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In a superconductor electrons form pairs despite the Coulomb repulsion as a result of an effective attractive interaction mediated by, for example phonons. In the present paper DeGennes' description of the dynamically screened Coulomb…

超导电性 · 物理学 2025-03-13 Dirk van der Marel

A new concept of generation of the cosmological baryon excess along with the cold dark matter (CDM) in the Universe is proposed and corresponding scenarios are outlined. Possible realizations of the idea in the framework of supersymmetric…

高能物理 - 唯象学 · 物理学 2014-11-17 Vadim A. Kuzmin

Coulomb interaction of charges in a metamaterial may be expressed via its effective dielectric response function. Coulomb interaction appears considerably enhanced in artificially engineered epsilon near zero (ENZ) and hyperbolic…

光学 · 物理学 2018-12-07 Igor I. Smolyaninov , Vera N. Smolyaninova

We study a mechanism through which the cosmic dark matter density can be explained simultaneously with the observed baryon asymmetry of the Universe. At the core of our proposal lie the out-of-equilibrium scattering processes of bath…

高能物理 - 唯象学 · 物理学 2022-09-15 Andreas Goudelis , Dimitrios Karamitros , Pantelis Papachristou , Vassilis C. Spanos

The prevalence of matter over antimatter in the observable universe remains one of the most profound puzzles in modern physics, necessitating sources of charge-parity (CP) symmetry violation beyond those incorporated in the Standard Model.…

高能物理 - 实验 · 物理学 2026-04-20 Jianyu Zhang

Current dark matter detection strategies are based on the assumption that the dark matter is a gas of non-interacting particles with a reasonably large number density. This picture is dramatically altered if there are significant self…

高能物理 - 唯象学 · 物理学 2018-12-19 Dorota M Grabowska , Tom Melia , Surjeet Rajendran

The kinematics of the extra-planar neutral and ionised gas in disc galaxies shows a systematic decline of the rotational velocity with height from the plane (vertical gradient). This feature is not expected for a barotropic gas, whilst it…

星系天体物理 · 物理学 2015-05-14 F. Marinacci , F. Fraternali , L. Ciotti , C. Nipoti

The dynamical mass of clusters of galaxies, calculated in terms of modified Newtonian dynamics, is a factor of two or three times smaller than the Newtonian dynamical mass but remains significantly larger than the observed baryonic mass in…

天体物理学 · 物理学 2009-11-13 R. H. Sanders

We consider the problem of relaxation in a one-dimensional system of interacting electrons. In the limit of weak interactions, we calculate the decay rate of a single-electron excitation, accounting for the nonlinear dispersion. The leading…

强关联电子 · 物理学 2013-04-09 Zoran Ristivojevic , K. A. Matveev

The MSSM has flat directions in its scalar potential, along which it is natural for Bose condensates of squarks to form in the early Universe. A baryon asymmetry can be induced in these condensates via Affleck-Dine baryogenesis. The…

高能物理 - 唯象学 · 物理学 2007-05-23 John McDonald

Electroweak baryogenesis (EWBG) remains a theoretically attractive and experimentally testable scenario for explaining the cosmic baryon asymmetry. We review recent progress in computations of the baryon asymmetry within this framework and…

高能物理 - 唯象学 · 物理学 2015-06-05 David E. Morrissey , Michael J. Ramsey-Musolf

Dark photons, a generic class of light gauge bosons that interact with the Standard Model (SM) exclusively through kinetic mixing, arise naturally in many gauge extensions of the SM. Motivated by these theoretical considerations, we present…

高能物理 - 唯象学 · 物理学 2025-12-10 Xun-Jie Xu , Boting Zhou

We evaluate the ratio of baryon and electric-charge cumulants at second order from the recent experimental results at $\sqrt{s_{_{NN}}}=200$ GeV by the STAR Collaboration. The baryon number cumulant is reconstructed from the proton number…

高能物理 - 唯象学 · 物理学 2022-12-28 Masakiyo Kitazawa , ShinIchi Esumi , Toshihiro Nonaka

The observational relation between the density of baryon and dark matter in the Universe, $\Omega_{\rm DM}/\Omega_B\simeq 5$, is one of the most difficult problems to solve in modern cosmology. We discuss a scenario that explains this…

高能物理 - 唯象学 · 物理学 2013-05-30 Kohei Kamada , Masahide Yamaguchi

The evolution of nonlinear density fluctuations around the Jeans mass shortly after cosmological recombination is analyzed using a 3D hydrodynamics/dark--matter code. The Cosmic Background Radiation (CBR) exerts Compton friction on free…

天体物理学 · 物理学 2009-10-22 M. Umemura , A. Loeb , E. L. Turner

The recent observational evidence for the current cosmic acceleration have stimulated renewed interest in alternative cosmologies, such as scenarios with interaction in the dark sector (dark matter and dark energy). In general, such models…

宇宙学与河外天体物理 · 物理学 2009-10-22 R. S. Goncalves , J. S. Alcaniz , A. Dev , D. Jain

We explore a simple model which naturally explains the observed baryon asymmetry of the Universe. In this model the strong coupling is promoted to a dynamical quantity, which evolves through the vacuum expectation value of a singlet scalar…

高能物理 - 唯象学 · 物理学 2020-04-08 Djuna Croon , Jessica N. Howard , Seyda Ipek , Timothy M. P. Tait

The inclusion of an additional $U(1)$ gauge symmetry is a common feature in many extensions of the Standard Model, revealing the intricate connections between particle physics and cosmology. The $L_{\mu} - L_{\tau}$ model stands as a…

高能物理 - 唯象学 · 物理学 2024-02-26 Ashutosh Kumar Alok , Neetu Raj Singh Chundawat , Arindam Mandal

The usual condensed matter lattice theories do not include dynamical electromagnetic (EM) field and do not have higher symmetries naturally (unless we engineer fine-tuned toy models to realize higher symmetries). However, for gapped…

强关联电子 · 物理学 2019-05-29 Xiao-Gang Wen

Electric double layers (EDL) with counterions only, say electrons with the elementary charge $-e$, in thermal equilibrium at the inverse temperature $\beta$ are considered. In particular, we study the effect of the surface charge modulation…

统计力学 · 物理学 2022-07-26 Ladislav Šamaj