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We analyse the shifted hybrid inflation in a no-scale SU(5) model with supersymmetry, which naturally circumvents the monopole problem. The no-scale framework is derivable as the effective field theory of the supersymmetric (SUSY)…

High Energy Physics - Phenomenology · Physics 2023-05-12 Waqas Ahmed , Muhammad Moosa , Shoaib Munir , Umer Zubair

Recent anomalies in cosmic rays could be due to dark matter annihilation in our galaxy. In order to get the required large cross-section to explain the data while still obtaining the right relic density, we rely on a non standard thermal…

High Energy Physics - Phenomenology · Physics 2009-09-02 Bhaskar Dutta , Louis Leblond , Kuver Sinha

By using a No-Scale Supergravity model, which was proved to explain WMAP observations appropriately, a mechanism of supersymmetry breaking and a preheating just after the end of inflation are investigated. Non-thermal production rate of…

High Energy Physics - Phenomenology · Physics 2010-01-29 Kenji Takagi , Yuta Koshimizu , Toyokazu Fukuoka , Takao Sakai , Hikoya Kasari , Mitsuo J. Hayashi

We study the effects of a non thermal neutralino production, due to the late decay in the early universe of a single modulus field, in the context of the deflected anomaly mediated scenario. In the regime in which the average number of…

High Energy Physics - Phenomenology · Physics 2007-06-01 A. M. Lionetto

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 derive the explicit form, and discuss some properties of the moduli dependent effective potential arising from M-theory compactified on $M_4 \times X\times S^1 / Z_2 $, when one of the boundaries supports a strongly interacting gauge…

High Energy Physics - Theory · Physics 2009-10-30 Zygmunt Lalak , Steven Thomas

The viability of a possible cosmological scenario is investigated. The theoretical framework is the constrained next-to-minimal supersymmetric standard model (cNMSSM), with a gravitino playing the role of the lightest supersymmetric…

High Energy Physics - Phenomenology · Physics 2014-11-20 Gabriela Barenboim , Grigoris Panotopoulos

In the supersymmetric extensions of the standard model, neutrino masses and leptogenesis requires existence of new particles. We point out that if these particles with lepton number violating interactions have standard model gauge…

High Energy Physics - Phenomenology · Physics 2009-10-31 David Delepine , Utpal Sarkar

The quasi-static solutions of the matter density perturbation in various dark energy models and modified gravity models have been investigated in numerous papers. However, the oscillating solutions in those models have not been investigated…

Cosmology and Nongalactic Astrophysics · Physics 2017-09-18 Jiro Matsumoto

Explicit string models which can realize inflation and low-energy supersymmetry are notoriously difficult to achieve. Given that sequestering requires very specific configurations, supersymmetric particles are in general expected to be very…

High Energy Physics - Phenomenology · Physics 2021-02-24 Rouzbeh Allahverdi , Igor Broeckel , Michele Cicoli , Jacek K. Osiński

It was recently found that the decay of inflaton and the SUSY breaking field produces many gravitinos in the gravity mediation scenario. These discoveries led to an exclusion of many inflation models such as chaotic, (smooth) hybrid,…

High Energy Physics - Phenomenology · Physics 2008-11-26 H. Nakajima , Y. Shinbara

Considering gravitino dark matter scenarios, we study constraints on the reheating temperature of inflation. We present the gauge-invariant result for the thermally produced gravitino yield to leading order in the Standard Model gauge…

High Energy Physics - Phenomenology · Physics 2008-11-26 Josef Pradler , Frank Daniel Steffen

We construct inflationary models in the context of supergravity with orthogonal nilpotent superfields [1]. When local supersymmetry is gauge-fixed in the unitary gauge, these models describe theories with only a single real scalar (the…

High Energy Physics - Theory · Physics 2016-03-23 John Joseph M. Carrasco , Renata Kallosh , Andrei Linde

We study moduli stabilization in combination with inflation in heterotic orbifold compactifications in the light of a large Hubble scale and the favored tensor-to-scalar ratio $r \approx 0.05$. To account for a trans-Planckian field range…

High Energy Physics - Theory · Physics 2015-05-25 Fabian Ruehle , Clemens Wieck

We consider different cosmological aspects of Heterotic M-theory. In particular we look at the dynamical behaviour of the two relevant moduli in the theory, namely the length of the eleventh segment (pi rho) and the volume of the internal…

High Energy Physics - Phenomenology · Physics 2009-10-31 T. Barreiro , B. de Carlos

The generic expectation in string/supergravity models is that there are multiple moduli fields with masses of the order of the supersymmetry breaking scale. We study the cosmology that arises as a result of vacuum misalignment of these…

High Energy Physics - Theory · Physics 2020-01-23 Bobby S. Acharya , Mansi Dhuria , Diptimoy Ghosh , Anshuman Maharana , Francesco Muia

Modular cosmology is plagued by overproduction of unwanted relics, gravitinos and especially moduli, at relatively low energy scales. Thermal inflation provides a compelling solution to this moduli problem, but invalidates most baryogenesis…

High Energy Physics - Phenomenology · Physics 2008-11-26 Donghui Jeong , Kenji Kadota , Wan-Il Park , Ewan D. Stewart

We investigate effects of the radiation and the moduli oscillation around the stabilized values on the evolution of a 6-dimensional spacetime compactified on $S^2$. In order to see the transition from the 5-dimensional space to the…

High Energy Physics - Theory · Physics 2023-06-14 Hajime Otsuka , Yutaka Sakamura

It has been recently shown that it is possible to excite gravitinos in an expanding background due to a time varying scalar field oscillating at the bottom of the inflationary potential. The two components of the gravitino, namely helicity…

High Energy Physics - Phenomenology · Physics 2009-10-31 Mar Bastero-Gil , Anupam Mazumdar

We discuss the moduli stabilization arising in the presence of gauge fluxes, R-symmetry twists and non-perturbative effects in the context of 6-dimensional supergravity models. We show how the presence of D-terms, due to the gauge fluxes,…

High Energy Physics - Theory · Physics 2007-10-26 A. P. Braun , A. Hebecker , M. Trapletti