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相关论文: Classically Scale Invariant Inflation, Supermassiv…

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We propose a cosmological framework in which neutrino masses evolve dynamically through coupling with a scalar field that simultaneously drives inflation. The neutrino mass is modeled as a power-law, exponential, or hybrid function of the…

宇宙学与河外天体物理 · 物理学 2025-12-01 Hemanshi Bundeliya , Gaurav Bhandari , S. D. Pathak , V. K. Sharma

A scheme of simplified smooth hybrid inflation is realized in the framework of supersymmetric $SU(5)$. The smooth model of hybrid inflation provides a natural solution to the monopole problem that appears in the breaking of $SU(5)$ gauge…

高能物理 - 唯象学 · 物理学 2017-10-06 Mansoor Ur Rehman , Umer Zubair

We investigate models in which the inflaton emerges as a composite field of a four dimensional, strongly interacting and nonsupersymmetric gauge theory featuring purely fermionic matter. We show that it is possible to obtain successful…

高能物理 - 唯象学 · 物理学 2011-05-12 Phongpichit Channuie , Jakob Jark Joergensen , Francesco Sannino

We assign the chiral fermion fields of the Standard model to triplets of flavor (family, generation, horizontal) $SU(3)_f$ symmetry, for anomaly freedom add one triplet of sterile right-handed neutrino fields, and gauge that symmetry. First…

高能物理 - 唯象学 · 物理学 2016-12-01 Jiri Hosek

We show how to enlarge the $\nu$MSM (the minimal extension of the standard model by three right-handed neutrinos) to incorporate inflation and provide a common source for electroweak symmetry breaking and for right-handed neutrino masses.…

高能物理 - 唯象学 · 物理学 2011-05-05 Mikhail Shaposhnikov , Igor Tkachev

Scalar singlet dark matter is one of the simplest and most predictive realisations of the WIMP (weakly-interacting massive particle) idea. Although the model is constrained from all directions by the latest experimental data, it still has…

高能物理 - 唯象学 · 物理学 2020-08-06 Peter Athron , Jonathan M. Cornell , Felix Kahlhoefer , James McKay , Pat Scott , Sebastian Wild

We show that embedding Natural Inflation in a more general scalar-tensor theory, with non-minimal couplings to the Ricci scalar and the kinetic term, alleviates the current tension of Natural Inflation with observational data. The coupling…

宇宙学与河外天体物理 · 物理学 2020-07-15 Guillem Simeon

This thesis presents a possible inflation scenario as a consequence of non-minimal gravitational couplings in the Conformal Standard Model. That model consists, in comparison to the SM, of additional right-chiral neutrinos and a complex…

广义相对论与量子宇宙学 · 物理学 2019-11-13 Jan Henryk Kwapisz

The Two-Higgs-Doublet-Standard Model-Axion-Seesaw-Higgs-Portal inflation (2hdSMASH) model consisting of two Higgs doublets, a Standard Model (SM) singlet complex scalar and three SM singlet right-handed neutrinos can embed axion dark…

高能物理 - 唯象学 · 物理学 2024-07-17 Michael Matlis , Juhi Dutta , Gudrid Moortgat-Pick , Andreas Ringwald

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

No-scale supergravity provides a successful framework for Starobinsky-like inflation models. Two classes of models can be distinguished depending on the identification of the inflaton with the volume modulus, $T$ (C-models), or a…

高能物理 - 唯象学 · 物理学 2020-01-15 Kunio Kaneta , Yann Mambrini , Keith A. Olive , Sarunas Verner

The cosmological relaxation of the electroweak scale has been proposed as a mechanism to address the hierarchy problem of the Standard Model. A field, the relaxion, rolls down its potential and, in doing so, scans the squared mass parameter…

高能物理 - 唯象学 · 物理学 2018-02-21 Walter Tangarife , Kohsaku Tobioka , Lorenzo Ubaldi , Tomer Volansky

We investigate the scenario where the Standard Model is extended with classical scale invariance, which is broken by chiral symmetry breaking and confinement in a new strongly-coupled gauge theory that resembles QCD. The Standard Model…

高能物理 - 唯象学 · 物理学 2017-06-21 Naoyuki Haba , Toshifumi Yamada

Motivated by the coincidence between the Hubble scale during inflation and the typical see-saw neutrino mass scale, we present a supergravity model where the inflaton is identified with a linear combination of right-handed sneutrino fields.…

高能物理 - 唯象学 · 物理学 2015-07-29 Jason L. Evans , Tony Gherghetta , Marco Peloso

We introduce a new method that allows for the Higgs to be the inflaton. That is, we let the Higgs be a pseudo-Nambu-Goldstone (pNG) boson of a global coset symmetry $G/H$ that spontaneously breaks at an energy scale $\sim 4\pi f$ and give…

高能物理 - 唯象学 · 物理学 2023-07-28 Stephon Alexander , Cyril Creque-Sarbinowski , Humberto Gilmer , Katherine Freese

Usual inflation is realized with a slow rolling scalar field minimally coupled to gravity. In contrast, we consider dynamics of a scalar with a flat effective potential, conformally coupled to gravity. Surprisingly, it contains an attractor…

高能物理 - 理论 · 物理学 2008-11-26 Lev Kofman , Shinji Mukohyama

We present an extended version of the Conformal Standard Model (characterized by the absence of any new intermediate scales between the electroweak scale and the Planck scale) with an enlarged scalar sector coupling to right-chiral…

高能物理 - 唯象学 · 物理学 2015-11-05 Adam Latosinski , Adrian Lewandowski , Krzysztof A. Meissner , Hermann Nicolai

We discuss the cosmological phenomenology of biscalar-tensor models displaying a maximally symmetric Einstein-frame kinetic sector and constructed on the basis of scale symmetry and volume-preserving diffeomorphisms. These theories contain…

宇宙学与河外天体物理 · 物理学 2019-03-20 Santiago Casas , Georgios K. Karananas , Martin Pauly , Javier Rubio

In this talk, I shall focus on theories beyond the Standard Model which predict massive neutrinos. Hybrid inflation emerges naturally in these theories: the slow-rolling inflaton field is a gauge singlet which couples with a GUT Higgs field…

高能物理 - 唯象学 · 物理学 2007-05-23 Rachel Jeannerot

Natural inflation is an attractive model for primordial inflation, since the potential for the inflaton is of the pseudo Nambu-Goldstone form, $V(\phi)=\Lambda^4 [1+\cos (\phi/f)]$, and so is protected against radiative corrections.…

宇宙学与河外天体物理 · 物理学 2018-11-19 Ricardo Z. Ferreira , Alessio Notari , Guillem Simeon