a distance, side length,

b side-length of a tetrahedron

c speed of light in the vacuum

d_E diameter of the earth

d_e diameter of the electron

d_S diameter of the sun

E energy

E_l energy of the arriving radiation

radiation power coming from the earth

radiation power arriving at the electron

radiation power offered the electron

radiation power effective at the electron

radiation power coming from the earth and being effective at the electron

f distance between two particles with a determined direction

g factor of components

H constant of Hubble

h constant of Planck

impulse of the arriving radiation

change of impulse of the arriving radiation

k constant of Boltzmann

L length of the suporrting structure between the nucleus and the 3 K-space

m₁ mass 1; the mass of the electron

m₂ mass 2; the mass of the earth

rest mass of the arriving radiation

m_e⁰  rest mass of the electron

N number

N_l number of l-groups

N_lp number of l-groups of the proton

N_le number of l_e-groups

number of  l_e-groups for one direction

N_S number of sunlight-particles

number of sunlight-particles on the surface of the sun with in a volumen of 1m³.

N_P number of particles concerned on building of the proton

N_photon number of photons

number of particles in a volumen of 1 m³

n number of photons; counter of the number of d_S

p_f probability for the particles to have determined directions in the distance f

p_3er probability for a 3 particle collision

p _particle1 probability, that the direction and the distance is right for particle 1

p _particle2 probability, that the direction and the distance is right for particle 2

p _particle3 probability, that the direction and the distance is right for particle 3

p _destruction probability for a destruction

R₀ radius of the earth

r distance, distance to the sun, distance between mass`

T absolute temperature

T8 particle with the starting number 8

T_S temperature on the surface of the sun

a angle of deflection of the star-light caused by the sun

a_Dn angle of deflection of a distance Dn*d_s covered from a star-light-particle

angle of deflection caused by one sun-light-particle

angle of deflection caused by one sun-light-particle

on passing a distance of 1m

angle of deflection in degree per 1m of running-lenght of the star-light

g constant of gravitation

D difference

Dl difference between two wave-lenght`