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Related papers: SO(10) Cosmic Strings and Baryon Number Violation

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An implicit, fully characteristic, numerical scheme for solving the field equations of a cosmic string coupled to gravity is described. The inclusion of null infinity as part of the numerical grid allows us to apply suitable boundary…

General Relativity and Quantum Cosmology · Physics 2009-10-31 U. Sperhake , K. R. P. Sjodin , J. A. Vickers

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

We present results of new field-theoretic simulation of cosmological axion strings, which are eight times longer than previous ones. We have upgraded our simulation of physical strings in Hiramatsu et al. (2011) in terms of the number of…

High Energy Physics - Phenomenology · Physics 2019-12-06 Masahiro Kawasaki , Toyokazu Sekiguchi , Masahide Yamaguchi , Jun'ichi Yokoyama

Within a class of superstring vacua which have an additional non-anomalous $U(1)'$ gauge factor, we address the scale of the $U(1)'$ symmetry breaking and constraints on the exotic particle content and their masses. We also show that an…

High Energy Physics - Phenomenology · Physics 2009-09-17 Mirjam Cvetic , Paul Langacker

A fermion-boson-type composite model for quarks and leptons is proposed. Elementary fields are only one kind of spin-1/2 and spin-0 preon. Both are in the global supersymmetric pair with the common electric charge of e/6 and belong to the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Takeo Matsushima

We consider the cosmological consequences of a network of superconducting cosmic strings. For strong enough current the period of friction domination never ends. Instead a plasma scaling solution is reached. We demonstrate that this gives…

High Energy Physics - Phenomenology · Physics 2009-10-31 K. Dimopoulos , A. C. Davis

Using recent simulation results, we provide the mass and speed spectrum of cosmic string loops. This is the quantity of primary interest for many phenomenological signatures of cosmic strings, and it can be accurately predicted using…

Cosmology and Nongalactic Astrophysics · Physics 2014-01-22 Jose J. Blanco-Pillado , Ken D. Olum , Benjamin Shlaer

Flat directions are a generic feature of the scalar potential in supersymmetric gauge field theories. They can arise, for example, from D-terms associated with an extra abelian gauge symmetry. Even when supersymmetry is broken softly, there…

High Energy Physics - Phenomenology · Physics 2008-11-26 Yanou Cui , Stephen P. Martin , David E. Morrissey , James D. Wells

Cosmic strings, a hot subject in the 1980's and early 1990's, lost its appeal when it was found that it leads to inconsistencies in the power spectrum of the measured cosmic microwave background temperature anisotropies. However,…

High Energy Physics - Theory · Physics 2008-11-26 Mairi Sakellariadou

We investigate the string solutions and cosmological implications of the gauge ${\rm U(1)_Z}\,\times$ global ${\rm U(1)_{PQ}}$ model. With two hierarchical symmetry-breaking scales, the model exhibits three distinct string solutions: a…

High Energy Physics - Phenomenology · Physics 2023-11-15 Xuce Niu , Wei Xue , Fengwei Yang

Baryogenesis scenarios at the string scale are considered. The observed baryon to entropy ratio, $n_B /s \sim 10^{-10}$, can be explained in these scenarios.

High Energy Physics - Phenomenology · Physics 2009-10-30 H. Aoki , H. Kawai

In this paper we investigate the non-Abelian cosmic string in de Sitter and anti-de Sitter spacetimes. In order to do that we construct the complete set of equations of motion considering the presence of a cosmological constant. By using…

General Relativity and Quantum Cosmology · Physics 2017-03-22 Antônio de Pádua Santos , Eugênio R. Bezerra de Mello

In this paper, we analyze numerically the behaviour of the solutions corresponding to a non-Abelian cosmic string in the framework of the Starobinsky model, i.e. where $f(R)=R + \zeta R^2$. We perform the calculations for both an…

General Relativity and Quantum Cosmology · Physics 2018-02-14 J. P. Morais Graça , A. de Pádua Santos , Eugênio R. Bezerra de Mello , V. B. Bezerra

If cosmic strings are present at the electroweak phase transition, they can act as seeds on which bubbles of true vacuum nucleate. We explore the nature of such a phase transition, in particular the wall velocity and thickness of the…

High Energy Physics - Phenomenology · Physics 2015-06-25 Susmita Bhowmik Duari , U. A. Yajnik

In the context of electroweak strings, the baryon number anomaly equation may be reinterpreted as a conservation law for baryon number minus helicity. Since the helicity is a sum of the link and twist numbers, linked or twisted loops of…

High Energy Physics - Phenomenology · Physics 2009-09-25 Tanmay Vachaspati , George B. Field

We show how two simple modifications to the standard cosmic string scenario for structure formation compare to the recently released Boomerang data set. Namely we consider pure string closed models and mixed models where both inflation and…

Astrophysics · Physics 2007-05-23 C. R. Contaldi

We fully investigate the symmetry breaking patterns occurring upon creation of composite non-Abelian strings: vortex strings in non-Abelian theories where different sets of colours have different amounts of flux. After spontaneous symmetry…

High Energy Physics - Theory · Physics 2020-01-14 Edwin Ireson

Operator nucleon vertices are constructed in composite superconformal string model. Splitting of baryon Regge trajectories with the same quantum numbers but with opposite parity is provided by inclusion of simple additional components to…

High Energy Physics - Theory · Physics 2014-03-04 V. A. Kudryavtsev

A scenario is suggested for spontaneous CP violation in non-SUSY and SUSY SU(10). The idea is to have a scalar potential which generates spontaneously a phase, at the high scale, in the VEV that gives a mass to the RH neutrinos. The case of…

High Energy Physics - Phenomenology · Physics 2007-05-23 Yoav Achiman

The extended electroweak $\mathrm{SU(3)_c \otimes SU(3)_L \otimes U(1)_X}$ symmetry framework "explaining" the number of fermion families is revisited. While $331$-based schemes can not easily be unified within the conventional field theory…

High Energy Physics - Phenomenology · Physics 2016-09-07 Andrea Addazi , J. W. F. Valle , C. A. Vaquera-Araujo
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