twistorial structure of loop quantum gravity transition...

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Twistorial structure of loop quantum gravity transition amplitudes Simone Speziale Centre de Physique Theorique de Luminy, Marseille, France ILQG 13-11-2012 mainly based on work with Wolfgang Wieland 1207.6348

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Twistorial structure of loop quantum gravity transition amplitudes

Simone Speziale

Centre de Physique Theorique de Luminy, Marseille, France

ILQG 13-11-2012mainly based on work with Wolfgang Wieland 1207.6348

Outline and goals

Classical Theory

‚ Description of the covariant phase space in terms of twistorsalgebra of the area matching and simplicity constraints

‚ Smearing the connection-tetrad algebra to the holonomy-flux algebra before or aftersolving the simplicity constraints is equivalent: T˚SUp2q with AB holonomy

‚ Notion of simple twistors solving the simplicity constraints

Quantum theory

‚ Hilbert space represented via homogeneous functions on spinor space(instead of cylindrical functions)

‚ Dynamics as integrals in twistor space

‚ Embedding of the Regge data of the EPRL asymptotics in the initial phase space

Work and ideas shared with a number of collaboratorsL. Freidel, E. Livine, W. Wieland, B. Dittrich, C. Rovelli, M. Dupuis, J. Tambornino, . . .

This talk: w Wolfgang Wieland 1207.6348 PRD12 w Miklos Langvik (to appear)

Speziale — Twistors and LQG 2/24

Smearing and simplicity constraints

Phase spaces:

SmearingSLp2,Cq variables ùñ T˚SLp2,Cq

ó Solve simplicity constraints ó

(primary and secondary)

Ashtekar-Barbero variables ùñ T˚SUp2q

Does the diagram commute?

LQG path: ë spin foam path: the other one

In the continuum:

‚ primary: simple bivectors, unique metric structure

‚ secondary: embedding of AB variables in covariant phase space: Γ “ ΓpEq

In the discrete:

‚ primary: simple twistors, unique (twisted) geometry

‚ secondary: non-trivial embedding of T˚SUp2q in T˚SLp2,Cq. Discrete ΓpEq ?

Speziale — Twistors and LQG 3/24

Smearing and simplicity constraints

Phase spaces:

SmearingSLp2,Cq variables ùñ T˚SLp2,Cq

ó Solve simplicity constraints ó

(primary and secondary)

Ashtekar-Barbero variables ùñ T˚SUp2q

Strategy: do symplectic reduction of the primary constraints, and think of thesecondary constraints as providing a non trivial gauge-fixing section.

ñ allows to show commutativity of the procedure, while postponingknowning explicitly the form and solution of the secondary constraints

Technique: twistorial tools: parametrize the phase spaces and the constraints interms of twistors

ñ allows to embed the non-linear HF phase space into a linear one,explicit calculations, plus direct link with variables used in the twistedgeometry parametrization

Speziale — Twistors and LQG 4/24

Panorama

twistors Ñ covariant ðñ covariantC-area matching twisted geometry loop gravity

SLp2,CqÓ simplicity constraints Ó Ó

SU(2) spinors Ñ “open” twisted geometry ðñ loop gravityarea matching SUp2q

Ó closure Ó Gauss law

“closed” twisted geometries ðñ gauge-inv.(polyhedra) loop gravity

Ó shape matching

Regge calculus

Speziale — Twistors and LQG 5/24

LQG and twisted geometries

On a fixed graph HΓ “ L2rSUp2qLs PΓ “ T˚SUp2qL

represents a truncation of the theory to a finite number of degrees of freedom w Rovelli, PRD 10

These can be interpreted as discrete geometries, called twisted geometries w Freidel, PRD 10, . . .

X, gùñ

Npζq, j, ξ, Npζq

hol-flux area-angles

Each classical holonomy-flux configuration on a fixed graph can be visualized as acollection of adjacent polyhedra with extrinsic curvature between them

‚ Each polyhedron is locally flat: curvature emerges at the hinges, as in Regge calculus

‚ They induce a discontinuous discrete metric: two neighbouring polyhedra areattached by faces with same area but different shape

‚ ξ: extrinsic geometry

‚ Realizes a link suggested by Immirzi, Smolin et al., with the subtlelty of discontinuity: Reggecalculus is too “rigid” to capture the kinematical degrees of freedom of a spin network

