a noncommutative friedman cosmological model
DESCRIPTION
A NONCOMMUTATIVE FRIEDMAN COSMOLOGICAL MODEL. A NONCOMMUTATIVE FRIEDMAN COSMOLOGICAL MODEL. Introduction Structure of the model Closed Friedman universe – Geometry and matter Singularities Concluding remarks. 1. INTRODUCTION. GEOMETRY. MATTER. Mach’s Principle (MP): - PowerPoint PPT PresentationTRANSCRIPT
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A NONCOMMUTATIVE FRIEDMAN COSMOLOGICAL
MODEL
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A NONCOMMUTATIVE FRIEDMAN COSMOLOGICAL MODEL
1. Introduction
2. Structure of the model
3. Closed Friedman universe – Geometry and matter
4. Singularities
5. Concluding remarks
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ikikikik TgRgR 2
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GEOMETRY MATTER
Mach’s Principle (MP): geometry from matter
Wheeler’s Geometrodynamics (WG): matter from (pre)geometry
1. INTRODUCTION1. INTRODUCTION
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•MP is only partially implemented in Genaral Relativity: matter modifies the space-time structure (Lense-Thirring effect), but
•it does not determine it fully ("empty" de Sitter solution),
in other words,
•SPACE-TIME IS NOT GENERATED BY MATTER
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For Wheeler pregeometry was "a combination of hope and need, of philosophy and physics and mathematics and logic''.
Wheeler made several proposals to make it more concrete. Among others, he explored the idea of propositional logic or elementary bits of information as fundamental building blocks of physical reality.
A new possibility:A new possibility: PREGEOEMTRY NONCOMMUTATIVE GEOMETRY
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References• Mathematical structure: J. Math. Phys. 46, 2005,
122501.• Physical Interpretation: Int. J. Theor. Phys. 46,
2007, 2494.• Singularities: J. Math. Phys. 36, 1995, 3644.• Friedman model: Gen. Relativ. Gravit. 41, 2009,
1625.• Earlier references therein.
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=EG
E
M = (p, g)
p
pg
1=EE = (p1, p2)p1
Transformation groupoid:
Pair groupod:
i 1 are isomorphic
p2
2. STRUCTURE OF THE MODEL2. STRUCTURE OF THE MODEL
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space-time
frame bundle
Lorentz group
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),( C cCA
with convolution as multiplication:
)(1
1121121 )()())((
d
dffff
The algebra:
Z(A) = {0}
MEMCZ MM :)),((* "Outer center":
),()(),)(,(
:
gpapfgpaf
AAZ
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Basic idea: Information about unified GR and QM is contained in the differential algebra (A, DerA)
DerA V = V1 + V2 + V3
V1 – horizontal derivations, lifted from M with the help of connection
V2 – vertical derivations, projecting to zero on M
V3 – InnA = {ad a: a A}
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21 VV
3V
3V
- gravitational sector
- quantum sector
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Metric
),(),(),( 2211 vukvugvuG
g - lifting of the metric g from M
ZVVk 22: assumed to be of the Killing type
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Gravitational sector:Gravitational sector:
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33 ),0(,,),,0(:),,,( STSTM
))sin(sin)(( 22222222 ddddRds
RR MME ,,,,:),,,,(
R
ttt
tt
G ,
0000
0000
00coshsinh
00sinhcosh
3. CLOSED FRIEDMAN UNIVERSE – GEOMETRY AND3. CLOSED FRIEDMAN UNIVERSE – GEOMETRY ANDMATTERMATTER
Metric:
Total space of the frame bundle:
Structural group:
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R 2121 ,:),,,,,(
Groupoid:
),( C cCA
Algebra:
R
dbaba ),,,,,(),,,,,(),,,,,)(( 2121
MaZ ,:),(
"Outer center":
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22222
22222222
sinsin)(
sin)()()(
ddR
dRdRdRds
Metric on V = V1V2:
Einstein operator G: V V
q
h
h
h
