Big bang nucleosynthesis limit on N_nu

ArXiv hep-ph/9901404 (1999)

Authors:

E Lisi, Subir Sarkar, FL Villante

Abstract:

Recently we presented a simple method for determining the correlated uncertainties of the light element abundances expected from big bang nucleosynthesis, which avoids the need for lengthy Monte Carlo simulations. We now extend this approach to consider departures from the Standard Model, in particular to constrain any new light degrees of freedom present in the thermal plasma during nucleosynthesis. Since the observational situation regarding the inferred primordial abundances has not yet stabilized, we present illustrative bounds on the equivalent number of neutrino species N_nu for various combinations of individual abundance determinations. Our 95% C.L. bounds on N_nu range between 2 and 4, and can easily be reevaluated using the technique provided when the abundances are known more accurately.

Big bang nucleosynthesis limit on N_nu

(1999)

Authors:

E Lisi, Subir Sarkar, FL Villante

Five--Branes and Supersymmetry Breaking in M--Theory

(1999)

Authors:

Andre Lukas, Burt A Ovrut, Daniel Waldram

Holomorphic Vector Bundles and Non-Perturbative Vacua in M-Theory

(1999)

Authors:

Ron Donagi, Andre Lukas, Burt A Ovrut, Daniel Waldram

Chiral symmetry breaking, instantons and the ultimate quenched calculation

Nuclear Physics B - Proceedings Supplements 73:1-3 (1999) 617-619

Authors:

U Sharan, M Teper

Abstract:

We calculate the spectral density of the Dirac operator over an ensemble of configurations composed of overlapping instantons and anti-instantons. We find evidence that the spectral density diverges in the limit λ → 0. This indicates the breaking of chiral symmetry and also provides evidence that quenched QCD may be pathological in nature.