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on the light front Sergei Alexandrov Laboratoire Charles Coulomb - PowerPoint PPT Presentation

First order gravity on the light front Sergei Alexandrov Laboratoire Charles Coulomb Montpellier work in progress with Simone Speziale Light Front Light cone coordinates: Light Front Light cone coordinates: Main features: Triviality


  1. First order gravity on the light front Sergei Alexandrov Laboratoire Charles Coulomb Montpellier work in progress with Simone Speziale

  2. Light Front Light cone coordinates:

  3. Light Front Light cone coordinates: Main features: • Triviality of the vacuum – energy – momentum

  4. Light Front Light cone coordinates: Main features: • Triviality of the vacuum – energy – momentum • Non-trivial physics of zero modes

  5. Light Front Light cone coordinates: Main features: • Triviality of the vacuum – energy – momentum • Non-trivial physics of zero modes • Importance of boundary conditions at

  6. Light Front Light cone coordinates: Main features: • Triviality of the vacuum – energy – momentum • Non-trivial physics of zero modes • Importance of boundary conditions at • Presence of second class constraints linear in velocities

  7. Gravity on the light front Null surfaces are natural in gravity (Penrose,…) null vectors • Sachs(1962) – constraint free formulation • conformal metrics on • intrinsic geometry of • extrinsic curvature of null foliation • Reisenberger – symplectic structure on the constraint free data

  8. Gravity on the light front Null surfaces are natural in gravity (Penrose,…) null vectors • Sachs(1962) – constraint free formulation • conformal metrics on • intrinsic geometry of • extrinsic curvature of null foliation • Reisenberger – symplectic structure on the constraint free data • Torre(1986) – canonical formulation in the metric formalism • Goldberg,Robinson,Soteriou(1991) – canonical formulation Constraint in the complex Ashtekar variables algebra • Inverno,Vickers(1991) – canonical formulation in the complex becomes a Lie algebra Ashtekar variables adapted to the double null foliation

  9. Gravity on the light front Null surfaces are natural in gravity (Penrose,…) null vectors • Sachs(1962) – constraint free formulation • conformal metrics on • intrinsic geometry of • extrinsic curvature of null foliation • Reisenberger – symplectic structure on the constraint free data • Torre(1986) – canonical formulation in the metric formalism • Goldberg,Robinson,Soteriou(1991) – canonical formulation Constraint in the complex Ashtekar variables algebra • Inverno,Vickers(1991) – canonical formulation in the complex becomes a Lie algebra Ashtekar variables adapted to the double null foliation • Veneziano et al. (recent) – light-cone averaging in cosmology

  10. Motivation Can the light front formulation be useful in quantum gravity (black holes, spin foams…)?

  11. Motivation Can the light front formulation be useful in quantum gravity (black holes, spin foams…)? • One needs the real first order formulation – was not analyzed yet on the light front

  12. Motivation Can the light front formulation be useful in quantum gravity (black holes, spin foams…)? • One needs the real first order formulation – was not analyzed yet on the light front • Can one find constraint free data in the first order formulation? (preferably without using double null foliation) Exact path integral (still to be defined)

  13. Motivation Can the light front formulation be useful in quantum gravity (black holes, spin foams…)? • One needs the real first order formulation – was not analyzed yet on the light front • Can one find constraint free data in the first order formulation? (preferably without using double null foliation) Exact path integral (still to be defined) • The issue of zero modes in gravity was not studied yet

  14. Motivation Can the light front formulation be useful in quantum gravity (black holes, spin foams…)? • One needs the real first order formulation – was not analyzed yet on the light front • Can one find constraint free data in the first order formulation? (preferably without using double null foliation) Exact path integral (still to be defined) • The issue of zero modes in gravity was not studied yet • In the first order formalism the null condition can be controlled by fields in the tangent space

  15. Technical motivation 3+1 decomposition of the tetrad Used in various approaches to quantum gravity (covariant LQG, spin foams…)

  16. Technical motivation 3+1 decomposition of the tetrad shift lapse spatial metric Used in various approaches to quantum gravity (covariant LQG, spin foams…)

