papers

Publications (14)

astro-ph1995

Mixed Cold-Hot Dark Matter Model with several Massive Neutrino Types

Dmitri Pogosyan, Alexei Starobinsky

Mixed cold-hot dark matter cosmological models (CHDM) with , approximately flat initial spectrum of adiabatic perturbations and 1, 2 or 3 types of massive neutrinos are…

astro-ph.CO2009

Signatures of a Graviton Mass in the Cosmic Microwave Background

Sergei Dubovsky, Raphael Flauger, Alexei Starobinsky +1

There exist consistent low energy effective field theories describing gravity in the Higgs phase that allow the coexistence of massive gravitons and the conventional 1/r potential…

hep-th2002

Prospects and Problems of Tachyon Matter Cosmology

Andrei Frolov, Lev Kofman, Alexei Starobinsky

We consider the evolution of FRW cosmological models and linear perturbations of tachyon matter rolling towards a minimum of its potential. The tachyon coupled to gravity is descri…

hep-ph1996

Comments on "Analytic and Numerical Study of Preheating Dynamics"

Lev Kofman, Andrei Linde, Alexei Starobinsky

In a recent paper Boyanovsky et al (hep-ph/9608205) studied preheating for a particular theory of the inflaton field. Although they results essentially confirm those of the origina…

astro-ph2000

The Case for a Positive Cosmological Lambda-term

Varun Sahni, Alexei Starobinsky

Recent observations of Type 1a supernovae indicating an accelerating universe have once more drawn attention to the possible existence, at the present epoch, of a small positive La…

hep-th1994

Reheating after Inflation

Lev Kofman, Andrei Linde, Alexei Starobinsky

The theory of reheating of the Universe after inflation is developed. The transition from inflation to the hot Universe turns out to be strongly model-dependent and typically consi…

astro-ph.CO2014

PRISM (Polarized Radiation Imaging and Spectroscopy Mission): An Extended White Paper

PRISM Collaboration, Philippe André, Carlo Baccigalupi +140

PRISM (Polarized Radiation Imaging and Spectroscopy Mission) was proposed to ESA in May 2013 as a large-class mission for investigating within the framework of the ESA Cosmic Visio…

astro-ph1994

Mixed Cold-Hot Dark Matter Model with Falling and Quasi-Flat Initial Perturbation Spectra

Dmitri Pogosyan, Alexei Starobinsky

The mixed cold-hot dark matter cosmological model (CHDM) with and a falling power-law initial spectrum of Gaussian adiabatic perturbations () is tested using rece…

hep-ph1997

Towards the Theory of Reheating After Inflation

Lev Kofman, Andrei Linde, Alexei Starobinsky

Reheating after inflation occurs due to particle production by the oscillating inflaton field. In this paper we describe the perturbative approach to reheating, and then concentrat…

astro-ph.CO2011

Curing singularities in cosmological evolution of F(R) gravity

Stephen Appleby, Richard Battye, Alexei Starobinsky

We study modified gravity models which are capable of driving the accelerating epoch of the Universe at the present time whilst not destroying the standard Big Bang and infl…

hep-th2002

Caustics in Tachyon Matter and Other Born-Infeld Scalars

Gary Felder, Lev Kofman, Alexei Starobinsky

We consider scalar Born-Infeld type theories with arbitrary potentials V(T) of a scalar field T. We find that for models with runaway potentials V(T) the generic inhomogeneous solu…

hep-ph1997

Structure of Resonance in Preheating after Inflation

Patrick Greene, Lev Kofman, Andrei Linde +1

We consider preheating in the theory , where the classical oscillating inflaton field decays into -particles and -particles. The paramet…

astro-ph2005

Stability properties of some perfect fluid cosmological models

Vittorio Gorini, Alexander Kamenshchik, Ugo Moschella +2

Flat FRW perfect fluid cosmologies can be reproduced as particular solutions of suitable field theoretical models. Here we investigate the stability of perfect fluid model trajecto…

astro-ph2006

Reconstructing Dark Energy

Varun Sahni, Alexei Starobinsky

This review summarizes recent attempts to reconstruct the expansion history of the Universe and to probe the nature of dark energy. Reconstruction methods can be broadly classified…