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相关论文: Conformally coupled dark matter

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The observed accelerating universe indicates the presence of Dark Energy which is probably interpreted in terms of an extremely light gravitational scalar field. We suggest a way to probe this scalar field which contributes to optical…

广义相对论与量子宇宙学 · 物理学 2011-11-03 Yasunori Fujii , Kensuke Homma

Recent astronomical observations of systems of dark matter, which have been cited as providing possible support for self-interacting cold dark matter, may provide evidence for the extra dimensions predicted by superstring scenarios. We find…

天体物理学 · 物理学 2007-05-23 Bo Qin , Ue-Li Pen , Joseph Silk

The nature of the dark matter that binds galaxies remains an open question. The favored candidate has been so far the neutralino. This massive species with evanescent interactions is now in difficulty. It would actually collapse in dense…

天体物理学 · 物理学 2009-11-06 Alexandre Arbey , Julien Lesgourgues , Pierre Salati

In view of ongoing measurements of the Higgs-like boson at the LHC and direct searches for dark matter, we explore the possibility of accommodating the potential results in a simple new-physics model with discrete gauge symmetry as well as…

高能物理 - 唯象学 · 物理学 2015-03-20 Cheng-Wei Chiang , Takaaki Nomura , Jusak Tandean

Dark matter consisting of a Bose--Einstein condensate (BEC) of ultra-light particles is predicted to have a soliton shape that shifts with the dark matter mass fraction in galaxies containing a centrally localized point mass (or black…

星系天体物理 · 物理学 2026-01-21 Dor Ben-Amotz

We present a mechanism for generating ultralight dark photon dark matter in the early Universe via a dilatonlike scalar field coupled to the dark photon's kinetic term. Energy is initially stored in the condensate of the dilaton, which…

高能物理 - 唯象学 · 物理学 2025-08-20 Peter Adshead , Kaloian D. Lozanov , Zachary J. Weiner

We consider a simple model of a dark sector with a chiral $U(1)$ gauge symmetry. The anomaly-free condition requires at least five chiral fermions. Some of the fermions acquire masses through a vacuum expectation value of a Higgs field, and…

高能物理 - 唯象学 · 物理学 2026-03-03 Xiao He , Takaaki Nomura , Norimi Yokozaki

Recent experimental results in direct dark matter detection may be interpreted in terms of a dark matter particle of mass around 10 GeV/c^2. We show that the required scenario can be realized with a new dark matter particle charged under an…

高能物理 - 唯象学 · 物理学 2015-05-28 Paolo Gondolo , Pyungwon Ko , Yuji Omura

We consider cosmological aspects of the Dark Dimension (a mesoscopic dimension of micron scale), which has recently been proposed as the unique corner of the quantum gravity landscape consistent with both the Swampland criteria and…

高能物理 - 唯象学 · 物理学 2022-09-27 Eduardo Gonzalo , Miguel Montero , Georges Obied , Cumrun Vafa

In the general frameworks of an earlier introduced quartet-metric/multi-component gravity, a theory of a massive scalar graviton supplementing the massless tensor one is consistently deduced. The peculiarities of the scalar-graviton field…

广义相对论与量子宇宙学 · 物理学 2019-02-13 Yury F. Pirogov

We study the possibility that dark matter is a baryon of a new strongly interacting gauge theory, which was introduced in the low energy theory of Cosmological SUSY Breaking (CSB). This particle can fit the observed dark matter density if…

高能物理 - 唯象学 · 物理学 2009-11-11 T. Banks , J. D. Mason , D. O'Neil

Assuming that cosmological dark matter consists of weakly interacting massive particles, we use the recent precise measurement of cosmological parameters to predict the guaranteed rates of production of such particles in association with…

高能物理 - 唯象学 · 物理学 2009-10-09 Andreas Birkedal , Konstantin Matchev , Maxim Perelstein

A dark matter model based on QCD-like $SU(N_c)$ gauge theory with electroweakly interacting dark quarks is discussed. Assuming the dark quark mass $m$ is smaller than the dynamical scale $\Lambda_d \sim 4\pi f_d$, the main component of the…

高能物理 - 唯象学 · 物理学 2024-09-19 Tomohiro Abe , Ryosuke Sato , Takumu Yamanaka

We generalize dark matter production to a two-metric framework whereby the physical metric, which couples to the Standard Model (SM), is conformally and/or disformally related to the metric governing the gravitational dynamics. We show that…

高能物理 - 唯象学 · 物理学 2021-02-03 Philippe Brax , Kunio Kaneta , Yann Mambrini , Mathias Pierre

Many theories of dark energy and modified gravity give rise to scalar fields that couple derivatively to the energy momentum tensor of matter. This is known as disformal coupling. I will show that laboratory searches for axions are ideally…

高能物理 - 唯象学 · 物理学 2013-01-09 Clare Burrage

It is shown that cosmological equations for homogeneous isotropic models deduced in the framework of the Poincar\'e gauge theory of gravity by certain restrictions on indefinite parameters of gravitational Lagrangian take at asymptotics the…

广义相对论与量子宇宙学 · 物理学 2009-09-29 A. V. Minkevich

The symmetron scalar field is a matter-coupled dark energy candidate which effectively decouples from matter in high-density regions through a symmetry restoration. We consider a previously unexplored regime, in which the vacuum mass $\mu…

高能物理 - 唯象学 · 物理学 2013-05-30 Amol Upadhye

The logarithmic $R^2$-corrected $F(R)$ gravity is investigated as a prototype model of modified gravity theories with quantum corrections. By using the auxiliary field method, the model is described by the general relativity with a scalaron…

广义相对论与量子宇宙学 · 物理学 2019-10-23 T. Inagaki , Y. Matsuo , H. Sakamoto

Conventional scenarios of purely gravitationally produced dark matter with masses below the Hubble parameter at the end of inflation are in tension with Cosmic Microwave Background (CMB) constraints on the isocurvature power spectrum. We…

高能物理 - 唯象学 · 物理学 2024-02-15 Marcos A. G. Garcia , Mathias Pierre , Sarunas Verner

We consider a dark electroweak phase transition, during which a baryon asymmetry in the dark neutrons and an equal lepton asymmetry in the dark Dirac neutrinos can be simultaneously induced by the CP-violating reflection of the dark…

高能物理 - 唯象学 · 物理学 2017-10-04 Pei-Hong Gu