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The evolution of high order correlation functions of a test scalar field in arbitrary inflationary backgrounds is computed. Whenever possible, exact results are derived from quantum field theory calculations. Taking advantage of the fact…

宇宙学与河外天体物理 · 物理学 2011-03-18 Francis Bernardeau

In this manuscript, we propose the generation of complex vector beams with high quality and stability based on a novel approach that relies on the combination of two techniques that seem incompatible at first glance. The first is Complex…

Starting with geometrical premises, we infer the existence of fundamental cosmological scalar fields. We then consider physically relevant situations in which spacetime metric is induced by one or, in general, by two scalar fields, in…

广义相对论与量子宇宙学 · 物理学 2015-11-03 Eduard G. Mychelkin , Maxim A. Makukov

The intensive cosmological creation of vector W, Z- bosons in the cosmological model with the relative units is considered. Field theoretical models are studied, which predict that the CMB radiation and the baryon matter in the universe can…

高能物理 - 唯象学 · 物理学 2015-06-25 D. B. Blaschke , S. I. Vinitsky , A. A. Gusev , V. N. Pervushin , D. V. Proskurin

We study the cosmology of bimetric theory with a composite matter coupling. We find two possible branches of background evolution. We investigate the question of stability of cosmological perturbations. For the tensor and vector…

高能物理 - 理论 · 物理学 2015-06-23 A. Emir Gumrukcuoglu , Lavinia Heisenberg , Shinji Mukohyama , Norihiro Tanahashi

Doppler peaks in the cosmic microwave background may allow us to distinguish among the two classes of theories-inflationary models and topological defect scenarios-which attempt to explain the origin of structure formation in the universe.…

天体物理学 · 物理学 2011-04-15 Mairi Sakellariadou

We reconsider the gravitational wave spectrum induced by scalar perturbations in spatially flat Friedmann-Lema\^itre-Robertson-Walker spacetimes, focusing on the matter- and $\Lambda$-dominated epochs. During matter domination, sub-horizon…

宇宙学与河外天体物理 · 物理学 2023-03-31 Marvin Sipp , Bjoern Malte Schaefer

In almost all structure formation models, primordial perturbations are created within a homogeneous and isotropic universe, like the one we observe. Because their ensemble averages inherit the symmetries of the spacetime in which they are…

天体物理学 · 物理学 2009-06-23 C. Armendariz-Picon

Increasing the complexity of a light field through the advanced manipulation of its degrees of freedom (DoF) provides new opportunities for fundamental studies and technologies. Correlating polarization with the light's spatial or spectral…

光学 · 物理学 2026-03-12 Lea Kopf , Rafael Barros , Robert Fickler

Eigenfunctions of total angular momentum for a charged vector field interacting with a magnetic monopole are constructed and their properties studied. In general, these eigenfunctions can be obtained by applying vector operators to the…

高能物理 - 理论 · 物理学 2009-10-22 Erick J. Weinberg

A particular compensation-type solution of the main cosmological constant problem has been proposed recently, with two massless vector fields dynamically canceling an arbitrary cosmological constant \Lambda. The naive expectation is that…

广义相对论与量子宇宙学 · 物理学 2015-05-28 F. R. Klinkhamer

We compute the primordial trispectrum for curvature perturbations produced during cosmic inflation in models with standard kinetic terms, when the initial quantum state is not necessarily the vacuum state. The presence of initial…

宇宙学与河外天体物理 · 物理学 2015-06-03 Ivan Agullo , Jose Navarro-Salas , Leonard Parker

The primordial perturbations of test scalar fields not affecting the evolution of background may be very interesting since they can be transferred to the curvature perturbations by some mechanisms, and thus under certain condition can be…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Yun-Song Piao , Yuan-Zhong Zhang

We describe an attempt to reconstruct the initial conditions for the formation of cosmological large-scale structure. The power spectrum of the primordial fluctuations is affected by bias, nonlinear evolution and redshift-space distortions,…

天体物理学 · 物理学 2015-06-24 J. A. Peacock , S. J. Dodds

It has recently been shown that a Hagedorn phase of string gas cosmology can provide a causal mechanism for generating a nearly scale-invariant spectrum of scalar metric fluctuations, without the need for an intervening period of de Sitter…

高能物理 - 理论 · 物理学 2008-11-26 Robert H. Brandenberger , Ali Nayeri , Subodh P. Patil , Cumrun Vafa

We propose a cosmological dark matter production mechanism in the form of a longitudinal massive vector boson. We build upon the work of Graham et.al. including non-minimal couplings of the massive vector with gravity, developing a well…

宇宙学与河外天体物理 · 物理学 2023-10-16 Ogan Özsoy , Gianmassimo Tasinato

We investigate matter density perturbations in models of structure formation with or without causal/acausal source. Under the fluid approximation in the linear theory, we first derive full perturbation equations in flat space with a…

天体物理学 · 物理学 2007-05-23 Jiun-Huei Proty Wu

We discuss the possibility that dark matter is made of a new complex massive vector field with a global $U(1)$-symmetry. The field interacts with the Standard Model via coupling to the gauge field of the hypercharge group. We study…

高能物理 - 唯象学 · 物理学 2020-04-30 Emin Nugaev , Andrey Shkerin

We construct a position-space cosmological perturbation theory around spatially flat Friedmann-Lema\^itre-Robertson-Walker geometries that allows to model localized primordial sources of gravitational waves. The equations of motion are…

广义相对论与量子宇宙学 · 物理学 2026-04-13 Geoffrey Compère , Sk Jahanur Hoque

Gauge-invariant treatments of the second-order cosmological perturbation in a four dimensional homogeneous isotropic universe are formulated without any gauge fixing. We have derived the Einstein equations in the case of the single perfect…

广义相对论与量子宇宙学 · 物理学 2009-01-27 Kouji Nakamura
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