De Sitter space as an arena for doubly special relativity
Post on 04-Jul-2016
Embed Size (px)
Physics Letters B 547 (2002) 291296www.elsevier.com/locate/npe
De Sitter space as an arena for doubly special relativity
Jerzy Kowalski-Glikman 1
Institute for Theoretical Physics, University of Wrocaw, Pl. Maxa Borna 9, Pl-50-204 Wrocaw, PolandReceived 1 August 2002; received in revised form 22 September 2002; accepted 30 September 2002
Editor: P.V. Landshoff
We show that Doubly Special Relativity (DSR) can be viewed as a theory with energymomentum space being the four-dimensional de Sitter space. Different formulations (bases) of the DSR theory considered so far can be therefore understood asdifferent coordinate systems on this space. The emerging geometrical picture makes it possible to understand the universalityof the non-commutative structure of spacetime of doubly special relativity. Moreover, it suggests how to construct the mostnatural DSR basis, which turns out to be the bicrossproduct basis. 2002 Published by Elsevier Science B.V.
1. The DSR theory
Doubly special relativity theory is a new attemptto approach the problem of quantum gravity. Thistheory was proposed about a year ago by Amelino-Camelia  and is based on two fundamental assump-tions: the principle of relativity and the postulate ofexistence of two observer-independent scales, of speedidentified with the speed of light c,2 and of mass (orlength = 1/) identified with the Planck mass. Thereare several theoretical indications that such a theorymay replace Special Relativity as a theory of relativis-tic kinematics of probes whose energies are close tothe Planck scale. First of all both loop quantum grav-
E-mail address: firstname.lastname@example.org(J. Kowalski-Glikman).
1 Research partially supported by the KBN grant 5PO3B05620.2 In what follows we set c= 1.
ity and string theory indicate appearance of the min-imal length scale. It is therefore not impossible thatthis scale would be present in description of ultra highenergy kinematics even in the regime, in which gravi-tational effects are negligible. Secondly, in both infla-tionary cosmology  and in black hole physics one faces the conceptual trans-Planckian puzzle ofordinary physical quanta being blue shifted up to thePlanck energies, which as advocated by many can besolved by assuming deviation from the standard dis-persion relation at high energies, and thus deviationfrom the standard relativistic kinematics. It should bealso stressed that some DSR models might providea resolution of observed anomalies in astrophysicaldata . Moreover, predictions of the DSR scenariomight be testable in forthcoming quantum gravity ex-periments .
Soon after appearance of the papers  it wasrealized [6,7] that the so-called -Poincar algebra in
0370-2693/02/$ see front matter 2002 Published by Elsevier Science B.V.PII: S0370-2693(02)0 27 62 -4
292 J. Kowalski-Glikman / Physics Letters B 547 (2002) 291296
the bicrossproduct basis  provides an example ofthe energymomentum sector of DSR theory.3 Thisalgebra consists of undeformed Lorentz generators
[Mi,Mj ] = iijkMk, [Mi,Nj ] = iijkNk,(1)[Ni,Nj ] = iijkMk,
the standard action of rotations on momenta
(2)[Mi,pj ] = iijkpk, [Mi,p0] = 0,along with the deformed action of boosts on momenta
[Ni,pj ] = i ij(
2(1 e2p0/)+ 1
(3) i 1pipj
governed by the observer-independent mass scale .The algebra (1)(3) is, of course, not unique. The
presence of the second observer-independent scale makes it possible to consider transformations toanother DSR basis, in which (1) holds, and thusthe Lorentz subalgebra is left unchanged, but oneintroduces new momentum variables
(4)p0 = f(p0, p 2;
), pi = g
(p0, p 2;
By construction p0 and pi transform under rotationsas scalar and vector, respectively. The functions f andg are assumed to be analytical in the variables p0 andp 2, and in order to guarantee the correct low energybehavior one assumes that for f(p0, p 2
) p0 +O(1/),(5)g(p0, p 2) 1+O(1/).
It can be shown  that also vice versa, any deformedPoincar algebra with undeformed Lorentz sector andstandard action of rotations, which has the standardPoincar algebra as its limit can be related tothe algebra (1)(3) by transformation of the form (4).One should note in passing that this means, in partic-ular, that any modified dispersion relation consideredin the context trans Planckian problem can be ex-tended to a DSR theory, and thus does not need to leadto breaking of Lorentz symmetry.
3 More recently another form of the DSR theory was presentedby . Relations between different forms of DSR were discussedin [10,11].
