The Approach of
The Approach of
The Approach of
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Collaborators and some publications Introduction Action <strong>of</strong> the <strong>Approach</strong> Yukawa couplings and scalar fields <strong>The</strong> spinor represent<br />
Dynamics <strong>of</strong> baryons<br />
<strong>The</strong> flux per unit time and unit surface <strong>of</strong> our Dark matter<br />
clusters hitting the Earth:<br />
Φ dm = ∑ i<br />
|⃗v dm i − ⃗v E | is ≈ equal to<br />
ρ dmi<br />
m c5<br />
Φ dm ≈ ∑ i<br />
ρ dmi<br />
⃗v dmi − ⃗v S<br />
{|⃗v dm i − ⃗v S | − ⃗v ES ·<br />
m c5 |⃗v dmi − ⃗v S | }.<br />
We assume ∑ i<br />
| v dmi ⃗ − ⃗v S | ρ dmi = ε vdmS ε ρ v S ρ 0 , and<br />
correspondingly<br />
∑<br />
i<br />
⃗v ES · ⃗v dmi −⃗v S<br />
|⃗v dmi −⃗v S | = v ESε vdmES cos θ sin ωt, with ω for our<br />
Earth rotation around our Sun.<br />
We evaluate 1 3 < ε v dmS<br />
< 3 and 1 3 < εv dmS<br />
ε vdmES<br />
< 3.<br />
N.S. Mankoč Borštnik, Cape Town 2010, 01-06 February University <strong>of</strong> Ljubljana<br />
<strong>The</strong> <strong>Approach</strong> Unifying spins and charges