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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
  • Teaching
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  • Outreach
  • Awards/News
  • 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

Thermalisation after inflation

(2000)

Authors:

Sacha Davidson, Subir Sarkar
More details from the publisher

Cosmic ray signatures of massive relic particles

ArXiv hep-ph/0005256 (2000)

Abstract:

The possibility that the Fermi scale is the only fundamental energy scale of Nature is under serious consideration at present, yet cosmic rays may already have provided direct evidence of new physics at a much higher scale. The recent detection of very high energy particles with no plausible astrophysical sources suggests that these originate from the slow decays of massive particles clustered in the halo of our Galaxy. Such particles had in fact been predicted to exist beforehand with mass and lifetime in the range required to explain the observations. I discuss recent work focussing on experimental tests of this speculative but exciting idea.
Details from ArXiV
More details from the publisher

Cosmic ray signatures of massive relic particles

(2000)
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Review of Particle Physics

15:1-4 (2000) 1-878

Authors:

DE Groom, M Aguilar-Benitez, C Amsler, RM Barnett, PR Burchat, CD Carone, C Caso, G Conforto, O Dahl, M Doser, S Eidelman, JL Feng, L Gibbons, M Goodman, C Grab, A Gurtu, K Hagiwara, KG Hayes, JJ Hernández, K Hikasa, K Honscheid, C Kolda, ML Mangano, AV Manohar, A Masoni, K Mönig, H Murayama, K Nakamura, S Navas, KA Olive, L Pape, A Piepke, M Roos, M Tanabashi, NA Törnqvist, TG Trippe, P Vogel, CG Wohl, RL Workman, WM Yao, B Armstrong, JL Casas Serradilla, BB Filimonov, PS Gee, SB Lugovsky, F Nicholson, KS Babu, D Besson, O Biebel, P Bloch, RN Cahn, A Cattai, RS Chivukula, RD Cousins, T Damour, K Desler, RJ Donahue, DA Edwards, J Erler, VV Ezhela, A Fasso, W Fetscher, D Froidevaux, M Fukugita, TK Gaisser, L Garren, S Geer, HJ Gerber, FJ Gilman, HE Haber, C Hagmann, I Hinchliffe, CJ Hogan, G Hohler, P Igo-Kemenes, JD Jackson, KF Johnson, D Karlen, B Kayser, SR Klein, K Kleinknecht, IG Knowles, EW Kolb, P Kreitz, R Landua, P Langacker, L Littenberg, DM Manley, J March-Russell, T Nakada, HR Quinn, G Raffelt, B Renk, L Rolandi, MT Ronan, LJ Rosenberg, HFW Sadrozinski, AI Sanda, M Schmitt, O Schneider, D Scott, WG Seligman, MH Shaevitz, T Sjostrand, GF Smoot, S Spanier, H Spieler, M Srednicki, A Stahl, T Stanev, M Suzuki, NP Tkachenko, MS Turner, G Valencia, K VanBibber, R Voss, D Ward, L Wolfenstein, J Womersley
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The Standard Big Bang Cosmology

Chapter in Large Scale Structure Formation, Springer Nature 247 (2000) 37-96
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