in higher dimensional spacetimes

More documents

Recommendations

Info

Numerical Setupuse Sperhake’s extended Lean code (Sperhake ’07, Zilhão et al ’10)3+1 Einstein equations with scalar fieldBaumgarte-Shapiro-Shibata-Nakamura formulation with moving punctureapproachdynamical variables: χ, ˜γ ij , K, Ã ij , ˜Γ i , ζ, K ζmodified puncture gaugeBrill-Lindquist type initial data∂ tα = β k ∂ k α − 2α(η K K + η Kζ K ζ )∂ tβ i = β k ∂ k β i − η β β i + η Γ˜Γ i D − 4− η λ ˜γ ij ∂ j ζ2ζψ = 1 + r D−3 D−3S,1/4r1 + r D−3S,2measure lengths in terms of r S withr D−3 16πS=M(D − 2)A SD−2D−3/4r2H. Witek (CENTRA / IST) 12 / 23
Unequal mass head-onin D = 5 dimensionsPhys. Rev. D 83, 2011H. Witek (CENTRA / IST) 13 / 23
Page 1 and 2: Black hole collisionsin higher dime
Page 3: High Energy Collision of Particlesa
Page 6 and 7: Life cycle of Mini Black Holes1 For
Page 8 and 9: Numerical Relativity in D Dimension
Page 10 and 11: Formulation of EEs as Cauchy Proble
Page 14 and 15: Unequal mass head-on in D = 5Modes
Page 16 and 17: Equal mass head-onin D = 4, 5, 6 di
Page 18 and 19: Head-on collisionsof boosted black
Page 20 and 21: Initial data for boosted BHs in D >
Page 23: Thank you!http://blackholes.ist.utl

in higher dimensional spacetimes

You also want an ePaper? Increase the reach of your titles

Delete template?

Save as template?