‚ The matching with Regge geometries becomes exact in 2+1 dimensions

The picture can be embedded in a SLp2,Cq formalism described by simple twistors

Speziale — Twistors and LQG 6/24

Twistors

‚ A pair of spinors, ω and π, chiral under Lorentz transformations,

Z “

ˆ

ωA

π 9A

˙

P T :“ C2ˆ C2˚

Twistor “complex helicity”: πAωA“ rπ|ωy SLp2,Cq-invariant

Twistor norm (helicity) s :“ Im`

rπ|ωy˘

SUp2, 2q invariant

‚ physical picture as a massless particle with a certain spin and momentum

‚ geometric picture via incidence relation ωA “ iXA 9Aπ 9A§ X a light ray in Minkowski space for a null twistor s “ 0§ X a congruence of light rays for a generic twistor

‚ can provide notion of non-linear graviton

We will see that twistors can be thought of as non-linear gravitons in a completelydifferent way than Penrose’s original one, as classical counterparts of LQG’s quantumgeometry

Speziale — Twistors and LQG 7/24

Representation of the Lorentz algebra

‚ C2 carries a representation of the Lorentz algebra (the celestial sphere)

‚ Similarly, there is a representation of the Lorentz algebra on twistor space T

ΠAB“

1

2pL` iKqAB “

1

2ωpAπBq

‚ We are interested in a representation of a larger Poissonian algebra, the one ofT˚SLp2,Cq: the holonomy-flux algebra of (covariant) loop quantum gravity

‚ This can be achieved on T2Q pZ, Zq,

ΠAB“

1

2ωpAπBq, ΠAB

“1

2ωpAπBq, hAB “

ωAπB ´ πAωB

?πω?πω

imposing a complex first-class constraint called complex area matching

C “ rπ|ωy ´ rπ|ωy “ 0,

C8{{C – T˚SLp2,Cq

That is, both Lorentz generators and holonomies can be expressed as simple functions ona space of two twistors, provided they have the same complex helicity

Speziale — Twistors and LQG 8/24

Twistor Poisson brackets

The symplectic structure simplifies in the larger space T2:

T2 C “ 0 T˚SLp2,CqtωA, ωBu “ 0 th, hu “ 0tπA, ω

Bu “ δBA ùñ tΠi, hu “ τ ih

tπA, πBu “ 0 tΠi,Πju “ εijkΠk

In particular, momenta commute.

16 twistors T2 Ñ T˚SLp2,Cq 12C-area matching C

Ó simplicity constraints Ó

8 simple twistors Ñ T˚SUp2q 6SU(2) spinors area matching C

Note: the complete system of constraints is reducible

Speziale — Twistors and LQG 9/24

Simplicity constraints

Gauge-fixed approach Pick a time direction nI (typically time gauge, nI “ p1, 0, 0, 0q)(cfr. with gauge-invariant approach e.g. Bianca and Jimmy)

‚ Allows to define SU(2) norm }ω}2 :“ δA 9AωAω

9A and xω|πy :“ δA 9Aω9AπA

‚ Primary simplicity constraints: matching of left and right geometries

K ` γL “ 0 ô Π “ eiθΠ, γ “ cotθ

2

and the same for tilded variables: Π “ eiθ ¯Π

‚ In terms of spinors:`

rπ|ωy “ R` iI˘

F1 “ R´ γI “ 0, F2 “ xω|πy “ 0, F2 “ 0

‚ On each link, pM,Fi, Fiq form a second class system: tF2, F2u ff 0which is further reducible: M and F1 imply F1.

3 indep. 1st class constraints`

C,D :“ F1 ` F1

˘

aut`

Cred P R, F1, F1

˘

4 2st class constraints F2, F2

Speziale — Twistors and LQG 10/24

Counting

3 indep. 1st class constraints`

C,D :“ F1 ` F1

˘

aut`

Cred P R, F1, F1

˘

4 2st class constraints F2, F2

16 twistors T2 Ñ T˚SLp2,Cq 12C-area matching C

Ó simplicity constraints Ó

8 simple twistors Ñ T˚SUp2q 6SU(2) spinors area matching C

Counting:

Right-Down: T2 C T˚SLp2,Cq D,F2, F2 T˚SUp2q

16 -2x2 12 -1x2-4 6

Down-Right: T2 F C4 Cred T˚SUp2q

16 -2x2-4 8 -1x2 6

Speziale — Twistors and LQG 11/24

Solution of the simplicity constraints

Focus first on half-link: pω, πq,`

F1 “ R´ γI, F2 “ xω|πy˘

‚ F1 “ 0 ñ rπ|ωy “ pγ ` iqj, j P R

‚ orbits: tF1, }ω}u “1

1`γ2 }ω}

‚ convenient to introduce a F1-gauge-invariant spinor

zA “?

