ar X iv : h ep - p h / 00 09 09 2 v 1 7 S ep 2 00 0 1 Status of the solutions to neutrino

ar X iv : h ep - p h / 06 09 07 7 v 1 7 S ep 2 00 6 Hadron multiplicities in e + e − annihilation with heavy primary quarks

ar X iv : h ep - p h / 00 09 23 7 v 1 2 0 Se p 20 00 “ Bottom - up ” thermalization in heavy ion collisions

We describe how thermalization occurs in heavy ion collisions in the framework of perturbative QCD. When the saturation scale Q s is large compared to Λ QCD , thermalization takes place during a time of order α −13/5 Q −1 s and the maximal temperature achieved is α 2/5 Q s .

ar X iv : h ep - p h / 01 09 01 7 v 1 3 S ep 2 00 1

The global data on solar neutrino rates and spectrum, including the SNO charged current rate, can be explained by LMA, LOW or the energy independent solution – corresponding to near-maximal mixing. All the three favour a mild upward renormalisation of the Cl rate. A mild downward shift of the B neutrino flux is favoured by the energy independent and to a lesser extent the LOW solution, but not ...

ar X iv : h ep - p h / 02 07 09 7 v 1 6 J ul 2 00 2 Remarks on the compactified six - dimensional model of a particle

Non-homogeneous gauge ground state solutions in a six-dimensional gauge model in the presence of non-zero extended fermionic charge density fluctuations are reviewed and fully reinterpreted.

ar X iv : h ep - p h / 00 09 23 7 v 2 2 1 Se p 20 00 “ Bottom - up ” thermalization in heavy ion collisions

We describe how thermalization occurs in heavy ion collisions in the framework of perturbative QCD. When the saturation scale Q s is large compared to Λ QCD , thermalization takes place during a time of order α −13/5 Q −1 s and the maximal temperature achieved is α 2/5 Q s .