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The Higgs potential appears to be fine-tuned, hence very sensitive to values of other scalar fields that couple to the Higgs. We show that this feature can lead to a new epoch in the early universe featuring violent dynamics coupling the…

高能物理 - 唯象学 · 物理学 2019-02-20 Mustafa A. Amin , JiJi Fan , Kaloian D. Lozanov , Matthew Reece

We consider a multiverse scenario made up of classically disconnected regions of the space-time that are, nevertheless, in a quantum entangled state. The addition of a scalar field enriches the model and allows us to treat both the…

广义相对论与量子宇宙学 · 物理学 2015-06-17 Iñaki Garay , Salvador Robles-Pérez

We numerically compute features in the power-spectrum that originate from the decay of fields during inflation. Using a simple, phenomenological, multi-field setup, we increase the number of fields from a few to thousands. Whenever a field…

宇宙学与河外天体物理 · 物理学 2015-03-17 Diana Battefeld , Thorsten Battefeld , John T. Giblin , Evan K. Pease

Previously defined covariant and gauge-invariant perturbation variables, representing, e.g., the fractional spatial energy density gradient on hypersurfaces of constant expansion, are used to simplify the linear perturbation analysis of a…

天体物理学 · 物理学 2009-10-30 Winfried Zimdahl

We study the emergence of quantum entanglement in multi-field inflation. In this scenario, the perturbations of one field contribute to the observable curvature perturbation, while multi-field dynamics with the other fields affect the…

宇宙学与河外天体物理 · 物理学 2018-09-19 Nadia Bolis , Tomohiro Fujita , Shuntaro Mizuno , Shinji Mukohyama

It has been argued that oscillatory features from spectator fields in the primordial power spectrum could be a probe of alternatives to inflation. In this work, we soften this claim by showing that the frequency and amplitude dependence of…

宇宙学与河外天体物理 · 物理学 2019-01-29 Guillem Domènech , Javier Rubio , Julius Wons

If Higgs is a spectator scalar, i.e. if it is not directly coupled to the inflaton, superhorizon Higgs modes must have been exited during inflation. Since Higgs is unstable its decay into photons is expected to seed superhorizon photon…

广义相对论与量子宇宙学 · 物理学 2018-04-11 Ali Kaya

We study the details of eternal inflation in the presence of a spectator Higgs field within the framework of the minimal Standard Model. We have recently shown that in the presence of scalar field(s) which allow inflation only within a…

高能物理 - 唯象学 · 物理学 2020-05-11 Mudit Jain , Mark P. Hertzberg

In this paper we study the survival of entanglement of a scalar field state created during inflation. We find that there exist UV-finite subdominant contributions to the entanglement entropy per momentum mode that scale with the number of…

广义相对论与量子宇宙学 · 物理学 2020-02-13 Llorenç Espinosa-Portalés , Juan García-Bellido

Cosmological phase transitions are thought to have taken place at the early Universe imprinting their properties on the observable Universe. There is strong evidence that, through the dynamics of a scalar field that lead a second order…

广义相对论与量子宇宙学 · 物理学 2021-12-08 Orfeu Bertolami

We investigate entanglement of a quantum field in de Sitter spacetime using a particle detector model. By considering the entanglement between two comoving detectors interacting with a scalar field, it is possible to detect the entanglement…

广义相对论与量子宇宙学 · 物理学 2015-06-16 Yasusada Nambu

The accelerated expansion of the early universe is an integral part of modern cosmology and dynamically realized by the mechanism of inflation. The simplest theoretical description of the inflationary paradigm is based on the assumption of…

高能物理 - 唯象学 · 物理学 2021-04-14 Christian F. Steinwachs

We propose a possible quantum signature of the early Universe that could lead to observational imprints of the quantum nature of the inflationary period. Graviton production from the presence of a classical, coherent state of the inflaton…

宇宙学与河外天体物理 · 物理学 2026-03-30 Pablo Tejerina-Pérez , Daniele Bertacca , Raul Jimenez , Leonid Sarieddine

Inflation in the early Universe is one of the most promising probes of gravity in the high-energy regime. However, observable scales give access to a limited window in the inflationary dynamics. In this essay, we argue that quantum…

高能物理 - 理论 · 物理学 2017-11-22 Robert J. Hardwick , Vincent Vennin , David Wands

There exist observational evidence to believe the existence of primordial magnetic fields generated during inflation. We study primordial gravitational waves (PGWs) during inflation in the presence of magnetic fields sustained by a gauge…

高能物理 - 理论 · 物理学 2023-06-09 Sugumi Kanno , Ann Mukuno , Jiro Soda , Kazushige Ueda

We study the entanglement entropy resulting from tracing out local degrees of freedom of a quantum scalar field in an expanding universe. It is known that when field modes become superhorizon during inflation they evolve to increasingly…

高能物理 - 理论 · 物理学 2023-10-30 Konstantinos Boutivas , Georgios Pastras , Nikolaos Tetradis

Inflation, a period of exponential expansion in the early Universe, is considered an important part of the standard $\Lambda$CDM cosmological model, and plays a crucial role in explaining a wide range of current observations. The standard…

广义相对论与量子宇宙学 · 物理学 2023-12-08 Maria Pia Piccirilli , Gabriel Leon

We investigate the behavior of the entanglement entropy of space in the primordial phase of the universe before the beginning of cosmic inflation. We argue that in this phase the entanglement entropy of a region of space grows from a…

广义相对论与量子宇宙学 · 物理学 2015-12-31 Eugenio Bianchi , Lucas Hackl , Nelson Yokomizo

Inflation is nowadays a well-established paradigm consistent with all the observations. The precise nature of the inflaton is however unknown and its role could be played by any candidate able to imitate a scalar condensate in the slow-roll…

高能物理 - 唯象学 · 物理学 2015-09-02 Javier Rubio

A mathematical model of the cosmological evolution of statistical systems of scalarly charged particles with Higgs scalar interaction is formulated and investigated. Examples are given of numerical modeling of such systems, revealing their…

综合物理 · 物理学 2020-10-08 Yu. G. Ignat'ev