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The discovery of an axion-like particle above the QCD line would rule out Grand Unified Theories, including the perturbative heterotic string with the Standard Model embedded in a single $E_8$ factor or $SO(32)$. In this work we study a…

High Energy Physics - Theory · Physics 2025-11-19 Mario Reig , Timo Weigand

Cosmic strings are generic cosmological predictions of many extensions of the Standard Model of particle physics, such as a $U(1)^\prime$ symmetry breaking phase transition in the early universe or remnants of superstring theory. Unlike…

High Energy Physics - Phenomenology · Physics 2018-06-13 Yanou Cui , Marek Lewicki , David E. Morrissey , James D. Wells

It is commonly assumed that the energy density of the Universe was dominated by radiation between reheating after inflation and the onset of matter domination 54,000 years later. While the abundance of light elements indicates that the…

We construct new superstring actions which are distinguished from standard superstrings by being space-time scale invariant. Like standard superstrings, they are also reparametrization invariant, space-time supersymmetric, and invariant…

High Energy Physics - Theory · Physics 2009-10-30 M. Awada , F. Mansouri

The importance of the mass spectroscopy of the superparticles is emphasized. It will be shown that the gauge coupling constants give us information on the GUT-scale mass spectrum once the superparticle masses are known. The gaugino masses…

High Energy Physics - Phenomenology · Physics 2009-09-25 Hitoshi Murayama

We construct a new cosmological model considering the superstring-inspired E_6 unification in the 4-dimensional space at the early stage of the Universe. We develop a concept of parallel existence in Nature of the ordinary and shadow worlds…

High Energy Physics - Phenomenology · Physics 2011-09-21 C. R. Das , L. V. Laperashvili , A. Tureanu

We derive a constraint on the cosmic density of string moduli fields in gauge-mediated supersymmetry-breaking theories by requiring that photons emitted from the unstable moduli fields should not exceed the observed X-ray backgrounds. Since…

High Energy Physics - Phenomenology · Physics 2015-06-25 M. Kawasaki , T. Yanagida

Starting from an initial classical four dimensional flat background of the heterotic or type II superstrings, we are able to determine at the string one-loop level the quantum corrections to the effective potential due to the spontaneous…

High Energy Physics - Theory · Physics 2010-05-12 Francois Bourliot , Costas Kounnas , Herve Partouche

Since it has been pointed out that physics beyond the Standard Model may be constrained by gravitational waves from cosmic strings, it has been more important to clarify in what cases cosmic strings are formed. We study the stability of the…

High Energy Physics - Phenomenology · Physics 2023-05-24 Yukihiro Kanda , Nobuhiro Maekawa

We describe the detailed study and results of high-resolution numerical simulations of string-induced structure formation in open universes and those with a non-zero cosmological constant. The effect from small loops generated from the…

Astrophysics · Physics 2009-09-25 J. H. P. Wu , P. P. Avelino , E. P. S. Shellard , B. Allen

In this paper, the knotlike cosmic strings in the Riemann-Cartan space-time of the early universe are discussed. It has been revealed that the cosmic strings can just originate from the zero points of the complex scalar quintessence field.…

High Energy Physics - Theory · Physics 2014-11-18 Yi-shi Duan , Xin Liu

A string cosmology scenario ("pre-big-bang") postulates that the evolution of the Universe starts from a state of very small curvature and coupling, undergoes a long phase of dilaton-driven kinetic inflation and at some later time joins…

High Energy Physics - Theory · Physics 2016-10-26 Ram Brustein

The acceleration of the cosmic expansion revealed by supernova observations indicates that the present universe is dominated by repulsive dark energy. It is natural that the coupling between the dark energy and the attractive gravity has to…

Cosmology and Nongalactic Astrophysics · Physics 2014-10-07 Ti-Pei Li , Mei Wu

Cosmic strings are a type of cosmic defect formed by a symmetry-breaking phase transition in the early universe. Individual strings would have gathered to build a network, and their dynamical motion would induce scalar--, vector-- and…

Cosmology and Nongalactic Astrophysics · Physics 2016-01-07 Kouichirou Horiguchi , Kiyotomo Ichiki , Naoshi Sugiyama

We study the network of Type-I cosmic strings using the field-theoretic numerical simulations in the Abelian-Higgs model. For Type-I strings, the gauge field plays an important role, and thus we find that the correlation length of the…

Cosmology and Nongalactic Astrophysics · Physics 2013-10-30 Takashi Hiramatsu , Yuuiti Sendouda , Keitaro Takahashi , Daisuke Yamauchi , Chul-Moon Yoo

In string theory the coupling parameters are functions of moduli fields. The actual values of the coupling constants are then dynamically determined through the vacuum expextation values of these fields. We review the attempts to connect…

High Energy Physics - Phenomenology · Physics 2007-05-23 Hans Peter Nilles

It is shown that the heterotic string emerges as a soliton in the type I superstring theory in ten dimensions. The collective coordinates of the soliton are described by a smooth, chiral worldsheet theory. There are eight bosonic and eight…

High Energy Physics - Theory · Physics 2009-10-28 Atish Dabholkar

Our answer is the latter. Space-time singularities, including the initial one, are described by world-sheet topological Abelian gauge theories with a Chern-Simons term. Their effective $N=2$ supersymmetry provides an initial fixed point…

High Energy Physics - Theory · Physics 2016-09-06 John Ellis , N. E. Mavromatos , D. V. Nanopoulos

We analyze the early stage of evolution of a universe with two scale factors proposed in [1] when matter is present. The scale factors describe two causally disconnected patches of the universe interacting trough a non-trivial Poisson…

General Relativity and Quantum Cosmology · Physics 2021-06-09 Carlos Maldonado , Fernando Mendez

We investigate gravitational-wave backgrounds (GWBs) of primordial origin that would manifest only at ultra-high frequencies, from kilohertz to 100 gigahertz, and leave no signal at either LIGO, Einstein Telescope, Cosmic Explorer, LISA, or…

High Energy Physics - Phenomenology · Physics 2024-05-27 Géraldine Servant , Peera Simakachorn
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