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Published byJewel Stevenson Modified over 9 years ago
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Conserved Quantities in General Relativity A story about asymptotic flatness
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Conserved quantities in physics Charge Mass Energy Momentum Parity Lepton Number
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Conserved quantities in physics Energy – Time translation Momentum – Linear translation Parity – Inversion Charge – Phase of the gauge field
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Measurement Direct – Scales, meter sticks Indirect – Fields due to the conserved quantity
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Measurement Direct Indirect – Fields due to the conserved quantity
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Extension to General Relativity Komar Mass, requires existence of Killing vector ADM Mass, h ab is the expansion of g ab around Minkowski
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Extension to General Relativity Komar Mass, requires existence of Killing vector ADM Mass, h ab is the expansion of g ab around Minkowski Small note: These definitions hold in an Asymptotically flat spacetime
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“Asymptotically Flat?” Intuitively,
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“Asymptotically Flat?” Intuitively, Problems: – Expansion might not be possible for a general metric – Exchanging limits and derivatives causes issues
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“Asymptotically Flat?” Better: Conformal mapping to put “infinity” in a finite place
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“Asymptotically Flat?” Better: Conformal mapping to put “infinity” in a finite place
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“Asymptotically Flat?” Einstein Universe – i 0 “spacelike infinity” R= , T=0 – i + “future timelike infinity” R=0, T= – “future null infinity” T= – R We’ve thus taken infinity and placed it in our extended spacetime
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“Asymptotically Flat?” Asymptotically simple: – (M,g ab ) is an open submanifold of (M,g ab ) with smooth boundary – There exists a smooth scalar field such that ( ) = 0 d ( ) not 0 g ab = 2 g ab – Every null geodesic in M begins and ends on – Asymptotically flat: Asymptotically simple R ab =0 in the neighbourhood of
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“Asymptotically Flat?” What is asymptotically flat: – Minkowski – Schwarzchild – Kerr What is not: – De Sitter universe (no matter, positive cosmological constant) – Schwarzschild-de Sitter lambdavacuum – Friedmann – Lemaître – Robertson – Walker Homogenous, isotropically expanding (or contracting)
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