RELA TIVE LOCALITY IN 2+1 DIMENSIONS ESFQG SISSA, SEPTEMBER 2014 - - PowerPoint PPT Presentation

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RELA TIVE LOCALITY IN 2+1 DIMENSIONS ESFQG SISSA, SEPTEMBER 2014 1 THE PLAN 1. 1. Curved momentum spac ace an and relat ative local ality; 2. 2. Alekseev-Mal alkin kin construct ction on of f effect ctive, , deformed


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SLIDE 1

„RELA TIVE LOCALITY” IN 2+1

DIMENSIONS

ESFQG – SISSA, SEPTEMBER 2014

1

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SLIDE 2

THE PLAN

1. 1. Curved momentum spac ace an and relat ative local ality; 2. 2. Alekseev-Mal alkin kin construct ction

  • n of

f effect ctive, , deformed par articl cle lag agran angian an in 2+1 dimensions*; 3. 3. Comments ts.

2

* Based on the (partially inpublished) work done with T

  • masz Trześniewski.
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SLIDE 3

SCALE AND GEOMETRY

The assumpti mption n that t the angle sum m is less than n 180 80 leads s to a geome metr try y quite e different from Euclid’s. . It depe pends nds on

  • n a

constant, tant, which ch is not given n a pr priori.

  • ri. As

As a a joke I e even wishe hed d Euclide idean an geome metr try was not true, , for then we would d have an absolute te me measure ure of

  • f le

length h a pr priori

  • ri.

. (Gauss, s, 182 827) 7) 3 If there re is an a pr priori ri scale, , you expe pect nontri rivial al geome metr try. y.

Ever erything ything is curved, d, unless s it cannot b t be

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SLIDE 4

FLA T/CURVED MOMENTUM SPACE

In the case of a standar ard d relati tivisti istic c particle cle we have flat spacetime ime and flat momentum m sp space:

4

Spacetime Momentum space

The phase space is a a cotan tange gent nt bun undle over flat t momentum m space

No scale required

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SLIDE 5

FLA T/CURVED MOMENTUM SPACE

For deformed d relativistic istic particle icle we have flat spaceti time me and curved d momentum um sp space:

5

Spacetime Curved momentum space (the curvature scale needed!)

The phase space is a a cotan tange gent nt bundle over curved d momentum m space

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SLIDE 6

RELA TIVE LOCALITY

In the RL framework work the no-trivia ial geometr try y of momentum m space exhibits its itse self f in a num umber of f ways ys: 1. 1. The kinetic term for a particle icle has the form with the no nontrivial ial momentum m space frame e field.

6

~ ( ) , ( ) 1

a a a a a

L p E p x E p f p

      

        

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SLIDE 7

RELA TIVE LOCALITY

The mass-shell ll relation ion is defined d as a square of the distan ance from zero to the po point P, with coordin dinat ates pμ(P): We need metric c to d define the m mass-sh shell ll relation tion ! If f the metric is n s nonlinear ar we need the mass ss sc scale to defi fine it.

 

2 2

( ) ( ) C p D p m

  

 

2

( )

p geodesic

D p ds g p p

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SLIDE 8

MOMENTUM ADDITION

In order r to add two momenta ta the notion of connecti tion

  • n (paralle

lel transpor port) ) is ne needed. d. If the c composition sition pq is nonlinear ar we need a mass scale to define it.

8

p q pq

) 1 ( q p q p p q

      

       

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SLIDE 9

RELA TIVE LOCALITY

In theories with curved d momentum m space, , localit lity y might be relative: e: 1. 1. The transl slati ation

  • n (and/or
  • r Lorentz

z transf sforma

  • rmation

ion) ) of f a particle icle wordline dline depends s on the momentum um that the particl icle e carrie ries; 2. 2. Therefore

  • re the worldline

dlines of the particle cles with differe rent t momenta ta transform

  • rm differently

tly; 3. 3. As a result, locali ality of events (defined d by worldl ldline ines intersecti tion

  • ns)

) is not absolut lute, e, and become

  • mes

s relative.

