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We perform a semi-classical analysis of the Emergent Universe scenario for inflation. Fixing the background, and taking the inflaton to be homogenous, we cast the inflaton's evolution as a one-dimensional quantum mechanics problem. We find…

High Energy Physics - Theory · Physics 2013-11-20 Anthony Aguirre , John Kehayias

We revisit inflation in induced gravity. Our focus is on models where the low scale Planck mass is completely determined by the breaking of the scaling symmetry in the field theory sector. The Higgs-like field which breaks the symmetry with…

High Energy Physics - Phenomenology · Physics 2008-11-26 Nemanja Kaloper , Lorenzo Sorbo , Jun'ichi Yokoyama

We consider a variant of Hybrid Inflation, where inflation is driven by two interacting scalar fields, one of which has a `Mexican hat' potential and the other a quartic potential. Given the appropriate initial conditions one of the fields…

Astrophysics · Physics 2016-08-24 David Roberts , Andrew R Liddle , David H Lyth

In a recently proposed Higgs-Seesaw model the observed scale of dark energy results from a metastable false vacuum energy associated with mixing of the standard model Higgs particle and a scalar associated with new physics at the GUT or…

High Energy Physics - Phenomenology · Physics 2014-04-23 Lawrence M. Krauss , Andrew J. Long

The properties of the recently discovered Higgs boson together with the absence of new physics at collider experiments allows us to speculate about consistently extending the Standard Model of particle physics all the way up to the Planck…

High Energy Physics - Phenomenology · Physics 2019-03-14 Javier Rubio

Starting with a theory of the discrete space-time at the Planck scale, we developed a Gravi-Weak Unification (GWU) - a $Spin(4,4)$-invariant model unified gravity with weak $SU(2)$ gauge and Higgs fields in the visible and invisible sectors…

General Relativity and Quantum Cosmology · Physics 2015-04-27 L. V. Laperashvili , H. B. Nielsen , B. G. Sidharth

We propose a new class of inflationary solutions to the standard cosmological problems (horizon, flatness, monopole,...), based on a modification of old inflation. These models do not require a potential which satisfies the normal…

High Energy Physics - Theory · Physics 2007-05-23 Gia Dvali , Shamit Kachru

Many models of supersymmetry breaking, in the context of either supergravity or superstring theories, predict the presence of particles with Planck-suppressed couplings and masses around the weak scale. These particles are generically…

High Energy Physics - Phenomenology · Physics 2010-02-03 G. F. Giudice , A. Riotto , I. Tkachev

The Hubble constant during the last stages of inflation in a broad class of models based on the KKLT mechanism should be smaller than the gravitino mass, H <~ m_{3/2}. We point out that in the models with large volume of compactification…

High Energy Physics - Theory · Physics 2009-09-29 Joseph P. Conlon , Renata Kallosh , Andrei Linde , Fernando Quevedo

Recent LHC data provides precise values of coupling constants of the Higgs field, however, these measurements do not determine its coupling with gravity. We explore this freedom to see whether Higgs field non-minimally coupled to…

Cosmology and Nongalactic Astrophysics · Physics 2016-08-17 Jose Mathew , S. Shankaranarayanan

It is possible that the expansion of the universe began with an inflationary phase, in which the inflaton driving the process also was a Higgs field capable of stabilizing magnetic monopoles in a grand-unified gauge theory. If so, then the…

General Relativity and Quantum Cosmology · Physics 2007-05-23 Alfred Scharff Goldhaber

Moduli fields, which parameterize perturbative flat directions of the potential in supersymmetric theories, are natural candidates to act as inflatons. An inflationary potential on moduli space can result if the scale of dynamical SUSY…

High Energy Physics - Theory · Physics 2009-10-28 Scott Thomas

The effective potential for the Standard Model Higgs field allows two quasi-degenerate vacua; one is our vacuum at the electroweak scale, while the other is at a much higher scale. The latter minimum may be at a scale much smaller than the…

High Energy Physics - Phenomenology · Physics 2015-05-08 Naoya Kitajima , Fuminobu Takahashi

Higgs G-inflation is a Higgs inflation model with a generalized Galileon term added to the standard model Higgs field, which realizes inflation compatible with observations. Recently, it was claimed that the generalized Galileon term…

High Energy Physics - Phenomenology · Physics 2013-12-17 Kohei Kamada , Tsutomu Kobayashi , Taro Kunimitsu , Masahide Yamaguchi , Jun'ichi Yokoyama

In the conventional metric formulation of gravity, the Higgs Inflation model violates unitarity in the electroweak vacuum in Higgs scattering at the energy scale $\Lambda \sim M_{Pl}/\xi$, where $\xi \sim 10^4$ is the non-minimal coupling…

High Energy Physics - Phenomenology · Physics 2021-05-05 J. McDonald

The discovery of the Higgs boson by the LHC and the measurement of its mass at around 125 GeV, taken together with the absence of signals of physics beyond the standard model, make it possible that we might live in a metastable electroweak…

High Energy Physics - Phenomenology · Physics 2015-12-04 Jose R. Espinosa

Moduli potential loses its minima due to external energy sources of inflaton energy density or radiation produced at the end of inflation. But, the non-existence of minima does not necessarily mean destabilization of moduli. In fact, the…

High Energy Physics - Phenomenology · Physics 2022-08-05 Khursid Alam , Koushik Dutta

Possibly, the most general action in the background of isotropic and homogeneous space-time has been considered to study the quantum evolution of the early universe, apart from a cosmological constant. The hermiticity of the effective…

High Energy Physics - Theory · Physics 2020-10-30 Ranajit Mandal , Dalia Saha , Mohosin Alam , Abhik Kumar Sanyal

Effective 4-dimensional theories are investigated which were obtained under dimensional reduction of multidimensional cosmological models with a minimal coupled scalar field as matter source. Conditions for the internal space stabilization…

High Energy Physics - Phenomenology · Physics 2009-10-31 U. Guenther , A. Zhuk

In many inflationary models, a large amount of energy is transferred rapidly to the long-wavelength matter fields during a period of preheating after inflation. We study how this changes the dynamics of the electroweak phase transition if…

High Energy Physics - Phenomenology · Physics 2009-10-31 A. Rajantie , P. M. Saffin , E. J. Copeland