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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Professor Pedro Ferreira

Professor of Astrophysics

Research theme

  • Particle astrophysics & cosmology

Sub department

  • Astrophysics

Research groups

  • Beecroft Institute for Particle Astrophysics and Cosmology
pedro.ferreira@physics.ox.ac.uk
Telephone: 01865 (2)73366
Denys Wilkinson Building, room 757
Personal Webpage
  • About
  • Publications

Observing the temperature of the Big Bang through large scale structure

(2007)

Authors:

Pedro Ferreira, Joao Magueijo
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Observing the temperature of the Big Bang through large scale structure

ArXiv 0708.0429 (2007)

Authors:

Pedro Ferreira, Joao Magueijo

Abstract:

It is widely accepted that the Universe underwent a period of thermal equilibrium at very early times. One expects a residue of this primordial state to be imprinted on the large scale structure of space time. In this paper we study the morphology of this thermal residue in a universe whose early dynamics is governed by a scalar field. We calculate the amplitude of fluctuations on large scales and compare it to the imprint of vacuum fluctuations. We then use the observed power spectrum of fluctuations on the cosmic microwave background to place a constraint on the temperature of the Universe before and during inflation. We also present an alternative scenario where the fluctuations are predominantly thermal and near scale-invariant.
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Generalized Einstein-Aether theories and the Solar System

(2007)

Authors:

Camille Bonvin, Ruth Durrer, Pedro G Ferreira, Glenn Starkman, Tom G Zlosnik
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Generalized Einstein-Aether theories and the Solar System

ArXiv 0707.3519 (2007)

Authors:

Camille Bonvin, Ruth Durrer, Pedro G Ferreira, Glenn Starkman, Tom G Zlosnik

Abstract:

It has been shown that generalized Einstein-Aether theories may lead to significant modifications to the non-relativistic limit of the Einstein equations. In this paper we study the effect of a general class of such theories on the Solar System. We consider corrections to the gravitational potential in negative and positive powers of distance from the source. Using measurements of the perihelion shift of Mercury and time delay of radar signals to Cassini, we place constraints on these corrections. We find that a subclass of generalized Einstein-Aether theories are compatible with these constraints.
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Searching for non Gaussian signals in the BOOMERanG 2003 CMB maps

ArXiv 0705.1615 (2007)

Authors:

G De Troia, PAR Ade, JJ Bock, JR Bond, J Borrill, A Boscaleri, P Cabella, CR Contaldi, BP Crill, P de Bernardis, G De Gasperis, A de Oliveira-Costa, G Di Stefano, PG Ferreira, E Hivon, AH Jaffe, TS Kisner, M Kunz, WC Jones, AE Lange, M Liguori, S Masi, S Matarrese, PD Mauskopf, CJ MacTavish, A Melchiorri, TE Montroy, P Natoli, CB Netterfield, E Pascale, F Piacentini, D Pogosyan, G Polenta, S Prunet, S Ricciardi, G Romeo, JE Ruhl, P Santini, M Tegmark, M Veneziani, N Vittorio

Abstract:

We analyze the BOOMERanG 2003 (B03) 145 GHz temperature map to constrain the amplitude of a non Gaussian, primordial contribution to CMB fluctuations. We perform a pixel space analysis restricted to a portion of the map chosen in view of high sensitivity, very low foreground contamination and tight control of systematic effects. We set up an estimator based on the three Minkowski functionals which relies on high quality simulated data, including non Gaussian CMB maps. We find good agreement with the Gaussian hypothesis and derive the first limits based on BOOMERanG data for the non linear coupling parameter f_NL as -300
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