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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
  • FASER2
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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  • 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

The Impact of Heavy Nuclei on the Cosmogenic Neutrino Flux

(2004)

Authors:

Dan Hooper, Andrew Taylor, Subir Sarkar
More details from the publisher

Review of particle physics

592:1-4 (2004) 1-5

Authors:

S Eidelman, KG Hayes, KA Olive, M Aguilar-Benitez, C Amsler, D Asner, KS Babu, RM Barnett, J Beringer, PR Burchat, CD Carone, C Caso, G Conforto, O Dahl, G D'Ambrosio, M Doser, JL Feng, T Gherghetta, L Gibbons, M Goodman, C Grab, DE Groom, A Gurtu, K Hagiwara, JJ Hernández-Rey, K Hikasa, K Honscheid, H Jawahery, C Kolda, Y Kwon, ML Mangano, AV Manohar, J March-Russell, A Masoni, R Miquel, K Mönig, H Murayama, K Nakamura, S Navas, L Pape, C Patrignani, A Piepke, G Raffelt, M Roos, M Tanabashi, J Terning, NA Törnqvist, TG Trippe, P Vogel, CG Wohl, RL Workman, WM Yao, PA Zyla, B Armstrong, PS Gee, G Harper, KS Lugovsky, SB Lugovsky, VS Lugovsky, A Rom, M Artuso, E Barberio, M Battaglia, H Bichsel, O Biebel, P Bloch, RN Cahn, D Casper, A Cattai, RS Chivukula, G Cowan, T Damour, K Desler, MA Dobbs, M Drees, A Edwards, DA Edwards, VD Elvira, J Erler, VV Ezhela, W Fetscher, BD Fields, B Foster, D Froidevaux, M Fukugita, TK Gaisser, L Garren, HJ Gerber, G Gerbier, FJ Gilman, HE Haber, C Hagmann, J Hewett, I Hinchliffe, CJ Hogan, G Höhler, P Igo-Kemenes, JD Jackson, KF Johnson, D Karlen

Abstract:

This biennial Review summarizes much of Particle Physics. Using data from previous editions, plus 1726 new measurements from 512 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. Among the 119 reviews are many that are new or heavily revised including those on neutrino mixing, CP violation in K, D, and B mesons, Vcb, the new exotic Θ(1540) particle, extra-dimensions, grand unified theories, cosmic background radiation, dark matter, cosmological parameters, and big bang cosmology. A booklet is available containing the Summary Tables and abbreviated versions ofsome 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. ©2004 Regents of the University of California.
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More details

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

Phys.Rev.D 69 (2004) 128302-128302

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.
More details from the publisher
Details from ORA
Details from ArXiV

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

ArXiv astro-ph/0406663 (2004)

Authors:

Brian Fields, Subir Sarkar

Abstract:

A critical review is given of the current status of cosmological nucleosynthesis. In the framework of the standard model with 3 types of relativistic neutrinos, the baryon-to-photon ratio, \eta, corresponding to the inferred primordial abundances of helium-4 and lithium-7 is presently ~2 \sigma below the value implied by the abundance of deuterium. The latter value is also coincident with the independent determination of \eta from WMAP observations of CMB anisotropy. However taking systematic uncertainties in the abundance estimates into account, there is overall concordance in the range \eta = (3.4 - 6.9) x 10^{-10} @ 95% c.l. corresponding to a cosmological baryon density \Omega_B h^2 = 0.012 - 0.025. If the above discrepancy is due to a neutrino chemical potential, then upto 7.1 effective neutrino species are allowed by nucleosynthesis. Other constraints on new physics are briefly discussed.
Details from ArXiV
More details from the publisher

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

(2004)

Authors:

Brian Fields, Subir Sarkar
More details from the publisher

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