51猎奇入口

Skip to main content
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • 51猎奇入口
    • Undergraduates
    • Postgraduates
  • Engage
    • For young people
    • For teachers
    • For the public
    • For alumni
    • For business
  • Support
Menu
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

Non-Gaussian spectra in cosmic microwave background temperature anisotropies

PHYSICAL REVIEW D 55:6 (1997) 3358-3372

Authors:

PG Ferreira, J Magueijo

Polarization-temperature correlation from a primordial magnetic field

PHYSICAL REVIEW D 56:12 (1997) R7493-R7497

Authors:

ES Scannapieco, PG Ferreira

Structure formation with a self-tuning scalar field

PHYSICAL REVIEW LETTERS 79:24 (1997) 4740-4743

Authors:

PG Ferreira, M Joyce

Non-Gaussian Spectra

(1996)

Authors:

Pedro G Ferreira, Joao Magueijo

How Anisotropic is our Universe?

Phys.Rev.Lett. 77 (1996) 2883-2886

Authors:

EF Bunn, P Ferreira, J Silk

Abstract:

Large-scale cosmic microwave background anisotropies in homogeneous, globally anisotropic cosmologies are investigated. We perform a statistical analysis in which the four-year data from the Cosmic Background Explorer satellite is searched for the specific anisotropy patterns predicted by these models and thereby set definitive upper limits on the amount of shear, $(\sigma/H)_0$ and vorticity, $(\omega/H)_0$, which are orders of magnitude stronger than previous constraints. We comment on how these results might impact our understanding of primordial global anisotropy.

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 127
  • Page 128
  • Page 129
  • Page 130
  • Current page 131
  • Page 132
  • Page 133
  • Page 134
  • Page 135
  • …
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

Department Of Physics text logo

漏 University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

  • Home
  • Research
  • 51猎奇入口
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • 51猎奇入口
  • Giving to Physics