It seems ms that relati ative localit lity y is neither her logical ally ly inconsist sistent nt nor does it contrad adict t any observat atio ional nal data. 9

  • G. Amelino-Camelia, L. Freidel, JKG, L. Smolin The principl

iple e of relati tive e localit

  • ity. Phys.Rev. D84 084010, arXiv:1101.0931 [hep-th];

Relati tive e localit ity: y: A deepenin ing g of the relati tivit ity y principl

  • iple. Gen.Rel.Grav. 43

43 2547arXiv:1106.0313 [hep-th]

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SLIDE 10

FUNDAMENTAL OR EMERGENT?

Is the curved d momentum m space fundame mental tal or emergent? 1. 1. If f it is s fun undame mental, tal, what is s the ass ssocia iated d dyn ynamic ics? s? 2. 2. If it is is emergent nt, , how does it arise? In the emergent t case the master r theory must provide ide a momentum m scale. In 3+1 3+1D D One can imagi gine the re regime me, , in wh which Planck length is small, l, while Planck k mass stays finite (relat lative to the charact acterist eristic ic scales of the pr proble blem) m)

10 10

4 Pl Pl

l G M

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SLIDE 11

IN 2+1 D THERE IS A MASS SCALE!

In 2+1 dimensions the Newton’s constant G3 has the dimension ion of inverse mass G3=1/ 1/κ. This suggests s that the momentum um space might t be curved, d, and I wi will show that it indeed d is. s. Of course, , 2+1D gravity is a a toy model, l, and we do not have to believe that it tells you anything ing relevant ant for the real world. d. However, r, it is in interesting ng becau ause: 1. 1. This s is s the only y example mple that we have; 2. 2. There might be real physical al systems, which are effectively ly 2+1 dimensional ional.

11 11

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SLIDE 12

GRAVITY IN 2+1 D WITH PARTICLES

The Lagrangian angian of 2+1 grav avit ity with one (massive) ) particle icle at at the origin in is is

12 12

2 1 2 1 2

1 2 ( ) F 2

ij i j ij ij

L d x A A d h hC k d x A hCh x    

 

         

  

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SLIDE 13

GRAVITY IN 2+1 D WITH PARTICLES

The Lagrangian angian of 2+1 grav avit ity with one (massive) ) particle icle at at the origin in is is

13 13

2 1 2 1 2

1 2 ( ) F 2

ij i j ij ij

L d x A A d h hC k d x A hCh x    

 

         

  

Kinetic term

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SLIDE 14

GRAVITY IN 2+1 D WITH PARTICLES

The Lagrangian angian of 2+1 grav avit ity with one (massive) ) particle icle at at the origin in is is

14 14

2 1 2 1 2

1 2 ( ) F 2

ij i j ij ij

L d x A A d h hC k d x A hCh x    

 

         

  

Kinetic term Particle term

is ' , ' translation C m Lorentz J sP h   

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SLIDE 15

GRAVITY IN 2+1 D WITH PARTICLES

The Lagrangian angian of 2+1 grav avit ity with one (massive) ) particle icle at at the origin in is is

15 15

2 1 2 1 2

1 2 1 ( )

ij i j ij ij

L d x A A h hC d x A F hCh x   

 

         

 

Kinetic term Particle term Constraint: curvature is nonzero only at the position of the particle

Poincare group C mJ P h s   

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SLIDE 16

GRAVITY IN 2+1 D WITH PARTICLES

The idea is is to solve the constrai aint and plug the solution

  • n back to the lagrangian

angian. . (This can be done explicit citly ly!) !)

16 16

2 1

1 2

ij i j

L d x A A h hC 

 

1 2

1 ( )

ij ij

F hCh x  

A.Y. Alekseev and A.Z. Malkin, Commun. Math. Phys. 169, 99 (1995) [arXiv:hep-th/9312004; C. Meusburger and B. J. Schroers,

  • Class. Quant. Grav. 20 (2003) 2193 [arXiv:gr-qc/0301108.
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SLIDE 17

SOL VING THE CONSTRAINT

17 17

1 2

1 ( )

ij ij

F hCh x  

1

(0) h 

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SLIDE 18

CONTINUITY CONDITION

18 18

The connection ion must be continuou

  • us across the boundar

dary of the disk. Decompo mposing ing the P Poincare are group elements into Lorentz and translat lational

  • nal parts
  • ne finds that the Lorentz part of the continuit

ity condition tion reads ds

,     ql q l

exp 2 m J             l(t, ) n(t) l(t, )

Lorentz group element!

