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We propose a general framework in which a phase transition is triggered during cosmic inflation by the slow-roll dynamics of a spectator field. The topological defects formed at the transition are inflated outside the horizon, reenter it…

高能物理 - 唯象学 · 物理学 2026-01-09 Yunjia Bao , Keisuke Harigaya

A scalar field with an exponential potential has the particular property that it is attracted into a solution in which its energy scales as the dominant component (radiation or matter) of the Universe, contributing a fixed fraction of the…

天体物理学 · 物理学 2009-10-30 Pedro G. Ferreira , Michael Joyce

We investigate various dark energy models by taking into account the thermal effects induced from Hawking radiation on the apparent horizon of the Universe, for example near a finite-time future singularity. If the dark energy density…

广义相对论与量子宇宙学 · 物理学 2021-02-17 Artyom V. Astashenok , Sergei D. Odintsov , Vasilis K. Oikonomou

We consider a universe with a positive effective cosmological constant and a nonminimally coupled scalar field. When the coupling constant is negative, the scalar field exhibits linear growth at asymptotically late times, resulting in a…

广义相对论与量子宇宙学 · 物理学 2015-04-06 Dražen Glavan , Tomislav Prokopec

The interplay between non-minimally coupled scalar fields and a kinetic-dominated era following the end of inflation triggers the spontaneous symmetry breaking of internal symmetries and the subsequent evolution of the fields towards large…

宇宙学与河外天体物理 · 物理学 2020-01-22 Dario Bettoni , Javier Rubio

The approximate late conformal time wavefunction for self-interacting scalar quantum fields in de Sitter space is computed. It dominates for conformal times much larger than a certain critical value, $\eta=\eta_{\text{crit}}$ which depends…

高能物理 - 理论 · 物理学 2013-10-14 Enrique Alvarez

In an (Anti-) de Sitter space and a charged black hole the Schwinger effect is either enhanced by the Hawking radiation or suppressed by the negative curvature. We use the contour integral method to calculate the production of charged pairs…

高能物理 - 理论 · 物理学 2016-03-16 Sang Pyo Kim

We explore the consequences of the existence of a very large number of light scalar degrees of freedom in the early universe. We distinguish between participator and spectator fields. The former have a small mass, and can contribute to the…

高能物理 - 理论 · 物理学 2009-05-11 Peter Adshead , Richard Easther , Eugene A. Lim

The main consequences of de Sitter Special Relativity to the Standard Cosmological Model of Physical Cosmology are examined. The cosmological constant Lambda appears, in this theory, as a manifestation of the proper conformal current, which…

广义相对论与量子宇宙学 · 物理学 2010-01-08 R. Aldrovandi , J. G. Pereira

We study evolution and thermodynamics of a slow-roll transition between early and late time de Sitter phases, both in the homogeneous case and in the presence of a black hole, in a scalar field model with a generic potential having both a…

高能物理 - 理论 · 物理学 2017-11-22 Ruth Gregory , David Kastor , Jennie Traschen

We investigate analytically and numerically the orbits of spinning particles around black holes in the post Newtonian limit and in the presence of cosmic expansion. We show that orbits that are circular in the absence of spin, get deformed…

广义相对论与量子宇宙学 · 物理学 2019-05-22 I. Antoniou , D. Papadopoulos , L. Perivolaropoulos

A thermodynamical description for the quasi-static collapse of radiating, self-gravitating spherical shells of matter in anti-de Sitter space-time is obtained. It is shown that the specific heat at constant area and other thermodynamical…

广义相对论与量子宇宙学 · 物理学 2008-11-26 G. L. Alberghi , R. Casadio , G. Venturi

We consider, in de Sitter spacetime, both freely falling and static two-level atoms in interaction with a conformally coupled massless scalar field in the de Sitter-invariant vacuum, and separately calculate the contributions of vacuum…

高能物理 - 理论 · 物理学 2008-11-26 Zhiying Zhu , Hongwei Yu

De Sitter space-time, essentially our own universe, is plagued by problems at the quantum level. Here we propose that Lorentzian de Sitter space-time is not fundamental but constitutes only an effective description of a more fundamental…

高能物理 - 理论 · 物理学 2023-04-12 Carlo A. Trugenberger

Scalar-tensor theory of gravity with non-minimal coupling is a fairly good candidate for dark energy, required to explain late-time cosmic evolution. Here we study the very early stage of evolution of the universe with a modified version of…

高能物理 - 理论 · 物理学 2018-05-22 Ranajit Mandal , Chandramouli Sarkar , Abhik Kumar Sanyal

The scalar particle production from vacuum in the presence of electric field, on the de Sitter spacetime is studied. We use perturbation methods to define the transition amplitude. We obtain that the momentum is not conserved in this…

高能物理 - 理论 · 物理学 2014-08-29 Băloi Mihaela-Andreea

We consider the response of an Unruh detector to scalar fields in an expanding space-time. When combining transition elements of the scalar field Hamiltonian with the interaction operator of detector and field, one finds at second order in…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Bjorn Garbrecht , Tomislav Prokopec

Spatial fluctuations of the local electric field induced by a constant applied electric field in composite media are studied analytically and numerically. It is found that the density of states for the fields exhibit sharp peaks and abrupt…

统计力学 · 物理学 2007-05-23 D. Cule , S. Torquato

The behaviour of a static thin shell embedded in dS space is investigated. To satisfy the junction conditions at the boundary, one rescales the time variable. The surface energy $\sigma$ on the shell is positive but its surface tension…

广义相对论与量子宇宙学 · 物理学 2017-05-31 Hristu Culetu

We investigate scalar-induced stochastic gravitational waves from adiabatic curvature perturbations sourced by a spectator field via the modulated reheating mechanism. We consider a spectator scalar with Higgs-like couplings and inflaton…

宇宙学与河外天体物理 · 物理学 2026-04-30 Michele Benaco , Dimitrios Karamitros , Sami Nurmi , Kimmo Tuominen