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Inflation in Early Universe: Experimental String Phenomenology

The data strongly supports the universe's inflation at a very early time, detailing supersymmetric particles' production and experimental studies from LEP and Fermilab. Particle Data Group confirms proton decay with a lifetime of around 10^33 years. Different string types like I, IIA, and IIB are explored along with brane configurations like E8 x E8 and 11-dimensional branes. Explore Kaluza-Klein vacuum decay and potential metastable states in this comprehensive study.

vladimir-dejesus
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Inflation in Early Universe: Experimental String Phenomenology

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  1. C:\papers\stringphenomenology.html

  2. The data strongly supports the idea that the universe underwent a period of ``inflation" at some very early time (t » 10-36 sec).

  3. g H

  4. g,Z e+ ~ m ~ m e- Production of supersymmetric particles

  5. Detailed experimentalStudies from LEP,Fermilab From Particle Data Group

  6. Signature: Proton Decay Signature: Proton Decay Lifetime » 1033 years Lifetime of order current experimental Limit (1033 years)

  7. Closed String Open String

  8. Type I IIA O(32) IIB 11-d E8 x E8

  9. S1 M4 x

  10. X

  11. Standard Brane Hidden Brane g Gmn q g

  12. V(R) ? R

  13. Decay of Kaluza-Klein Vacuum – to nothing

  14. e m

  15. V | f E 101000 metastable states?

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