2JωA

}ω}iγ`1, }z} :“

?2J, tF1, z

Au “ 0

constraint surface orbitspωA, πAq ÝÑ pωA, jq ÝÑ zA

Fi “ 0 }ω}

Symplectic reduction: C4{{F – C2

‚ Solutions parametrized by a SU(2) spinor zA

(transforms linearly under rotations but not under boosts)

‚ Simple twistors (on the 5d constraint surface): Z “ pωA, jq “ pzA, }ω}q

Speziale — Twistors and LQG 12/24

Area matching and T ˚SUp2q

On the link:16 pωA, πA, ωA, πAq P T2 Ñ pΠ, hq 12

C-area matching C

Ó simplicity constraints Ó

8 pzA, zAq P C4 Ñ pX, gq 6area matching Cred

Cred “ }z} ´ }z} C4{{Cred “ T˚SUp2q Q pX, gq Freidel PRD10

Symplectic reduction by the linear primary simplicity constraints selects an SUp2qholonomy-flux algebra from the covariant SLp2,Cq one

‚ Flux: X “ L “ ´K{γ‚ Holonomy X Ø h „ AγAB Ø A

Recall that Π “ ´hΠh´1. From this plus Fi “ Fi “ 0, it follows that

ph:hqABωB “ e´ΞωA, ph:hqABπ

B “ eΞπA

Using this one proves that the reduced g is the holonomy of the Ashtekar-Barberoconnection, a non-trivial and γ-dependent mixing of real and imaginary parts oflnh “ Γ` iK:

g „ eRe lnheγIm lnh ` opΞq

Speziale — Twistors and LQG 13/24

Geometric interpretation

Properties of the reduction:

‚ On C “ 0 surface, 1st class diagonal simplicity constraint D “ F1 ` F1

‚ Each orbit of D spanned by

Ξ :“ 2 ln

ˆ

}ω}

}ω}

˙

‚ In the time gauge,nIΛphq

IJnJ “ ´ cosh Ξ

The dihedral angle parametrizes the orbits of the diagonal simplicity constraint

‚ Symplectic reduction eliminates the dependence on Ξ, which is the coordinate of theorbits of the diagonal simplicity constraint D

‚ Secondary constraints: provide a non-trivial gauge-fixing of the orbits and thusnon-trivial embedding of T˚SUp2q in T˚SLp2,Cq, precisely as in the continuum

Speziale — Twistors and LQG 14/24

Geometric interpretation: covariant twisted geometries

‚ gauge-fixed approach pick a time direction nI (typically nI “ p1, 0, 0, 0q)

nIΛphqIJnJ “ ´ cosh Ξ, Ξ :“ 2 ln

ˆ

}ω}

}ω}

˙

pΠ, hq ÞÑ´

rπ|ωy, ζ, ζ, α, α, ξ,Ξ¯

given by

ζ “ ´ω1

ω0, α “

e2i argpω0q

rπ|ωyF2, ξ :“ 2 argpω0

q ´ 2 argpω0q ` γΞ.

reduction to twisted geometries:

Π “ ´ i2rπ|ωynpζqTατ3T

´1α n´1

pζq R´ γI “ α “ α “ 0 X “ jnpζqτ3n´1pζq

ÝÑ

h “ npζqTαep´ξ`pγ´iqΞqτ3T´1

α n´1pζq Ξ “ 0 g “ npζqe´ξτ3n´1

pζq

A “ Γ` iK “ AγAB ´ pγ ´ iqK

Speziale — Twistors and LQG 15/24

More on the brackets and the role of γ

Symplectic potential of T˚SLp2,Cq: pΠ, hq ÞÑ´

rπ|ωy “ R` iI, ζ, ζ, α, α, ξ,Ξ¯

Θ “ ´2Re´

TrrΠh´1dhs¯

“ pR´ γIqdΞ` Idξ ´iI

1` |ζ|2pζdζ ´ ζdζq ´

1

1` |ζ|2pαrπ|ωydζ ` αxω|πsdζq

´iI

1` |ζ|2pζd

¯ζ ´

¯ζdζq ´

1

1` |ζ|2prπ|ωyαd

¯ζ ` xω|πs ¯αdζq.

