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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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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

The clustering of ultra-high energy cosmic rays and their sources

(2002)

Authors:

N Wyn Evans, Francesc Ferrer, Subir Sarkar

Review of Particle Physics: Particle data group

66:1 I (2002) 100011-10001958

Authors:

K Hagiwara, K Hikasa, K Nakamura, M Tanabashi, 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, DE Groom, A Gurtu, KG Hayes, JJ Hern谩ndez-Rey, K Honscheid, C Kolda, ML Mangano, DM Manley, AV Manohar, J March-Russell, A Masoni, R Miquel, K M枚nig, H Murayama, S Navas, KA Olive, L Pape, C Patrignani, A Piepke, M Roos, J Terning, NA T枚rnqvist, TG Trippe, P Vogel, CG Wohl, RL Workman, WM Yao, B Armstrong, PS Gee, KS Lugovsky, SB Lugovsky, VS Lugovsky, M Artuso, D Asner, KS Babu, E Barberio, M Battaglia, H Bichsel, O Biebel, P Bloch, RN Cahn, A Cattai, RS Chivukula, RD Cousins, G Cowan, T Damour, K Desler, RJ Donahue, DA Edwards, VD Elvira, J Erler, VV Ezhela, A Fass贸, W Fetscher, BD Fields, B Foster, D Froidevaux, M Fukugita, TK Gaisser, L Garren, HJ Gerber, FJ Gilman, HE Haber, C Hagmann, J Hewett, I Hinchliffe, CJ Hogan, G H枚hler, P Igo-Kemenes, JD Jackson, KF Johnson, D Karlen, B Kayser, SR Klein, K Kleinknecht, IG Knowles, P Kreitz, YV Kuyanov, R Landua, P Langacker, L Littenberg, AD Martin

Abstract:

This biennial Review summarizes much of Particle Physics. Using data from previous editions, plus 2205 new measurements from 667 papers, we list, evaluate, and average measured properties of gauge bosons, leptons, quarks, mesons, and baryons. We also summarize searches for hypothetical particles such as Higgs bosons, heavy neutrinos, and supersymmetric particles. All the particle properties and search limits are listed in Summary Tables. We also give numerous tables, figures, formulae, and reviews of topics such as the Standard Model, particle detectors, probability, and statistics. This edition features expanded coverage of CP violation in B mesons and of neutrino oscillations. For the first time we cover searches for evidence of extra dimensions (both in the particle listings and in a new review). Another new review is on Grand Unified Theories. A booklet is available containing the Summary Tables and abbreviated versions of some of the other sections of this full Review. All tables, listings, and reviews (and errata) are also available on the Particle Data Group website: http://pdg.lbl.gov.

Big Bang Nucleosynthesis

Nuclear and Particle Physics Proceedings Elsevier 110:2 (2002) 137-143

Possible astrophysical probes of quantum gravity

MOD PHYS LETT A 17:15-17 (2002) 1025-1035

Abstract:

A satisfactory theory of quantum gravity will very likely require modification of our classical perception of space-time, perhaps by giving it a 'foamy' structure at scales of order the Planck length. This is expected to modify the propagation of photons and other relativistic particles such as neutrinos, such that they will experience a non-trivial refractive index even in vacuo. The implied spontaneous violation of Lorentz invariance may also result in alterations of kinematical thresholds for key astrophysical processes involving high energy cosmic radiation. We discuss experimental probes of these possible manifestations of the fundamental quantum nature of space-time using observations of distant astrophysical sources such as gamma-ray bursts and active galactic nuclei.

Measuring the baryon content of the universe: BBN vs CMB

ArXiv astro-ph/0205116 (2002)

Abstract:

The relic abundance of baryons - the only form of stable matter whose existence we are certain of - is a crucial parameter for many cosmological processes, as well as material evidence that there is new physics beyond the Standard Model. We discuss recent determinations of the cosmological baryon density from analysis of the abundances of light elements synthesised at the end of ``the first three minutes'', and from the observed temperature anisotropies imprinted on small angular-scales in the cosmic microwave background when the universe was about 100,000 yr old.

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