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Related papers: Entropy production by domain wall decay in the NMS…

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For several independent reasons, the idea that notorious sources of entropy could exist in the Universe has been recently revived. Taking advantage of a new framework accounting for non-equilibrium processes in cosmology, we explicitly…

General Relativity and Quantum Cosmology · Physics 2025-05-27 Jamy-Jayme Thézier , Aurélien Barrau , Killian Martineau

Entropy production is often interpreted as a proxy for microscopic disorder or environmental roughness in stochastic systems. We test this interpretation using controlled simulations of overdamped stochastic dynamics on curved surfaces in…

Statistical Mechanics · Physics 2026-02-23 Patrick Romanescu

If one simultaneously invokes the SUSY solution to the gauge hierarchy problem and the PQ solution to the strong CP problem, then one might expect mixed axion/neutralino dark matter (DM), i.e. two dark matter particles. In this case, dark…

High Energy Physics - Phenomenology · Physics 2013-06-18 Kyu Jung Bae , Howard Baer , Andre Lessa

Thermal inflation is an attractive solution to the cosmological moduli problem. However, domain walls may be formed after thermal inflation and some mechanisms are needed to eliminate the domain wall before it dominates the Universe. We…

High Energy Physics - Phenomenology · Physics 2011-08-31 Takeo Moroi , Kazunori Nakayama

We discuss effects of cosmological moduli fields on the cosmic microwave background (CMB). If a modulus field \phi once dominates the universe, the CMB we observe today is from the decay of \phi and its anisotropy is affected by the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Takeo Moroi , Tomo Takahashi

Grand unified theories can admit cosmic strings with fermion zero modes which result in the string carrying a current and the formation of stable remnants, vortons. We consider theories in which the zero modes do not survive a subsequent…

High Energy Physics - Phenomenology · Physics 2009-10-30 Anne-Christine Davis , Warren B. Perkins

The presence of domain walls separating regions of unbroken $SU(2)_L$ and $SU(2)_R$ is shown to provide necessary conditions for leptogenesis which converts later to the observed Baryon aymmetry. The strength of lepton number violation is…

High Energy Physics - Phenomenology · Physics 2008-11-26 U. A. Yajnik , J. Cline , M. Rabikumar

A recent paper investigated minimal R$\nu$MDM models with the type T1-iii and T3 one-loop topologies. However, the candidate most-minimal model does not possess an accidental symmetry - the scalar potential contains an explicit symmetry…

High Energy Physics - Phenomenology · Physics 2016-06-01 Amine Ahriche , Kristian L. McDonald , Salah Nasri , Ivica Picek

We consider the scenario in which the Peccei-Quinn symmetry breaking is followed by a period of inflation. A particularly interesting case is that the string-domain wall network produced by the symmetry breaking enters the horizon after the…

High Energy Physics - Phenomenology · Physics 2022-11-16 Keisuke Harigaya , Lian-Tao Wang

Production of gravitational vacuum defects and their contribution to the energy density of our Universe are discussed. These topological microstructures (defects) could be produced in the result of creation of the Universe from "nothing"…

General Relativity and Quantum Cosmology · Physics 2008-01-03 V. Burdyuzha , G. Vereshkov , J. Pacheco

We present a model of spontaneous (or dynamical) C and CP violation where it is possible to generate domains of matter and antimatter separated by cosmologically large distances. Such C(CP) violation existed only in the early universe and…

Cosmology and Nongalactic Astrophysics · Physics 2015-10-15 A. D. Dolgov , S. I. Godunov , A. S. Rudenko , I. I. Tkachev

The spontaneous breaking of B-L symmetry naturally accounts for the small observed neutrino masses via the seesaw mechanism. We have recently shown that the cosmological realization of B-L breaking in a supersymmetric theory can…

High Energy Physics - Phenomenology · Physics 2012-07-19 Wilfried Buchmüller , Valerie Domcke , Kai Schmitz

It is tempting to inflate along one of the many flat directions that arise in supersymmetric theories. The required flatness of the potential to obtain sufficient inflation and to not overproduce density fluctuations occurs naturally.…

High Energy Physics - Phenomenology · Physics 2009-10-28 Katherine Freese , Tony Gherghetta , Hideyuki Umeda

We investigate the time evolution of the temperature and entropy of gravitationally collapsing domain walls as seen by an asymptotic observer. In particular, we seek to understand how topology and the addition of a cosmological constant…

General Relativity and Quantum Cosmology · Physics 2015-05-28 Evan Halstead

A $Z_{2L}\times Z_{2R}$ generation symmetry in the neutrino sector predicts the atmospheric neutrino mixing to be maximal, and the MNS matrix element $U_{e3}$ to be zero, consistent with observations. Solar neutrino mixing may be maximal…

High Energy Physics - Phenomenology · Physics 2007-05-23 C. S. Lam

It is shown that the minimal left-right symmetric model admits cosmic string and domain wall solutions. The cosmic strings arise when the SU(2)_R is broken and can either be destabilized at the electroweak scale or remain stable through the…

High Energy Physics - Phenomenology · Physics 2014-11-17 U. A. Yajnik , Hatem Widyan , Shobhit Mahajan , Amitabha Mukherjee , Debajyoti Choudhari

We explore the stability of domain wall and bubble solutions in theories with compact extra dimensions. The energy density stored inside of the wall can destabilize the volume modulus of a compactification, leading to solutions containing…

High Energy Physics - Theory · Physics 2011-02-25 Anthony Aguirre , Matthew C Johnson , Magdalena Larfors

We present a comprehensive analysis of constraints on the sterile neutrino as a dark matter candidate. The minimal production scenario with a standard thermal history and negligible cosmological lepton number is in conflict with…

Astrophysics · Physics 2009-11-11 Kevork Abazajian , Savvas M. Koushiappas

We consider a cosmogony with a dark matter component consisting of a network of frustrated domain walls. Such a network provides a solid dark matter component with $p=-(2/3)\rho $ that remains unclustered on small scales and with…

Astrophysics · Physics 2007-05-23 Richard A. Battye , Martin Bucher , David Spergel

Non-invertible global symmetry often predicts degeneracy in axion potentials and carries important information about the global form of the gauge group. When these symmetries are spontaneously broken they can lead to the formation of stable…

High Energy Physics - Phenomenology · Physics 2023-09-12 Clay Cordova , Sungwoo Hong , Lian-Tao Wang