The algebra (1)(3) does not furnish the wholephysical picture of the DSR theory. To describephysical processes we need also a spacetime sectorof this theory. The question arises as to if it is possibleto construct this sector from the energymomentumsector. The answer turns out to be affirmative if oneextends the energymomentum DSR algebra to thequantum (Hopf) algebra. It was shown in  thatsuch an extension is possible in the case of any DSRalgebra, in particular, for the algebra (1)(3) one getsthe following expressions for the co-product
(6)(pi)= pi 1+ ep0/ pi,(7)(p0)= p0 1+ 1 p0,(8)(Ni)=Ni 1+ ep0/ Ni + 1
(the co-product for rotations is trivial). Then onemakes use of the so-called Heisenberg double pre-scription4  in order to get the following commuta-tors
[p0, x0] = i, [pi, xj ] = iij ,(9)[pi, x0] = i
By using the same method one finds also that thespacetime of DSR theory is non-commuting
(10)[x0, xi] = ixi
and that position operators transform under boosts inthe following way [12,13]
[Ni, xj ] = iij x0 iijkMk,
(11)[Ni, x0] = ixi iNi
(x0 and xi transform as scalar and vector underrotations).
It is important to note that as proved in  ifthe Heisenberg double method is used to derive thespacetime sector of the DSR theory, both the spacetime non-commutativity (10) and the form of theboost action on position operators (11) is universalfor all the DSR theories, i.e., it is invariant of the
4 It should be stressed that the Heisenberg double method is nota unique way of deriving the spacetime structure of the DSR theory(though appealing by its mathematical naturalness).
J. Kowalski-Glikman / Physics Letters B 547 (2002) 291296 293
energymomentum transformations (4), (5). As wewill see this observation finds its natural explanationin the complementary geometrical picture of DSR, tobe developed below, and this is, of course, a strongargument in favor of the Heisenberg double method.
2. DSR algebra and de Sitter space
Since the spacetime algebra of Lorentz generatorsand positions given by (1), (10) and (11) is universal,it is worth to investigate it a bit closer. The first thingto note is that this algebra is the SO(4,1) Lie algebrawith Lorentz generators belonging to its SO(3,1) Liesubalgebra (recall that in special relativity we have todo with the semidirect sum of SO(3,1) and R4, in-stead). Let us recall now that both Lorentz generatorsand positions can be interpreted as symmetry genera-tors, acting on the space of momenta as rotations andtranslations, respectively. But then it follows that thespace of momenta can be identified with (a subspaceof) the group quotient space so(4,1)/so(3,1) which isnothing but the de Sitter space.
To see this explicitly, let us note that amonginfinitely many DSR bases, related to each other bytransformation (4), (5) one finds the basis, in whichthe action of Lorentz algebra on energymomentumsector is classical, i.e.,
(12)[Ni,Pj ] = iij P0, [Ni,P0] = iPi ,while for positions we have the universal algebra (11).Moreover, one finds that in this basis
[Pi,Xj ] = iij(
[Xi,P0] = iPi + i
[Xi,P0] = iPi + i
(13)[P0,X0] = i(
and again the commutator of space and time is givenby (10).5
5 The energymomentum sector of this basis is identical with theenergymomentum sector of Snyders theory of non-commutativespacetime . The relation between this basis and Snyders theory
As it stands, the algebra (10)(13) looks like aparticular DSR basis. The important observation isthat, in agreement with general argument given at thebeginning of this section, the momenta P0 and Pi canbe viewed as coordinates on de Sitter space. Indeed,let de Sitter space be defined by equation
(14)20 + 21 + 22 + 23 + 24 = 2,and let us define the coordinates
(15)P = 4
, = (0, . . . ,3).
It is clear that the coordinates P cover only halfof the whole de Sitter space (the points (,4) and(,4) are identified in these coordinates). Ifone now derives the form of generators of SO(4,1)symmetry of de Sitter space in these coordinates,such that Mi , Ni belong to its SO(3,1) subalgebra,while X are the remaining four generators belongingto the quotient of two algebras SO(4,1)/SO(3,1), onefinds that they satisfy the SO(4,1) relations (1), (10),(11) as well as the cross relations (13).
This simple observation clarifies the universal sta-tus of the algebra satisfied by positions and boost androtation generators in any DSR basis (10), (11). Tounderstand this let us look at the DSR theory fromgeometric perspective suggested by the constructionabove. From this viewpoint the space of momentais not a flat space, as in Special Relativity, but acurved, maximally symmetric space of constant cur-vature. The fact that we need a maximally symmetricspace is related, of course to the fact that only suchspace has the required number of symmetry genera-tors, namely, six rotations identified with Lorentztransformations and four translations in the energymom