Theoretical Cosmology

Lead Research Organisation: University of Portsmouth
Department Name: Institute of Cosmology and Gravitation

Abstract

In recent years there has been an explosion in the amount and precision of observational data with which we can probe models of our Universe. This enables us to test speculative ideas about the physics at work in the very early Universe, the material content of the universe today, and even the nature of gravity and spacetime. A period of rapid, accelerated expansion in the very early universe, known as cosmological inflation provides the initial conditions from which the large scale structure of our universe can subsequently evolve. Quantum fluctuations during inflation are swept up to astrophysical scales by the rapid expansion, and we can distinguish between different possible models of inflation by the spectrum of fluctuations they leave behind. We intend to study the type of density fluctuations they produce, and the statistical properties of these fluctuations both in large galaxy surveys and in the pattern of temperature fluctuations in the cosmic microwave background radiation, which survives as a relic of the hot big bang. The most dramatic discovery in science in the past decade has been the revelation that the expansion of our Universe is actually accelerating today. This implies that the expansion must be driven, not by ordinary matter but by an unknown dark energy, similar to the quantum fields that drove inflation at high energies in the very early universe. However we have no clear idea what low-energy physics could lie behind the dark energy. It is important to distinguish the whether this dark energy is a cosmological constant, or whether it could vary in space and time. The growth of structure in our Universe revealed by observational surveys will be used to study the clustering of dark energy. In particular we will use weak gravitational lensing to probe the distribution of energy density in our Universe and an effect known as the integrated Sachs-Wolfe effect which probes the evolution of the gravitational potential as structure forms. We will also develop geometrical tests of the expansion history of our Universe, preparing for the next generation of massive cosmological data-sets that will be available to researchers in Portsmouth. We will develop advanced methods for cosmological data analysis with such surveys and make projections of the accuracy of geometrical tests. We will be seeking to distinguish models of dark energy from an alternative possibility that Einstein's theory of general relativity iteslf is modified on large scales. Our view of gravity and spacetime has been revolutionised in recent years by brane-world models which propose that our observed Universe may in fact be a four-dimensional 'brane' (with three space dimensions plus time) embedded in a higher-dimensional bulk spacetime. This could reconcile our observed four-dimensional world with string theory that requires extra, hidden spatial dimensions. We will continue work to study the implications of such brane-world models through their effect on models of inflation in the early universe, the evolution of cosmological structure, and the late-time acceleration of our Universe.

Publications

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Abazajian K (2009) THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY in The Astrophysical Journal Supplement Series

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Arroja F (2007) Low energy effective theory on a regularized brane in 6D gauged chiral supergravity in Journal of Cosmology and Astroparticle Physics

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Arroja F (2009) Full trispectrum in single field DBI inflation in Physical Review D

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Arroja F (2008) Non-Gaussianity from the bispectrum in general multiple field inflation in Journal of Cosmology and Astroparticle Physics

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Assadullahi H (2009) Gravitational waves from an early matter era in Physical Review D

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Assadullahi H (2007) Primordial non-Gaussianity from two curvaton decays in Physical Review D

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Barrow J (2007) Cosmology with inhomogeneous magnetic fields in Physics Reports

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Beynon E (2010) Weak lensing predictions for modified gravities at non-linear scales in Monthly Notices of the Royal Astronomical Society

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Bozza V (2009) A solution to the anisotropy problem in bouncing cosmologies in Journal of Cosmology and Astroparticle Physics

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Byrnes C (2010) Scale dependence of local f NL in Journal of Cosmology and Astroparticle Physics

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Byrnes C (2007) Diagrammatic approach to non-Gaussianity from inflation in Journal of Cosmology and Astroparticle Physics

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Böhmer C (2008) Dynamics of dark energy with a coupling to dark matter in Physical Review D

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Cailleteau T (2008) Singularities in loop quantum cosmology. in Physical review letters

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Caldera-Cabral G (2009) Dynamics of interacting dark energy in Physical Review D

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Caldera-Cabral G (2009) The growth of structure in interacting dark energy models in Journal of Cosmology and Astroparticle Physics

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Cardoso A (2008) Generalized perturbation equations in bouncing cosmologies in Physical Review D

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Copeland E (2007) Cosmological matching conditions in Journal of Cosmology and Astroparticle Physics

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Corradini O (2008) Induced gravity on intersecting brane worlds. II. Cosmology in Physical Review D

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Cresswell J (2009) Scale-dependent galaxy bias in the Sloan Digital Sky Survey as a function of luminosity and colour in Monthly Notices of the Royal Astronomical Society

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Crittenden R (2009) Investigating dark energy experiments with principal components in Journal of Cosmology and Astroparticle Physics

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De Risi G (2007) Graceful exit via polymerization of pre-big-bang cosmology in Physical Review D

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Durrer R (2007) Dark energy and dark gravity: theory overview in General Relativity and Gravitation

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Ellis G (2007) Editorial on the GRG special issue on dark energy in General Relativity and Gravitation

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Ellis G (2007) Causality and the speed of sound in General Relativity and Gravitation

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Esposito-Farèse G (2010) Vector theories in cosmology in Physical Review D

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Giannantonio T (2007) The effect of reionization on the cosmic microwave background-density correlation in Monthly Notices of the Royal Astronomical Society

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Hikage C (2009) Limits on isocurvature perturbations from non-Gaussianity in WMAP temperature anisotropy in Monthly Notices of the Royal Astronomical Society

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Hollenstein L (2009) Constraints on early dark energy from CMB lensing and weak lensing tomography in Journal of Cosmology and Astroparticle Physics

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Hollenstein L (2008) Challenges for creating magnetic fields by cosmic defects in Physical Review D

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Keskitalo R (2007) Hints of isocurvature perturbations in the cosmic microwave background? in Journal of Cosmology and Astroparticle Physics

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Kobayashi T (2007) Cosmological magnetic fields from nonlinear effects in Physical Review D

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Koyama K (2009) Velocities as a probe of dark sector interactions in Journal of Cosmology and Astroparticle Physics

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Koyama K (2007) Primordial perturbations from slow-roll inflation on a brane in Journal of Cosmology and Astroparticle Physics

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Koyama K (2007) Non-Gaussianities from ekpyrotic collapse with multiple fields in Journal of Cosmology and Astroparticle Physics

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Koyama K (2010) Non-Gaussianity of quantum fields during inflation in Classical and Quantum Gravity

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Koyama K (2009) Ghosts in asymmetric brane gravity and the decoupled stealth limit in Journal of High Energy Physics

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Koyama K (2007) Ghosts in the self-accelerating universe in Classical and Quantum Gravity