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We investigate an influence of an external magnetic field on chiral symmetry breaking in a four-fermion interaction model at finite temperature and chemical potential. By using the Fock-Schwinger proper-time method, we calculate the…

高能物理 - 唯象学 · 物理学 2009-11-10 Tomohiro Inagaki , Daiji Kimura , Tsukasa Murata

Dark sector may exist and interact with Standard Model (SM) through the $U(1)$ kinetic mixing. Through this portal-type interaction, dark photon from dark sector couples to SM fermions, and may explain the discrepancy between experimental…

高能物理 - 唯象学 · 物理学 2026-02-04 Chuan-Ren Chen , Yuan-Feng Hsieh , Chrisna Setyo Nugroho

We have developed an exact, general method to compute Casimir interactions between a finite number of compact objects of arbitrary shape and separation. Here, we present details of the method for a scalar field to illustrate our approach in…

统计力学 · 物理学 2008-11-26 T. Emig , N. Graham , R. L. Jaffe , M. Kardar

In a previous work a model was proposed for the phase transitions of crystals with localized magnetic moments which at low temperature have a "conical" arrangement that at higher T transforms into a more symmetrical structure (depending on…

统计力学 · 物理学 2009-11-13 Vittorio Massidda

Four-fermion interaction models are often used as simplified models of interacting fermion fields with the chiral symmetry. The chiral symmetry is dynamically broken for a larger four-fermion coupling. It is expected that the broken…

高能物理 - 理论 · 物理学 2019-04-11 Tomohiro Inagaki , Yamato Matsuo , Hiromu Shimoji

Polarized $\Lambda_b \to \Lambda \gamma$ decays at the Z pole are shown to be well suited for probing a large variety of New Physics effects. A new observable is proposed, the angular asymmetry between the $\Lambda_b$ spin and photon…

高能物理 - 唯象学 · 物理学 2009-11-07 G. Hiller , A. Kagan

This paper treats nonrelativistic matter and a scalar field $\phi$ with a monotonically decreasing potential minimally coupled to gravity in flat Friedmann-Lema\^{i}tre-Robertson-Walker cosmology. The field equations are reformulated as a…

广义相对论与量子宇宙学 · 物理学 2015-11-11 Artur Alho , Claes Uggla

Using ideas underlying the flavour-blind "Nijmegen Unitarised Meson Model" we try to understand on the basis of a system of Schroedinger equations with one meson-meson and one (spinless) quark-antiquark channel coupled by a simple…

高能物理 - 唯象学 · 物理学 2009-11-10 F. Kleefeld

Nonmagnetic spheres confined in a ferrofluid layer (magnetic holes) present dipolar interactions when an external magnetic field is exerted. The interaction potential of a microsphere pair is derived analytically, with a precise care for…

软凝聚态物质 · 物理学 2009-11-10 Renaud Toussaint , Jørgen Akselvoll , Eirik G. Flekkøy , Geir Helgesen , Arne T. Skjeltorp

We study the relational cosmological dynamics emerging from interacting group field theory (GFT) models minimally coupled to a massless clock scalar field and a self-interacting scalar field. We focus on two broad classes of GFT…

广义相对论与量子宇宙学 · 物理学 2025-08-25 Tom R. Ladstätter , Luca Marchetti

We consider a renormalizable extension of the standard model whose fermionic dark matter (DM) candidate interacts with a real singlet pseudo-scalar via a pseudo-scalar Yukawa term while we assume that the full Lagrangian is CP-conserved in…

高能物理 - 唯象学 · 物理学 2015-01-12 Karim Ghorbani

The phenomenological features of the mixing in the neutral pseudoscalar mesons K0-K0bar can be illustrated in the classical framework of mechanics and by means of electromagnetic coupled circuits. The time-reversed not-invariant processes…

高能物理 - 唯象学 · 物理学 2015-06-25 D. Cocolicchio , L. Telesca

Fermion mixing is conveniently described using the effective Lagrangian formalism. We apply this approach to study top mixing in models with an infinite tower of Kaluza-Klein fermion excitations. In the Randall-Sundrum background with a…

高能物理 - 唯象学 · 物理学 2007-05-23 F. del Aguila , J. Santiago

The smallness of fermion masses and mixing angles has recently been been attributed to approximate global $U(1)$ symmetries, one for each fermion type. The parameters associated with these symmetry breakings are estimated here directly from…

高能物理 - 唯象学 · 物理学 2009-12-30 Lawrence Hall , Steven Weinberg

The most general Two Higgs Doublet Model potential without explicit CP violation depends on 10 real independent parameters . Excluding spontaneous CP violation results in two 7 parameter models. Although both models give rise to 5 scalar…

高能物理 - 唯象学 · 物理学 2017-08-23 Lars Brucher , Rui Santos

In this work, $\gamma^{(\ast)}\gamma^{(\ast)}$ interactions in electron-positron collisions are studied across both low- and high-energy regimes. The analysis includes contributions from the Vector Meson Dominance (VMD) model (via Reggeon…

高能物理 - 唯象学 · 物理学 2025-09-01 G. Zardo Becker

In this paper we give a variation of the gauge procedure which employs a scalar gauge field, $B (x)$, in addition to the usual vector gauge field, $A_\mu (x)$. We study this variant of the usual gauge procedure in the context of a complex…

高能物理 - 理论 · 物理学 2015-06-18 Eduardo I. Guendelman , Douglas Singleton

We consider a cosmological scenario endowed with an interaction between the universe's dark components $-$ dark matter and dark energy. Specifically, we assume the dark matter component to be a pressure-less fluid, while the dark energy…

广义相对论与量子宇宙学 · 物理学 2021-08-03 Andronikos Paliathanasis , Genly Leon , Wompherdeiki Khyllep , Jibitesh Dutta , Supriya Pan

A class of chiral gauge theories is studied with accidentally-stable pseudo Nambu-Goldstone bosons playing the role of dark matter (DM). The gauge group contains a vector-like dark color factor that confines at energies larger than the…

高能物理 - 唯象学 · 物理学 2021-02-24 Roberto Contino , Alessandro Podo , Filippo Revello

Fundamental constants such as masses and coupling constants of elementary particles can have small temporal and spatial variations in the scalar field dark matter model. These variations entail time oscillations of other constants, such as…

高能物理 - 唯象学 · 物理学 2024-11-18 V. V. Flambaum , A. J. Mansour , I. B. Samsonov , C. Weitenberg
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