“Abelian” sector, described by the pR, I, ξ,Ξq, with Poisson brackets

tR,Ξu “ 1, tR, ξu “ γ, tI,Ξu “ 0, tI, ξu “ 1.

On the constraint surface, we recover the twisted geometry brackets, in particular

tj, ξu “ 1

where ξ :“ 2 argpω0q ´ 2 argpω0

q ` γΞ encodes the extrinsic curvature(But to be able to extract it I need to know explicitly the solution of the secondaryconstraints, i.e. the embedding in the covariant phase space)

Speziale — Twistors and LQG 16/24

Geometry of a simple twistor

‚ Incidence relation, ωA “ iXA 9Aπ 9A, X PM iff null twistor, s “ 0

‚ Simple twistors (Fi “ 0q:

ωA “1

rnA

9Aeiθ2 π 9A, r :“

ja

1` γ2

}ω}2

1. Not null, but isomorphic to null twistors:

Z ÞÑ Zγ “ pωA, eiθ{2π 9Aq, spZγq “ 0

Isomorphism depends on γ, reduces to the identity for γ “ 8

2. F2 “ xω|πy “ 0 aligns the spinors’ null poles to the time normal

`Ipωq `1

r2kIpπq “

?2}ω}2nI

A simple twistor is a γ-null twistor with a time-like direction picked up

The projective twistor space PN does not depend on the “scale” jwhereas it depends on |xω|πy|

Speziale — Twistors and LQG 17/24

Twistor networks

Zsl

Ztl

Zsm

Graph Γ decorated with a twistor on each half-link,

pT2qL{{CL – T˚SLp2,CqL

Quantization gives covariant spin networks ΨΓ,pρl,klq,In rGls,

with the covariant holonomy-flux algebra

‚ The standard Penrose interpretation is a collection of spinning massless particles

‚ A new interpretation in terms of geometries can be achieved thanks to thegauge-invariance at the nodes (Ψrh´1

splqGl htplqs “ ΨrGls):

ÿ

lPn

~JLl “ÿ

lPn

~JRl “ 0

Established in two steps:

1. each left- and right-handed sector defines a twisted geometry

2. simplicity constraints impose the matching between the two geometries

Speziale — Twistors and LQG 18/24

Further comments and questions

‚ Twistor space carries a representation of the larger group SU(2,2) of conformaltransformations of Minkowski: Non-trivial effect on a twisted geometry!See upcoming paper with Miklos Langvik

‚ Explicit form of the secondary constraints? Open problemAssume they correspond to a discretization of the continuum secondary constraints:

torsionlessness, Γ “ ΓpEq

Such a discrete Levi-Civita connection is well known in the context of Regge calculusCan it be constructed also without shape matching conditions? Yes!See brand new paper by Haggard-Rovelli-Vidotto-Wieland 1211.2166

‚ Open question: is there a consistent classical dynamics for twisted geometries, oronly for the subsector of Regge geometries?

‚ Does shape mismatch play a role in the dynamics?

‚ Can torsion be consistently encoded in ξ alone?

– end of classical part –

Speziale — Twistors and LQG 19/24

Quantization

Dirac quantization: first quantize auxiliary space, then impose constraints: simplicity onhalf-links, then area matching on full link

‚ Quantize initial twistorial phase space, a la Schrodinger:

πA, ωBs “ ´i~δBA , fpωq P L2

pC2, d4ωq´

ω “ ω, π “ ´i~ BBω

¯

ˆπA, ˆωB‰

“ i~δBA , fpπq

‚ Convenient basis homogeneous functions f pρ,kqpλωq “ λ´k´1`iρλk´1`iρf pρ,kqpωq(carry a unitary, infinite dimensional representation of the Lorentz group)

‚ Simplicity constraints

F1fpρ,kq

pωq “ 0 ñ ρ “ γk

M “ F2F2 Mf pρ,kqpωq “ 0 ñ k “ j

‚ Solution space fpγj,jqjm pωq “ }ω}2piγj´j´1q

xj,m|j, ωyPerelomov

(Not a function of the F1-reduced phase space, C2 Q zA. Half-density?d2ωf

pγj,jqjm is.)

