A linear programming approach to inhomogeneous primordial nucleosynthesis
Richard E. Leonard, Robert J. Scherrer
Abstract
We examine inhomogeneous primordial nucleosynthesis for arbitrary distributions f of the baryon-to-photon ratio η, in the limit where neither particle diffusion nor gravitational collapse is important. By discretizing f(η) and using linear programming, we show that for a set of m constraints on the primordial element abundances, the maximum and minimum possible values of η (the final mean value of η) are given when f(η) is a sum of at most m+1 delta functions. Our linear programming results indicate that when f is taken to be an arbitrary function, there is no lower bound on η, while the upper bound is essentially the homogeneous upper bound.
Create a lesson
Related papers
On binary pulsars and the force of gravity
Davor Palle
Tidal torques. A critical review of some techniques
Michael Efroimsky, James G. Williams
Dynamics of a Spherical Accretion Shock with Neutrino Heating and Alpha-Particle Recombination
Rodrigo Fernández, Christopher Thompson
Asymptotically FRW black holes
J. T. Firouzjaee, Reza Mansouri
Reaction of Accretion Disks to Abrupt Mass Loss During Binary Black Hole Merger
Sean M. O'Neill, M. Coleman Miller, Tamara Bogdanovic et al.
A Gamma-Ray Burst/Pulsar for Cosmic-Ray Positrons with a Dark Matter-like Spectrum
Kunihito Ioka