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Related papers: Primordial Monopoles and Strings, Inflation, and G…

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We revisit the hybrid inflation model gauged by $U(1)_{B-L}$ extension of the Minimal Supersymmetric Standard Model (MSSM) in a no-scale background. Considering a single predictive framework, we study inflation, leptogenesis, gavitino…

High Energy Physics - Phenomenology · Physics 2022-10-27 Waqas Ahmed , M. Junaid , Salah Nasri , Umer Zubair

Supersymmetric grand unification based on $SO(10)$ is one of the most attractive paradigms in physics beyond the Standard Model. Inspired by the recent NANOGrav signal, we discuss the implications of detecting a stochastic gravitational…

High Energy Physics - Phenomenology · Physics 2021-09-01 So Chigusa , Yuichiro Nakai , Jiaming Zheng

We consider the formation of metastable cosmic strings in a left-right unified theory. The produced monopoles are diluted by a stage of F-term hybrid inflation (FHI) which is realized consistently with the SUSY breaking and a global $U(1)$…

High Energy Physics - Phenomenology · Physics 2026-03-20 C. Pallis

In the context of supersymmetric models, we analyze the production of topological defects at the end of inflation driven by a conjugate pair of inflaton fields which are non-singlets under the continuous symmetry group of the theory. We…

High Energy Physics - Phenomenology · Physics 2008-11-26 G. Lazarides , Q. Shafi

Future detection/non-detection of tensor modes from inflation in CMB observations presents a unique way to test certain features of string theory. Current limit on the ratio of tensor to scalar perturbations, r=T/S, is r < 0.3, future…

High Energy Physics - Theory · Physics 2009-11-13 Renata Kallosh , Andrei Linde

We discuss some testable predictions of a non-supersymmetric $SO(10)$ model supplemented by a Peccei-Quinn symmetry. We utilize a symmetry breaking pattern of $SO(10)$ that yields unification of the Standard Model gauge couplings, with the…

High Energy Physics - Phenomenology · Physics 2022-12-09 George Lazarides , Rinku Maji , Rishav Roshan , Qaisar Shafi

We demonstrate that string motivated inflation ending via tachyonic instability leaves a detectable imprint on the cosmic microwave background (CMB) radiation by virtue of the excitation of non-Gaussian gravitational fluctuations. The…

High Energy Physics - Theory · Physics 2007-05-23 Kari Enqvist , Asko Jokinen , Anupam Mazumdar , Tuomas Multamaki , Antti Vaihkonen

This is a short review of string cosmology. We wish to connect string-scale physics as closely as possible to observables accessible to current or near-future experiments. Our possible best hope to do so is a description of inflation in…

High Energy Physics - Theory · Physics 2015-12-07 Alexander Westphal

The combination of non-minimal couplings to gravity with the post-inflationary kinetic-dominated era typically appearing in quintessential inflation scenarios may lead to the spontaneous symmetry breaking of internal symmetries and its…

Cosmology and Nongalactic Astrophysics · Physics 2019-02-18 Dario Bettoni , Guillem Domènech , Javier Rubio

The spontaneous breaking of $SO(10)$ grand unified symmetry to $SU(3)_c \times SU(2)_L \times U(1)_Y \times U(1)_\chi$ yields the GUT monopole as well as a comparably heavy $U(1)_\chi$ monopole which also carries $U(1)_Y$ flux. A metastable…

High Energy Physics - Phenomenology · Physics 2025-06-26 Rinku Maji , Qaisar Shafi

The scale of small-field inflation cannot be constrained via primordial gravitational waves through measurement of tensor-to-scalar ratio $r$. In this study, I show that if cosmic strings are produced after symmetry breaking at the end of…

High Energy Physics - Phenomenology · Physics 2021-06-02 Chia-Min Lin

In this paper we consider an inflating universe with long straight cosmic string along z-axis. We show that the effect of cosmic string can be taken as a perturbation on the background of FRW metric. Then by doing cosmological perturbations…

General Relativity and Quantum Cosmology · Physics 2024-05-07 S. Azar Ag Galeh , A. M. Abbassi , M. H. Abbassi

Many symmetry breaking patterns in grand unified theories (GUTs) give rise to cosmic strings that eventually decay when pairs of GUT monopoles spontaneously nucleate along the string cores. These strings are known as metastable cosmic…

High Energy Physics - Phenomenology · Physics 2024-01-23 Wilfried Buchmuller , Valerie Domcke , Kai Schmitz

We point out that the inclusion of a string component contributing around 5% to the CMB power spectrum amplitude on large scales can increase the preferred value of the spectral index n_s of density fluctuations measured by CMB experiments.…

Astrophysics · Physics 2009-11-11 Richard A. Battye , Bjorn Garbrecht , Adam Moss

We discuss the gravitational waves (GW) in the context of vector inflation. We derive the action for tensor perturbations and find that tachyonic instabilities are present in most (but not all) of the inflationary models with large fields.…

Astrophysics · Physics 2009-03-20 Alexey Golovnev , Viatcheslav Mukhanov , Vitaly Vanchurin

Detecting the parity-odd, or B-mode, polarization pattern in the cosmic microwave background radiation due to primordial gravity waves is considered to be the final observational key to confirming the inflationary paradigm. The search for…

Astrophysics · Physics 2009-06-23 Levon Pogosian , Mark Wyman

We explore supersymmetric SO(10) models predicting observable proton decay and various topological defects which produce different shapes and strengths of gravitational wave backgrounds depending on the scales of intermediate symmetry…

High Energy Physics - Phenomenology · Physics 2022-08-31 Eung Jin Chun , Liliana Velasco-Sevilla

A metastable cosmic-string network is a generic consequence of many grand unified theories (GUTs) when combined with cosmic inflation. Metastable cosmic strings are not topologically stable, but decay on cosmic time scales due to pair…

High Energy Physics - Phenomenology · Physics 2021-12-15 Wilfried Buchmuller , Valerie Domcke , Kai Schmitz

When cosmic strings are formed during inflation, they regrow to reach a scaling regime, leaving distinct imprints on the stochastic gravitational wave background (SGWB). Such signatures, associated with specific primordial features, can be…

Cosmology and Nongalactic Astrophysics · Physics 2025-11-18 Mainak Baidya , Anish Ghoshal , David F. Mota

String theory avoids the ultraviolet infinities that arise in trying to quantize gravity. It is also more predictive than conventional quantum field theory, one aspect of this being the way that it contributed to the emergence of the…

High Energy Physics - Theory · Physics 2007-05-23 Edward Witten