  17. Technical motivation 3+1 decomposition of the tetrad shift lapse spatial metric Used in various approaches to determines the nature of the foliation quantum gravity (covariant LQG, spin foams…) spacelike spacelike lightlike timelike

  18. Technical motivation 3+1 decomposition of the tetrad shift lapse spatial metric Used in various approaches to determines the nature of the foliation quantum gravity (covariant LQG, spin foams…) spacelike spacelike lightlike timelike What happens at ? light front formulation

  19. Technical motivation 3+1 decomposition of the tetrad shift lapse spatial metric Used in various approaches to determines the nature of the foliation quantum gravity (covariant LQG, spin foams…) spacelike spacelike lightlike timelike What happens at ? light front formulation Perform canonical analysis for the real first order formulation of general relativity on a lightlike foliation

  20. Plan of the talk 1. Canonical formulation of field theories on the light front 2. A review of the canonical structure of first order gravity 3. Canonical analysis of first order gravity on the light front 4. The issue of zero modes

  21. Massless scalar field in 2d Solution:

  22. Massless scalar field in 2d Solution: Light front formulation Primary constraint Hamiltonian

  23. Massless scalar field in 2d Solution: Light front formulation Primary constraint Hamiltonian is of second class Stability condition:

  24. Massless scalar field in 2d Solution: Light front formulation Primary constraint Hamiltonian is of second class Stability condition: first class Identification: zero mode

  25. Massless scalar field in 2d Solution: Light front formulation Primary constraint Hamiltonian is of second class Stability condition: first class Identification: zero mode • the phase space is one-dimensional Conclusions: • the lost dimension is encoded in the Lagrange multiplier

  26. Massive theories One generates the same constraint but different Hamiltonian

  27. Massive theories One generates the same constraint but different Hamiltonian inhomogeneous Stability equation condition:

  28. Massive theories One generates the same constraint but different Hamiltonian inhomogeneous Stability equation condition: The existence of the zero mode contradicts to the natural boundary conditions

  29. Massive theories One generates the same constraint but different Hamiltonian inhomogeneous Stability equation condition: The existence of the zero mode contradicts to the natural boundary conditions In massive theories the light front constraints do not have first class zero modes

  30. Massive theories One generates the same constraint but different Hamiltonian inhomogeneous Stability equation condition: The existence of the zero mode contradicts to the natural boundary conditions In massive theories the light front constraints do not have first class zero modes In higher dimensions: behave like massive 2d case

  31. Dimensionality of the phase space On the light front dim. phase space = num. of deg. of freedom

  32. Dimensionality of the phase space On the light front dim. phase space = num. of deg. of freedom Fourier decompositions

  33. Dimensionality of the phase space On the light front dim. phase space = num. of deg. of freedom Fourier decompositions Symplectic structure is non-degenerate Dirac bracket Second class constraint

  34. First order gravity (spacelike case) Canonical variables: – normal to the foliation Fix

  35. First order gravity (spacelike case) Canonical variables: – normal to the foliation Fix Linear simplicity constraints

  36. First order gravity (spacelike case) Canonical variables: – normal to the foliation Fix Linear simplicity constraints Hamiltonian is a linear combination of constraints

  37. First order gravity (spacelike case) Canonical variables: – normal to the foliation Fix Linear simplicity constraints Hamiltonian is a linear combination of constraints 3 6

  38. First order gravity (spacelike case) Canonical variables: – normal to the foliation Fix Linear simplicity constraints Hamiltonian is a linear combination of constraints 3 6 secondary constraints

  39. First order gravity (spacelike case) Canonical variables: – normal to the foliation Fix Linear simplicity constraints Hamiltonian is a linear combination of constraints 3 1st class 6 2d class secondary constraints

  40. First order gravity (spacelike case) Canonical variables: – normal to the foliation Fix Linear simplicity constraints Hamiltonian is a linear combination of constraints 3 1st class 6 2d class secondary constraints dim. of phase space = 2 × 18 – 2(3+3+1)-(3+9+6)=4

  41. Cartan equations Cartan equations

  42. Cartan equations Cartan equations do not contain time derivatives and Lagrange multipliers 12 constraints

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