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The onset of inflation in hybrid models require fine tuning in the initial conditions. The inflaton field should have an initial value close to the Planck scale $M_{P}$, whereas the auxiliary "orthogonal" field must be close to zero with an…

高能物理 - 唯象学 · 物理学 2009-11-07 Zurab Berezhiani , Anupam Mazumdar , Abdel Pérez-Lorenzana

The scale at which supersymmetry is broken and the mechanism by which supersymmetry breaking is fed down to the observable sector has rich implications on the way Nature may have chosen to accomplish inflation. We discuss a simple model for…

高能物理 - 唯象学 · 物理学 2014-11-17 Antonio Riotto

A gauged U(1)_B-L symmetry predicts three right handed handed neutrinos and its spontaneous breaking automatically yields the seesaw mechanism. In a supersymmetric setting this breaking can be nicely linked with inflation to yield deltaT/ T…

高能物理 - 唯象学 · 物理学 2007-05-23 V. N. Senoguz , Q. Shafi

Supersymmetry breaking close to the scale of grand unification can explain cosmic inflation. As we demonstrate in this paper, this can be achieved in strongly coupled supersymmetric gauge theories, such that the energy scales of inflation…

高能物理 - 唯象学 · 物理学 2018-06-26 Valerie Domcke , Kai Schmitz

We propose a variant scenario of spontaneous baryogenesis from asymmetric inflaton based on current-current interactions between the inflaton and matter fields with a non-zero B-L charge. When the inflaton starts to oscillate around the…

高能物理 - 唯象学 · 物理学 2016-03-16 Fuminobu Takahashi , Masaki Yamada

We comprehensively investigate a chaotic inflation model proposed recently in the framework of supergravity. In this model, the form of K\"ahler potential is determined by a symmetry, that is, the Nambu-Goldstone-like shift symmetry, which…

高能物理 - 唯象学 · 物理学 2009-10-31 M. Kawasaki , Masahide Yamaguchi , T. Yanagida

We reconsider the possibility that inflation was driven by a sneutrino - the scalar supersymmetric partner of a heavy singlet neutrino - in the minimal seesaw model of neutrino masses. We show that this model is consistent with data on the…

高能物理 - 唯象学 · 物理学 2009-09-11 J. Ellis , M. Raidal , T. Yanagida

We investigate a novel scenario of cosmological inflation in a gauged $B-L$ extended minimal supersymmetric Standard Model with R-symmetry. We use a noncanonical K\"{a}hler potential and a superpotential, both preserving the R-symmetry to…

高能物理 - 唯象学 · 物理学 2014-05-22 Masato Arai , Shinsuke Kawai , Nobuchika Okada

Recently a new model of "Affleck-Dine inflation" was presented, that produces the baryon asymmetry from a complex inflaton carrying baryon number, while being consistent with constraints from the cosmic microwave background. We adapt this…

高能物理 - 唯象学 · 物理学 2020-06-24 James M. Cline , Matteo Puel , Takashi Toma

We consider a phenomenological extension of the minimal supersymmetric standard model which incorporates chaotic inflation and a radiatively generated intermediate mass scale. Initially a period of chaotic inflation is driven by a quartic…

高能物理 - 唯象学 · 物理学 2009-10-28 Tony Gherghetta , Gordon L. Kane

We discuss a five dimensional inflationary scenario based on a supersymmetric SO(10) model compactified on $S^1/(Z_2\times Z_2')$. Inflation is implemented through scalar potentials on four dimensional branes, and a brane-localized…

高能物理 - 唯象学 · 物理学 2007-05-23 Bumseok Kyae

Inflation, as currently understood, requires the presence of fields with very flat potentials. Supersymmetric models in which supersymmetry breaking is communicated by supergravity naturally yield such fields, but the scales are typically…

高能物理 - 唯象学 · 物理学 2009-10-30 Michael Dine , Antonio Riotto

The asymmetric dark matter scenario is known to give an interesting solution for the cosmic coincidence problem between baryon and dark matter densities. In the scenario, the dark matter asymmetry, which is translated to the dark matter…

高能物理 - 唯象学 · 物理学 2015-05-27 Naoyuki Haba , Shigeki Matsumoto , Ryosuke Sato

We studied the question of parity breaking in a supersymmetric left-right model, in which the left-right symmetry is broken with Higgs doublets (carrying $B-L=\pm 1$). Unlike the left-right symmetric models with triplet Higgs scalars…

高能物理 - 唯象学 · 物理学 2014-11-20 Sudhanwa Patra , Anjishnu Sarkar , Utpal Sarkar

We propose a simple framework to split neutrinos with a slight departure from tribimaximal mixing - where two of the neutrinos are Majorana type which provide thermal leptogenesis. The Dirac neutrino with a tiny Yukawa coupling explains…

高能物理 - 唯象学 · 物理学 2013-05-30 Anupam Mazumdar , Stefano Morisi

We present a dynamical cosmological solution that simultaneously accounts for the early inflationary stage of the Universe and solves the supersymmetric little hierarchy problem via the relaxion mechanism. First, we consider an inflationary…

高能物理 - 唯象学 · 物理学 2017-06-28 Jason L. Evans , Tony Gherghetta , Natsumi Nagata , Marco Peloso

A variation of Affleck-Dine mechanism was proposed to generate the observed baryon asymmetry in [1], in which the inflaton was assumed to be a complex scalar field with a weakly broken $U(1)$ symmetry, and the baryon asymmetry generation…

宇宙学与河外天体物理 · 物理学 2015-06-22 Nan Li , Ding-fang Zeng

We elaborate on a minimal inflation scenario based entirely on the general properties of supersymmetry breaking in supergravity models. We identify the inflaton as the scalar component of the Goldstino superfield. We write plausible…

高能物理 - 理论 · 物理学 2011-10-19 Luis Alvarez-Gaume , Cesar Gomez , Raul Jimenez

In this work, we present a unified theoretical framework that simultaneously addresses some of the most intriguing puzzles in particle physics and cosmology, namely the origins of neutrino mass, baryon asymmetry, and cosmic inflation. In…

高能物理 - 唯象学 · 物理学 2024-09-05 Ajay Kaladharan , Shaikh Saad

We consider a supersymmetric model of inflation in which the primordial density fluctuations are nearly scale invariant (the spectral index n is approximately 0.98) with amplitude proportional to (M/M_{Planck})^2, where M ~ 10^{16} GeV…

高能物理 - 唯象学 · 物理学 2008-11-26 G. Lazarides , R. K. Schaefer , Q. Shafi