Sevillano Muñoz

It has been hypothesized that dark matter is comprised of ultra-light bosons whose collective phenomena can be described as a scalar field undergoing coherent oscillations. Examples include axion and fuzzy dark matter models. In this…

高能物理 - 唯象学 · 物理学 2023-05-08 Jeremy Sakstein , Ippocratis D. Saltas

Recently, a mechanism for generating astrophysically relevant magnetic fields via ultralight pseudoscalar dark matter, through the coupling term $g_{\phi \gamma} \phi F_{\mu \nu}\tilde{F}^{\mu\nu}$ in the Lagrangian density, was proposed in…

宇宙学与河外天体物理 · 物理学 2026-04-21 Ramkishor Sharma , Samarth Majumdar , Divya Sachdeva

We consider Dark Matter composed of an oscillating singlet scalar field. On top of the mass term, the scalar is equipped with a potential spontaneously breaking Z_2-symmetry. This potential dominates at early times and leads to the…

高能物理 - 唯象学 · 物理学 2020-10-02 Eugeny Babichev , Dmitry Gorbunov , Sabir Ramazanov

We present a scenario in which a scalar field dark energy is coupled to the trace of the energy momentum tensor of the baryonic matter fields. In the slow-roll regime, this interaction could give rise to the cosmological features of dark…

宇宙学与河外天体物理 · 物理学 2011-02-02 Alejandro Aviles , Jorge L. Cervantes-Cota

We consider ultralight scalar dark matter that couples to right-handed neutrinos. Due to the high density of neutrinos in the early universe, the background neutrino density dominates the dynamics of the scalar field, and qualitatively…

高能物理 - 唯象学 · 物理学 2025-02-05 Ryan Plestid , Sophia Tevosyan

The existence of dark energy is essential to explain the cosmic accelerated expansion. We consider a homogenous interacting tachyonic scalar field as a possible candidate for the dynamical dark energy. The interaction between the tachyonic…

广义相对论与量子宇宙学 · 物理学 2023-05-02 V K Ojha , Adithya A Rao , S D Pathak

We discuss the coupling between dark energy and matter by considering a homogeneous tachyonic scalar field as a candidate for dark energy. We obtained the functional form of scale factor by assuming that the coupling strength depends…

广义相对论与量子宇宙学 · 物理学 2021-01-27 A Kundu , S D Pathak , V K Ojha

Dark Matter might be an accidentally stable baryon of a new confining gauge interaction. We extend previous studies exploring the possibility that the DM is made of dark quarks heavier than the dark confinement scale. The resulting…

高能物理 - 唯象学 · 物理学 2017-11-21 Andrea Mitridate , Michele Redi , Juri Smirnov , Alessandro Strumia

Primordial magnetic fields are often thought to be the early Universe seeds that have bloomed into what we observe today as galactic and extra-galactic magnetic fields. Owing to their minuscule strength, primordial magnetic fields are very…

宇宙学与河外天体物理 · 物理学 2021-02-11 Sabir Ramazanov , Federico R. Urban , Alexander Vikman

We investigate primordial magnetogenesis within a quantum bouncing model driven by a scalar field, focusing on various non-minimal couplings between the electromagnetic field and the scalar field. We test three cases: no coupling, a Cauchy…

广义相对论与量子宇宙学 · 物理学 2024-11-06 Marcus V. Bomfim , Emmanuel Frion , Nelson Pinto-Neto , Sandro D. P. Vitenti

Despite the success of Maxwell's electromagnetism in the description of the electromagnetic interactions on small scales, we know very little about the behaviour of electromagnetic fields on cosmological distances. Thus, it has been…

宇宙学与河外天体物理 · 物理学 2011-12-07 Jose Beltran Jimenez , Antonio L. Maroto

We take a more detailed look at the recently proposed magnetogenesis mechanism triggered by ultralight dark matter coupled to electromagnetism. The proposed mechanism made use of a tachyonic resonance channel which leads to the exponential…

宇宙学与河外天体物理 · 物理学 2026-02-05 Nirmalya Brahma , Robert Brandenberger

We study in detail the recently proposed mechanism of generating superheavy Dark Matter with the mass larger than the Hubble rate at the end of inflation. A real scalar field constituting Dark Matter linearly couples to the inflaton. As a…

高能物理 - 唯象学 · 物理学 2019-06-04 Eugeny Babichev , Dmitry Gorbunov , Sabir Ramazanov

We review the gauged quintessence scenario, wherein the quintessence scalar field responsible for dark energy is promoted to a complex field charged under a dark $U(1)$ gauge symmetry. This construction leads to new and potentially rich…

高能物理 - 唯象学 · 物理学 2025-08-08 Kunio Kaneta , Hye-Sung Lee , Jiheon Lee , Jaeok Yi

Despite growing interest and extensive effort to search for ultralight dark matter in the form of a hypothetical dark photon, how it fits into a consistent cosmology is unclear. Several dark photon dark matter production mechanisms proposed…

高能物理 - 唯象学 · 物理学 2019-05-03 Raymond T. Co , Aaron Pierce , Zhengkang Zhang , Yue Zhao

This paper consider an universe dominated by baryonic matter, radiation and a nonminimally coupled massive scalar field under the action of a symmetry breaking potential. Inflation occurs naturally with appropriated slow-roll values. The…

宇宙学与河外天体物理 · 物理学 2021-11-02 S. H. Pereira

We discuss the dynamics and phenomenology of an oscillating scalar field coupled to the Higgs boson that accounts for the dark matter in the Universe. The model assumes an underlying scale invariance such that the scalar field only acquires…

高能物理 - 唯象学 · 物理学 2018-05-25 Catarina Cosme , João G. Rosa , O. Bertolami
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