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where I'd like to be ...

Prof Subir Sarkar

Professor Emeritus

Research theme

  • Particle astrophysics & cosmology
  • Fundamental particles and interactions

Sub department

  • Rudolf Peierls Centre for Theoretical Physics

Research groups

  • Particle theory
Subir.Sarkar@physics.ox.ac.uk
Telephone: 01865 (2)73962
Rudolf Peierls Centre for Theoretical Physics, room 60.12
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Brief CV
  • About
  • Research
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  • IceCube@Oxford
  • Publications

IceCube

Physics World 2013 Breakthrough of the Year
IceCube at Oxford

I am a member since 2004 of the IceCube collaboration which discovered cosmic high energy neutrinos and identified some of their astrophysical sources.

IceCube @ Oxford

Big Bang Nucleosynthesis (in "The Review of Particle Properties" 2004)

(2004)

Authors:

Brian Fields, Subir Sarkar
More details from the publisher

Have Atmospheric Cerenkov Telescopes Observed Dark Matter?

(2004)

Authors:

Dan Hooper, Ignacio de la Calle Perez, Joseph Silk, Francesc Ferrer, Subir Sarkar
More details from the publisher

Reply to ``Cuts and penalties: comment on `The clustering of ultra-high energy cosmic rays and their sources' ''

(2004)

Authors:

NW Evans, Francesc Ferrer, Subir Sarkar
More details from the publisher

Reply to “Comment on ‘Clustering of ultrahigh energy cosmic rays and their sources’ ”

Physical Review D Particles Fields Gravitation and Cosmology 69:12 (2004)

Authors:

NW Evans, F Ferrer, S Sarkar

Abstract:

We reiterate that there is no evidence that BL Lacs are sources of ultrahigh energy cosmic rays. © 2004 The American Physical Society.
More details from the publisher
More details

New physics from ultrahigh energy cosmic rays

ACTA PHYS POL B 35:1 (2004) 351-364

Abstract:

Observations of cosmic rays with energies above similar to 4 x 10(10) GeV have inspired several speculative suggestions concerning their origin. The crucial question is whether or not the spectrum exhibits the expected 'GZK cutoff' at this energy-concerning which there are presently contradictory results. If there is indeed a cutoff, then the sources are cosmologically distant and rather exotic in nature. If there is no cutoff then new physics is required.
More details
Details from ArXiV

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