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We study the role of domain walls and their relics in the very early Universe within the framework of the mode-matching technique. Domain walls formed during the spontaneous breaking of discrete symmetries are modelled as a short lived…

宇宙学与河外天体物理 · 物理学 2026-03-03 K. K. Venkataratnam

We formulate new conformal models of inflation and dark energy which generalise the Higgs-Dilaton scenario. We embed these models in unimodular gravity whose effect is to break scale invariance in the late time Universe. In the early…

宇宙学与河外天体物理 · 物理学 2015-06-18 P. Brax , A. C. Davis

The shortcomings of the Standard Big Bang Cosmological Model as well as their resolution in the context of inflationary cosmology are discussed. The inflationary scenario and the subsequent oscillation and decay of the inflaton field are…

高能物理 - 唯象学 · 物理学 2007-05-23 G. Lazarides

A problem with high central densities in dark halos has arisen in the context of LCDM cosmologies with scale-invariant initial power spectra. Although n=1 is often justified by appealing to the inflation scenario, inflationary models with…

天体物理学 · 物理学 2008-11-26 Andrew R. Zentner , James S. Bullock

In a recent paper, we suggested that the density fluctuation spectra arising from power-law (or extended) inflation, which are tilted with respect to the Harrison--Zel'dovich spectrum, may provide an explanation for the excess large scale…

天体物理学 · 物理学 2007-05-23 David H Lyth , Andrew A Liddle

It has been suggested that the dark energy density \rho_v ~ 10^{-12} eV^4 in the universe is associated with a metastable (false) vacuum, while the true vacuum has a vanishing cosmological constant. By including supergravity corrections we…

高能物理 - 唯象学 · 物理学 2009-11-11 Qaisar Shafi , Arunansu Sil , Siew-Phang Ng

A viable model of large-field (chaotic) inflation with efficient production of primordial black holes is proposed in Starobinsky-like (modified) supergravity leading to the "no-scale-type" K\"ahler potential and the Wess-Zumino-type…

宇宙学与河外天体物理 · 物理学 2024-09-05 Ryotaro Ishikawa , Sergei V. Ketov

We investigate the creation of dark matter particles as a result of the decay of the scalar field in the framework of warm inflationary models, by using the irreversible thermodynamics of open systems with matter creation/annihilation. We…

广义相对论与量子宇宙学 · 物理学 2023-03-07 Teodora Matei , Tiberiu Harko , Gabriela Mocanu

We investigate the inflationary consequences of the oscillating dark energy model proposed by Ti\'an [\href{https://doi.org/10.1103/PhysRevD.101.063531}{Phys. Rev. D {\bf 101}, 063531 (2020)}], which aims to solve the cosmological…

宇宙学与河外天体物理 · 物理学 2021-06-29 S. X. Tian , Zong-Hong Zhu

We consider inflation and supersymmetry breaking in the context of a minimal model of supersymmetry in which the only "low" energy remnant of supersymmetry is the gravitino with a mass of order an EeV. In this theory, the supersymmetry…

高能物理 - 唯象学 · 物理学 2018-01-03 Emilian Dudas , Tony Gherghetta , Yann Mambrini , Keith A. Olive

We investigate the recently proposed class of chaotic inflation models in supergravity with an arbitrary inflaton potential. These models are extended to include matter fields in the visible sector and we employ a mechanism of SUSY breaking…

高能物理 - 理论 · 物理学 2013-05-29 Renata Kallosh , Andrei Linde , Keith A. Olive , Tomas Rube

We consider how accelerated expansion, whether due to inflation or dark energy, imposes strong constraints on fundamental theories obtained by compactification from higher dimensions. For theories that obey the null energy condition (NEC),…

高能物理 - 理论 · 物理学 2009-07-30 Paul J. Steinhardt , Daniel Wesley

Axion models have two serious cosmological problems, domain wall and isocurvature perturbation problems. In order to solve these problems we investigate the Linde's model in which the field value of the Peccei-Quinn (PQ) scalar is large…

高能物理 - 唯象学 · 物理学 2013-11-14 Masahiro Kawasaki , Tsutomu T. Yanagida , Kazuyoshi Yoshino

In this paper we investigate a model of an inflationary universe in Kaluza-Klein theory, which is a four-dimensional de Sitter space plus a one-dimensional compactified internal space. We find that the energy scale for inflation can be…

天体物理学 · 物理学 2012-08-27 Li-Xin Li , J. Richard Gott , III

We extend to multidimensional cosmology Vilenkin's prescription of tunnelling from nothing for the quantum origin of the observable Universe. Our model consists of a $D+4$-dimensional spacetime of topology ${\cal R}\times {\cal S}^3…

广义相对论与量子宇宙学 · 物理学 2009-10-28 Enrico Carugno , Marco Litterio , Franco Occhionero , Giuseppe Pollifrone

Space-based missions studying the cosmic microwave background (CMB) have progressively refined the parameter space in conventional models of inflation shortly ($\sim 10^{-37}$ seconds) after the big bang. While most inflationary scenarios…

宇宙学与河外天体物理 · 物理学 2024-04-18 Jingwei Liu , Fulvio Melia

Though simple inflationary models describe the CMB well, their corrections are often plagued by infrared effects that obstruct a reliable calculation of late-time behaviour. We adapt to cosmology tools designed to address similar issues in…

广义相对论与量子宇宙学 · 物理学 2016-08-30 C. P. Burgess , R. Holman , G. Tasinato

The Starobinsky model of cosmological inflation in four spacetime dimensions is reviewed with the emphasis on impact of quantum gravity corrections. As a specific example of the quantum corrections, the Grisaru-Zanon quartic curvature terms…

广义相对论与量子宇宙学 · 物理学 2025-01-09 Shunsuke Toyama , Sergei V. Ketov

This paper focuses on the Starobinsky model of inflation. We derive solutions for various cosmological observables, such as the scalar spectral index $n_s$, the tensor-to-scalar ratio $r$ and their runnings, as well as the number of…

宇宙学与河外天体物理 · 物理学 2024-03-22 Gabriel German , Juan Carlos Hidalgo , Luis E. Padilla

General Relativity is extended into the quantum domain. A thought experiment is explored to derive a specific topological build-up for Planckian space-time. The presented arguments are inspired by Feynman's path integral for superposition…

综合物理 · 物理学 2013-07-18 Marco Spaans