Diffusion coefficients and constraints on hadronic inhomogeneities in the early universe
Abstract Hadronic inhomogeneities are formed after the quark hadron phase transition. The nature of the phase transition dictates the nature of the inhomogeneities formed. Recently some scenarios of inhomogeneities have been discussed where the strange quarks are in excess over the up and down quark...
Main Authors: | Sovan Sau, Sayantan Bhattacharya, Soma Sanyal |
---|---|
Format: | Article |
Language: | English |
Published: |
SpringerOpen
2019-05-01
|
Series: | European Physical Journal C: Particles and Fields |
Online Access: | http://link.springer.com/article/10.1140/epjc/s10052-019-6938-6 |
Similar Items
Calculating the inhomogeneous reionization of the universe
by: Razoumov, Alexei O.
Published: (2009)
by: Razoumov, Alexei O.
Published: (2009)
Similar Items
-
Decay of baryon inhomogeneities in an expanding universe
by: Pratik K. Das, et al.
Published: (2021-09-01) -
Neutrino currents in wakes of cosmic strings
by: Sovan Sau, et al.
Published: (2020-02-01) -
Reaction diffusion models with spatially inhomogeneous diffusion coefficients
by: Benson, Debbie Lisa
Published: (1994) -
The quark-hadron transition and hot hadronic matter in the early universe
by: Von Oertzen, Detlof Wilhelm
Published: (2015) -
Transport Coefficients of Interacting Hadrons
by: Wiranata, Anton
Published: (2011)