Higgs Phase of Gravity in String Theory - LUTh

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$J. Phys. A: Math. Gen. 32 (1999) - LUTH - Observatoire de Paris$

Cosmological Application (II) Alternative to DE/DM • For FRW universe, it behaves like c.c. + CDM. CDM Ghost condensation dS ( 2 ( ∂ ) ) P φ Λ=0 Λeff >0 CDM dS ( Φ) • Clustering properties remain unexplored and may be different from c.c. + CDM. V Usual Higgs mechanism Λ < 0 Λ < 0 eff Λ=0 eff Φ
Cosmic Uroboros String/M theory? Higgs phase DE/DM of gravity
Page 1 and 2: Higgs Phase of Gravity Shinji Mukoh
Page 3 and 4: Historical remark: Precession of pe
Page 5 and 6: Order Parameter Higgs Mechanism Gho
Page 7 and 8: Order Parameter Higgs Mechanism Gho
Page 9 and 10: Gauge choice: φ( t , x) = t. Resid
Page 11 and 12: ( ) ( ) 2 4⎧2α 1 2 Leff = LEH+ M
Page 13 and 14: Bounds on symmetry breaking scale M
Page 15 and 16: E dt dx → → → π → rE r r r
Page 17: 3-point function for ghost inflatio
Page 21 and 22: Correspondence principle Stringy Ob
Page 23 and 24: x i Spontaneous Lorentz breaking
Page 25 and 26: • The dispersion relation is simi
Page 27 and 28: Summary • Ghost condensation is t

Higgs Phase of Gravity in String Theory - LUTh

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