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We propose a scenario for inflation based upon the braneworld picture, in which high-energy corrections to the Friedmann equation permit inflation to take place with potentials ordinarily too steep to sustain it. Inflation ends when the…

天体物理学 · 物理学 2009-10-31 Edmund J Copeland , Andrew R Liddle , James E Lidsey

We consider the potential problems due to the production of inflatinos and gravitinos after inflation. Inflationary models with a single scale set by the microwave background anisotropies have a low enough reheat temperature to avoid…

高能物理 - 唯象学 · 物理学 2009-09-15 Hans Peter Nilles , Keith A. Olive , Marco Peloso

The warm inflation paradigm considers the continuous production of radiation during inflation due to dissipative effects. In its strong dissipation limit, warm inflation gives way to a radiation dominated Universe. High scale inflation then…

高能物理 - 唯象学 · 物理学 2011-03-18 Juan C. Bueno Sanchez , Mar Bastero-Gil , Arjun Berera , Konstantinos Dimopoulos , Kazunori Kohri

In supersymmetric models of warm inflation, the large temperature of the radiation bath produced by the dissipative motion of the inflaton field may induce a significant thermal abundance of potentially dangerous gravitinos. While previous…

高能物理 - 唯象学 · 物理学 2013-01-16 Sam Bartrum , Arjun Berera , Joao G. Rosa

We investigate the thermal production of gravitinos in the context of the brane world cosmology. Since the expansion law is modified from the one in the standard cosmology, the Boltzmann equation for the gravitino production is altered. We…

高能物理 - 唯象学 · 物理学 2009-11-10 Nobuchika Okada , Osamu Seto

The low reheat temperature at the end of inflation from the gravitino bound constrains the creation of heavy Majorana neutrinos associated with models of leptogenesis. However, a detailed view of the reheating of the Universe at the end of…

高能物理 - 唯象学 · 物理学 2014-11-18 Raghavan Rangarajan , Narendra Sahu

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,…

高能物理 - 唯象学 · 物理学 2008-11-26 H. Nakajima , Y. Shinbara

Gravitino production and decay in the inflationary universe are reexanimed. Assuming that gravitino mainly decays into photon and photino, we have calculated the upperbound of the reheating temperature. Compared to previous works, we have…

天体物理学 · 物理学 2009-09-25 M. Kawasaki , T. Moroi

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…

高能物理 - 唯象学 · 物理学 2010-01-29 Kenji Takagi , Yuta Koshimizu , Toyokazu Fukuoka , Takao Sakai , Hikoya Kasari , Mitsuo J. Hayashi

In this paper, we explore the parameter space of hilltop supernatural inflation model and show the regime within which there is no gravitino problem even if we consider both thermal and nonthermal production mechanisms. We make plots for…

高能物理 - 唯象学 · 物理学 2011-03-14 Kazunori Kohri , Chia-Min Lin

In this talk, we studied the implication of the constraint on the reheating temperature coming from the gravitino problem on models of leptogenesis. We point out that in supersymmetric extensions of the standard model, all existing models…

高能物理 - 唯象学 · 物理学 2007-05-23 D. Delepine

Gravitino production and decay in the inflationary universe are reexamined. Assuming that the gravitino mainly decays into a photon and a photino, we calculate the upperbound on the reheating temperature. Compared to previous works, we have…

高能物理 - 唯象学 · 物理学 2017-02-01 M. Kawasaki , T. Moroi

Gravitino problem is discussed in detail. We derive an upperbound on the reheating temperature from the constraints of the big-bang nucleosynthesis and the present mass density of the universe. Compared to previous works, we have improve…

高能物理 - 唯象学 · 物理学 2016-09-01 Takeo Moroi

We consider the abundance of gravitinos created from the vacuum fluctuation, in a class of `new' inflation models for which global supersymmetry is a good approximation. Immediately after inflation, gravitinos are produced, with number…

高能物理 - 唯象学 · 物理学 2009-10-31 David H Lyth

We study a N=1 Supergravity chaotic inflationary model, in the context of the braneworld scenario. It is shown that successful inflation and reheating consistent with phenomenological constraints can be achieved via the new terms in the…

天体物理学 · 物理学 2009-11-07 M. C. Bento , O. Bertolami

In supersymmetric theories, the gravitino is abundantly produced in the early Universe from thermal scattering, resulting in a strong upper bound on the reheat temperature after inflation. We point out that the gravitino problem may be…

高能物理 - 唯象学 · 物理学 2017-11-22 Raymond T. Co , Keisuke Harigaya

We revisit the F-term hybrid inflation model in supergravity. In particular, we point out that a constant term in the superpotential has significant effects on the inflaton dynamics. It is shown that the hybrid inflation model suffers from…

高能物理 - 唯象学 · 物理学 2011-04-15 Kazunori Nakayama , Fuminobu Takahashi , Tsutomu T. Yanagida

Supergravity embedding of the Standard Model of particle physics provides phenomenologically well-motivated and observationally viable inflationary scenarios. We investigate a class of inflationary models based on the superconformal…

高能物理 - 唯象学 · 物理学 2023-03-02 Shinsuke Kawai , Nobuchika Okada

We show that the gravitino-overproduction problem is prevalent among inflation models in supergravity. An inflaton field \phi generically acquires (effective) non-vanishing auxiliary field G_\phi, if the K\"ahler potential is non-minimal.…

高能物理 - 唯象学 · 物理学 2009-11-11 Masahiro Kawasaki , Fuminobu Takahashi , T. T. Yanagida

Models of leptogenesis are constrained by the low reheat temperature at the end of reheating associated with the gravitino bound. However a detailed view of reheating, in which the maximum temperature during reheating, $\Tmax$, can be…

高能物理 - 唯象学 · 物理学 2008-11-26 Raghavan Rangarajan , Narendra Sahu
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