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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
  • About
  • Publications

The C鈩揙VER experiment

Proceedings of SPIE--the International Society for Optical Engineering SPIE, the international society for optics and photonics 7020 (2008) 70201e-70201e-10

Authors:

L Piccirillo, P Ade, MD Audley, C Baines, R Battye, M Brown, P Calisse, A Challinor, WD Duncan, P Ferreira, W Gear, DM Glowacka, D Goldie, PK Grimes, M Halpern, V Haynes, GC Hilton, KD Irwin, B Johnson, M Jones, A Lasenby, P Leahy, J Leech, S Lewis, B Maffei, L Martinis, PD Mauskopf, SJ Melhuish, CE North, D O'Dea, S Parsley, G Pisano, CD Reintsema, G Savini, RV Sudiwala, D Sutton, A Taylor, G Teleberg, D Titterington, VN Tsaneva, C Tucker, R Watson, S Withington, G Yassin, J Zhang

Constraining Lorentz violation with cosmology

(2008)

Authors:

JA Zuntz, PG Ferreira, TG Zlosnik

Map-making in small field modulated CMB polarisation experiments: approximating the maximum-likelihood method

(2008)

Authors:

D Sutton, BR Johnson, ML Brown, P Cabella, PG Ferreira, KM Smith

Living in a Void: Testing the Copernican Principle with Distant Supernovae

(2008)

Authors:

Timothy Clifton, Pedro G Ferreira, Kate Land

Dark Matter, Modified Gravity and the Mass of the Neutrino

ArXiv 0806.0116 (2008)

Authors:

PG Ferreira, C Skordis, C Zunckel

Abstract:

It has been suggested that Einstein's theory of General Relativity can be modified to accomodate mismatches between the gravitational field and luminous matter on a wide range of scales. Covariant theories of modified gravity generically predict the existence of extra degrees of freedom which may be interpreted as dark matter. We study a subclass of these theories where the overall energy density in these extra degrees of freedom is subdominant relative to the baryon density and show that they favour the presence of massive neutrinos. For some specific cases (such as a flat Universes with a cosmological constant) one finds a conservative lower bound on the neutrinos mass of $m_\nu>0.31$ eV.

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