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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
  • Teaching
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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

Domain wall problems for the NMSSM

High-energy physics. Proceedings, International Europhysics Conference, HEP ’95, Brussels, Belgium, July 27-August 2, 1995 (1995)

Authors:

S Abel, Subir Sarkar, P White

Cosmological Constraints on Perturbative Supersymmetry Breaking

ArXiv hep-ph/9409350 (1994)

Authors:

SA Abel, S Sarkar

Abstract:

We discuss the cosmology of string models with perturbative supersymmetry breaking at a scale of ${\cal O}$(TeV). Such models exhibit Kaluza-Klein like spectra and contain unstable massive gravitinos/gravitons. We find that considerations of primordial nucleosynthesis constrain the maximum temperature following inflation to be not much larger than the supersymmetry breaking scale. This imposes conflicting requirements on the scalar field driving inflation, making it rather difficult to construct a consistent cosmological history for such models.
Details from ArXiV
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Cosmological Constraints on Perturbative Supersymmetry Breaking

(1994)

Authors:

SA Abel, S Sarkar
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Cosmic neutrinos from unstable relic particles

Nuclear Physics, Section B 392:1 (1993) 111-133

Authors:

P Gondolo, G Gelmini, S Sarkar

Abstract:

We derive constraints on the relic abundance of a generic particle of mass ∼ 1-1014 TeV which decays into neutrinos at cosmological epochs, using data from the Fréjus and IMB nucleon decay detectors and the Fly's Eye air-shower array. The lifetime of such unstable particles which may constitute the dark matter today is bounded to be greater than ∼ 1014-1018 yr, depending on the mass. For lifetimes shorter than the age of the universe, neutrino energy losses due to scattering and the expansion redshift become important and set limits to the ability of neutrino observatories to probe the early universe. © 1993.
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FURTHER RESULTS ON CERIUM FLUORIDE-CRYSTALS

NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT 332:3 (1993) 373-394

Authors:

S ANDERSON, E AUFFRAY, T AZIZ, S BACCARO, S BANERJEE, P BAREYRE, LE BARONE, B BORGIA, D BOUTET, JP BURQ, M CHEMARIN, R CHIPAUX, I DAFINEI, P DATANASIO, F DENOTARISTEFANI, B DEZILLIE, C DUJARDIN, S DUTTA, JL FAURE, J FAY, D FERRERE, O FRANCESCANGELI, BA FUCHS, SN GANGULI, G GILLESPIE, M GOYOT, SK GUPTA, A GURTU, J HECK, A HERVE, H HILLEMANNS, F HOLDENER, B ILLE, L JONSSON, J KIERSTEAD, W KRENZ, W KWAY, JM LEGOFF, M LEBEAU, P LEBRUN, P LECOQ, Y LEMOIGNE, G LOOMIS, K LUBELSMEYER, N MADJAR, G MAJNI, H ELMAMOUNI, S MANGLA, JA MARES, JP MARTIN, M MATTIOLI, GJ MAUGER, K MAZUMDAR, P MENGUCCI, JP MERLO, B MOINE, N NIKL, JP PANSART, C PEDRINI, J POINSIGNON, K POLAK, R RAGHAVAN, P REBOURGEARD, D RINALDI, J ROSA, A ROSOWSKY, P SAHUC, V SAMSONOV, S SARKAR, V SCHEGELSKI, D SCHMITZ, M SCHNEEGANS, D SELIVERSTOV, S STOLL, K SUDHAKAR, A SVENSSON, SC TONWAR, V TOPA, JP VIALLE, M VIVARGENT, W WALLRAFF, MJ WEBER, N WINTER, C WOODY, CR WUEST, V YANOVSKI
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