High-energy neutrinos from astrophysical accelerators of cosmic ray
nuclei
 Anchordoqui, L Hooper, D Sarkar, S Taylor, A Astropart.Phys. volume 29 1-13 (01 Mar 2007) http://arxiv.org/abs/astro-ph/0703001v4
On the APM power spectrum and the CMB anisotropy: Evidence for a phase
transition during inflation?
 Barriga, J Gaztanaga, E Santos, M Sarkar, S Mon.Not.Roy.Astron.Soc. volume 324 977 (21 Nov 2000) http://arxiv.org/abs/astro-ph/0011398v3
Measuring the baryon content of the universe: BBN vs CMB
 Sarkar, S in "Frontiers of the Universe", eds L Celnekier and J Tran Thanh Van (The Gioi Publishers, 2004) pp.53-63 (08 May 2002) http://arxiv.org/abs/astro-ph/0205116v1
An Alternative to the cosmological ’concordance model’
 Blanchard, A Douspis, M Rowan-Robinson, M Sarkar, S Astron.Astrophys. volume 412 35-44 (2003)
A ’Baedecker’ for the dark matter annihilation signal
 Evans, N Ferrer, F Sarkar, S Phys.Rev. volume D69 123501-123501 (2004)
Reply to ``Cuts and penalties: comment on `The clustering of ultra-high
energy cosmic rays and their sources' ''
 Evans, N Ferrer, F Sarkar, S Phys.Rev.D volume 69 128302-128302 (30 Jun 2004) http://arxiv.org/abs/astro-ph/0403527v1
Dark matter profiles and annihilation in dwarf spheroidal galaxies:
prospectives for present and future gamma-ray observatories - I. The
classical dSphs
 Charbonnier, A Combet, C Daniel, M Funk, S Hinton, J Maurin, D Power, C Read, J Sarkar, S Walker, M Wilkinson, M MNRAS volume 418 1526-1556 (03 Apr 2011) http://arxiv.org/abs/1104.0412v2
Direct detection of dark matter in models with a light Z'
 Frandsen, M Kahlhoefer, F Sarkar, S Schmidt-Hoberg, K JHEP volume 1109 128 (11 Jul 2011) http://arxiv.org/abs/1107.2118v2
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