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AntonioLao · **mad photons before nsyn -** 10-11-2007, 12:58 PM

The era of the angry mad photons is limited to within the first 3 minutes of the big bang. This period is also responsible for the first of two types of nucleosynthesis (nsyn): first is primordial and second is stellar. Although stellar nsyn is still taking place as we speak in the interior of stars, primordial nsyn happened only once. The fusion products are the observed cosmic abundances of simple nuclei no heavier than the first 4 elements of the periodic table: hydrogen, helium, lithium, and beryllium with respective atomic number of 1, 2, 3, and 4. Primordial nsyn rejected all fusion products with atomic numbers of 5 and above. Subsequently these are synthesized by stellar nsyn when stars were born.

Before the nsyn era the temperature is above 1 billion Kelvins and the age of the universe is less than 3 minutes. This is the era of mad photons each with an average kinetic energy of 1 ten billionth of a joule. By a cosmic coincidence this is also the relativistic energy needed for the creation of a proton. Therefore, two mad photons each with higher energy going at each other’s throat will annihilate and produce a proton-antiproton pair. But the proton are favored to survive thus the universe becomes dominated by matter not antimatter.

This process is based on the validity of QED’s pair production and annihilation. On the other hand, by QCD, proton is made of 2 up quarks and 1 down quark. Therefore, there must a fundamental connection between photon and quark which is really a boson-fermion connection rather than boson-boson or fermion-fermion. The lingering question is where are the mad angry quarks before nsyn?

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AntonioLao Raider of the lost time Status: Offline Posts: 5,274 Thanks Given: 714 Thanked 121x in 119 Posts Join Date: Nov 2003 Rep Power: 73	mad photons before nsyn - 10-11-2007, 12:58 PM The era of the angry mad photons is limited to within the first 3 minutes of the big bang. This period is also responsible for the first of two types of nucleosynthesis (nsyn): first is primordial and second is stellar. Although stellar nsyn is still taking place as we speak in the interior of stars, primordial nsyn happened only once. The fusion products are the observed cosmic abundances of simple nuclei no heavier than the first 4 elements of the periodic table: hydrogen, helium, lithium, and beryllium with respective atomic number of 1, 2, 3, and 4. Primordial nsyn rejected all fusion products with atomic numbers of 5 and above. Subsequently these are synthesized by stellar nsyn when stars were born. Before the nsyn era the temperature is above 1 billion Kelvins and the age of the universe is less than 3 minutes. This is the era of mad photons each with an average kinetic energy of 1 ten billionth of a joule. By a cosmic coincidence this is also the relativistic energy needed for the creation of a proton. Therefore, two mad photons each with higher energy going at each other’s throat will annihilate and produce a proton-antiproton pair. But the proton are favored to survive thus the universe becomes dominated by matter not antimatter. This process is based on the validity of QED’s pair production and annihilation. On the other hand, by QCD, proton is made of 2 up quarks and 1 down quark. Therefore, there must a fundamental connection between photon and quark which is really a boson-fermion connection rather than boson-boson or fermion-fermion. The lingering question is where are the mad angry quarks before nsyn? Time independence: [∂E(g)]²=[∂F(a)×∂r(a)]·[∂F(b)×∂r(b)] and Mass independence: ¶a(t)·¶r(t)=c²