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SLIDE 19

HOLONOMY AND MOMENTUM

Since the connection ion AH is is gauge ge trivial ial, , its holonomy

  • my along the boundar

dary is is given by by Here is is the group valued momentum charact acteriz rizing ng motion

  • n of the particle

icle. . In terms П of f the lagrangi angian an of f the particle cle has the form

19 19

1 1

2 Hol ( ) (0) (2 ) (0)exp (0)

H J

A C k  

  

          l l l l

1 2

(spin part)=- ( ( ) ( ) is the momentum space frame fiel ) d

a a a

E L P x P E N P m P P

     

 

     x

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SLIDE 20

THE MOMENTUM SPACE

The momentum of П the particle icle is is defined by the group element and thus the momentum sp space is is a a group up manifold

  • ld.

. In fact, the 2+1 +1D D Lorentz group up, , to which П belongs gs is is the 2 2+1D Anti de Sitter space

20 20

 

2 2 2 2 3 1 2 2

1 1 4 P P P P     

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SLIDE 21

NONCOMMUTA TIVE POSITIONS

By dualit ity (Born reciprocit

  • city,

, Majid id co co-gravit ity) ) the position

  • n space is

is non- commu mutat tative

21 21

 

1 ,

a b ab c c

x x x  

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SLIDE 22

TWO PARTICLES

In the case of two (or

  • r many)

) particle icles the procedur dure is is very similar lar:

22 22

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SLIDE 23

TWO PARTICLES

23 23

In the case of two (or

  • r many)

) particle icles the procedur dure is is very similar lar:

D1 D2 H

П1 П2

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SLIDE 24

TWO PARTICLES

The deformed lagrangian angian has the form (no spin) and there is is a a nontrivial ial coup uplin ing between particle icles. . This is is this coup upling ng that makes the total momentum um of the system equal to the deformed composit ition ion

  • f the individual

dual parti ticle cles momenta ta, , given by group product ct. T

  • see this define center and the relative position
  • ns

So So that the lagrangi gian an is is invaria iant under rigid id translat lation ions which do not change ge the partic icle les relative position

  • n,

, with the associa iated total momentum um being П.

24 24

 

1 1 1 1 1 1 1 1 2 2 2 2 1 1 2 1 1 2

L   

    

              x x x

   

1 2 1 2

1 1 , 2 2     x x x d x x

1 2 1

terms, L 

        x d

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SLIDE 25

COMMENTS

No relati tive e localit ity! y! In this s mo model there e is no sign of r relati tive e lo localit lity: y: the rela lati tive e po positio tion n of

  • f t

the pa partic ticle les s is invaria ariant nt under r rigi gid d translation slations. s.

  • BTW. (for expe

perts) s) this ma makes the construc uction tion of t the vertex quite ite natural and unique ue (no sudoku needed!) d!). This s effecti tive e pa partic icle le mo model works s only in 2+1D and cannot t be extende nded d to higher her dime mensio sions. . There e is a mo model with h (kind nd of) the κ-Poinc ncar are struct cture, ure, which h can be extende nded d to higher er dime mensio sion n (talk k in Rome me). 25 25

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SLIDE 26

COMMENTS: AND WHA T ABOUT 3+1D?

There are only circumstan mstantial tial evidences: 1. 1. Grav avit ity in 3+ 3+1D D can be defi fined as s a const straine ained topologic

  • gical

al fi field theory, , when the constrain aint is is forced to vanish one has a TFT; 2. 2. One One can couple this theory to parti ticle cle(s) (s) and even argue that such a a system can be describe bed by CS theory in 2 2+1D, like 2+1 gravit ity, , but with more complic licate ated gauge ge group;

26 26

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SLIDE 27

THE MESSAGE

1. 1. In 2+1D we c can honesty derive the deforme med d single- and multi-pa parti ticle cle action ions s with momentum um sp space being a group up manifold;

  • ld; and momenta

ta of f the particle( icle(s) ) represented d by group p elements; 2. 2. The total momentum m of the multi-par parti ticle cle system is gi given by the group p produc duct t of the group p elements representing ing momenta ta of the particle icles; 3. 3. The multipar particle icle lagrangi gian contain ins the „topological interaction terms” and the form of these t terms is such that local alit ity turns out to be a absolu

  • lute

e (not relative). e). 4. 4. It is un unclear ar if this results can be applie ied d beyond the 2+1D setup.

27 27