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.

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.

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

(2004)

Authors:

Brian Fields, Subir Sarkar

Have Atmospheric Cerenkov Telescopes Observed Dark Matter?

(2004)

Authors:

Dan Hooper, Ignacio de la Calle Perez, Joseph Silk, Francesc Ferrer, Subir Sarkar

Have Atmospheric Cerenkov Telescopes Observed Dark Matter?

ArXiv astro-ph/0404205 (2004)

Authors:

Dan Hooper, Ignacio de la Calle Perez, Joseph Silk, Francesc Ferrer, Subir Sarkar

Abstract:

Two ground-based experiments have recently independently detected TeV $\gamma$-rays from the direction of the Galactic center. The observations made by the VERITAS and CANGAROO collaborations are unexpected, although not impossible to interpret in terms of astrophysical sources. Here we examine in detail whether the observed $\gamma$-rays may arise from the more exotic alternative of annihilations of dark matter particles clustered in the center of the Galaxy.