‚ Area matching constraint´

Mfρ,k b f ρ,k¯

pω, πq “ 0 ñ pρ “ ρ, k “ kq

‚ Solution space Gpjqmmpω, πq :“ f

pγj,jqjm pωqf

pγj,jqjm pπq

Speziale — Twistors and LQG 20/24

From homogeneous functions to cylindrical functions

‚ Solution space Gpjqmmpω, πq :“ f

pγj,jqjm pωqf

pγj,jqjm pπq

(Morally Perelomov coherent states up to non-Lorentz-inv. norms }ω} and }π})

‚ carries a representation of the holonomy-flux algebra though harmonic oscillators§ Fluxes: Schwinger representation of SLp2,Cq§ Holonomy: ordering ambiguities, more natural operators twisted geometries ζ, ξ, etc.

‚ And the usual cylidrical functions? The relation is a kernel in twistor space:

@

Gpjqm,m

D

pgq :“ş

T2 dµpZ, Zq eiSBF pZ,Z,gqG

pjqm,mpω, πq “ µpjqD

pγj,jqjm jmpgq,

‚ It allows us to recover the EPRL model

Apgq “ÿ

j

µf pjqTrj

´

ź

wPf

Dpγj,jqpgwg´1w q

¯

, ZC “

ż

ź

v,τ

dgvτ

Speziale — Twistors and LQG 21/24

Dynamics as integrals in twistor space@

Gpjqm,m

D

pgq :“ş

T2 dµpZ, Zq eiSBF pZ,Z,gqG

pjqm,mpω, πq “ µpjqD

pβj,jqjm jmpgq,

Two ingredients:

1. Measureż

T2gf

dωA ^ dωA^ . . . δCpMq fpZ, Zq “

ż

T˚SLp2,Cqd3Π^ dHaarh^ c.c. fpΠ, hq

FP fixing of the complex area matching condition§ direct geometric proof of gauge-invariance§ Morally the same as the Gaussian version by Etera, Maite and Johannes

2. BF action in terms of spinors

SwrB,As “ ΠABrtwsh

BArBws ` c.c. “

`

gg´1˘A

BpωBπA ` π

BωAq ` c.c.

§ bilinear in the spinors§ mixes bulk and boundary elements

See paper for details of proof and explicit value of µpjq

Speziale — Twistors and LQG 22/24

What do we learn from this?@

Gpjqm,m

D

pgq :“ş

T2 dµpZ, Zq eiSBF pZ,Z,gqG

pjqm,mpω, πq “ µpjqD

pβj,jqjm jmpgq,

1. As a path integral in twistors, action gives trivial dynamics in phase space

@

Gpjqm,m

D

pgq “

ż

T2

dµpZ, Zq eiStotpZ,Z,gq

2. non-trivial dynamics emerges by an interplay between boundary phase spacevariables (the twistors) and bulk degrees of freedom (the bulk holonomies g)key “gluing” role played by saddle point conditions

3. 4-simplex asymptotics and Regge data: 3d dihedral angles fit in the phase space(the ζ’s), whereas areas j and extrinsic geometry ξ,Ξ are thrown away, butrecovered, in two different ways:

§ areas identified with quantum spins, and summed over in the definition of the model§ dihedral angles Ξ encoded in the bulk holonomies g which become the

Regge-Levi-Civita holonomies at the saddle point

4. Relaxing wedge flatness, we can define a curvature tensor and decompose it intoirreps: Weyl, Ricci and torsional parts

§ Still of Petrov type D, like in Regge calculus§ Additional torsional components carried by certain pieces of the holonomy identified

All of this points in the same direction: can we rewrite the model in a fully coherent way,where the phase space variables are treated on equal footing?Similar ideas have been expressed at length, Daniele, Etera, Maite, Valentin, Laurent, . . .

Speziale — Twistors and LQG 23/24

Conclusions and outlook

Can we express the dynamics as integrals over phase space? i.e.ř

j Ñş

djdξ(see Etera and Maite for an euclidean model of this)

in such a way that exponential of a suitable discretization of GR immediately emerges,not only at holonomy saddle point. This should be a discretization of GR:

1. in the first order formalism

2. without shape matching

Again, the key open question is the existence of a dynamics for twisted geometries

Remarks:

‚ A priori this is not necessary: correct semiclassical limit may also emerge from coarsegraining graphs, and not graph by graph But we need to find this out!

‚ Regardless, there should be many different discrete versions of GR, like there are ofgauge theories on a lattice. Why do we know only one version?

Longer term questions

‚ Can the formulation as integrals in twistor space improve explicit calculations?

‚ Any connections with twistors of the complete, infinitely-many-dofs LQG theory?

– finis terrae –

Speziale — Twistors and LQG 24/24