B
Gcd
0000
0000
0000
0000
0000
))(
)('
)(
1(3
4
2
2
R
R
RB
)(
)(''2
)(
)('
)(
134
2
2
R
R
R
R
Rh
))(
)(''
)(
1(3
32
R
R
Rq
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Einstein equation: G(u)= u, uV
5
4
3
2
1
5
4
3
2
1
0000
0000
0000
0000
0000
u
u
u
u
u
u
u
u
u
u
q
h
h
h
B
),...,( 51 - generalized eigenvalues of G
i Z13
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iWe find by solving the equation
0)det( IG
))(
)('
)(
1(3
4
2
2 tR
tR
tRB
Solutions:Generalized eigenvalues: Eigenspaces:
WB – 1-dimensional
)(
)(''2
)(
)('
)(
134
2
2 tR
tR
tR
tR
tRh Wh – 3-dimensional
))(
)(''
)(
1(3
32 tR
tR
tRq Wq – 1-dimensional
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By comparing B and h with the components of theperfect fluid enery-momentum tenor for the Friedmanmodel, we find
)(8 GB
)(8 Gph c = 1
We denote
GT B 8/00
3,2,1,)()8/( kipGT ikh
ik
In this way, we obtain components of the energy-momentum tensor as generalized eigenvalues of Einstein operator.
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What about q?
hBq 2
3
2
1
This equation encodes equation of state:
))(3)((4 tptG
Gq 4
0q
- dust
- radiation
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INTERPRETATION
• When the Einstein operator is acting on the module of derivations, it selects the submodule to which there correspond generalized eigenvalues • These eigenvalues turn out to be identical with the components of the energy-momentum tensor and theequation representing a constraint on admissible equations of state. • The source term is no longer made, by our decree, equal to the purely geometric Einstein tensor, but is produced by the Einstein operator as its (generalized) eigenvalues. • In this sense, we can say that in this model ‘pregeometry’ generates matter.
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4. SINGULARITIES4. SINGULARITIES
Schmidt's b-boundary
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Quantum sector of the model:
p
daa
by
HBoundA
p
pp
11
11 )()())()((
)(:
- regular representation
)(,, 2 pp LHEp
Every a A generates a random operator ra on (Hp)pE
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Random operator is a family of operators r = (rp)pE,i.e. a function
ep
pHBoundEr
)(:
such that(1) the function r is measurable: if ppp H ,
then the function CprpE pp ),)((
is measurable with respect to the manifold measure on E.
(2) r is bounded with respect to the norm ||r|| = ess sup ||r(p)|| where ess sup means "supremum modulo zer measure sets".
In our case, both these conditions are satisfied.19
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N0 – the algebra of equivqlence classes (modulo equalityeverywhere) of bounded random operators ra, a A.
N = N0'' – von Neumann algebra, called von Neumann
algebra of the groupoid .
In the case of the closed Friedman model
))((,( 2 RLBoundMLN
Normal states on N (restricted to N0) are
RRM
ddddaA 212121 ,,,),,,(),,,()(
Epp aA ))(( - density function which is integrable, positive, normalized;to be faithful it must satisfy the condition >0.
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We are considering the model 1],0[ STM Let 0 or 0.Since is integrable, (A) is well defined for every aon the domaini.e. the functional (A) does not feel singularities.
RRM
Tomita-Takesaki theorem there exists the 1-parametergroup of automotphisms of the algebra N
pp itHa
itHat eprepr )())((
which describes the (state dependent) evolution ofrandom opertors with the Hamiltonian )( pLogH p
This dynamics does not feel singularities. 21
A. Connes, C. Rovelli, Class. QuantumGrav.11, 1994, 2899.
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5. CONCLUDING REMARKSOur noncommutative closed Friedman world model is a toy model. It is intended to show how concepts can interact with each other in the framework of noncommutative geometry rather than to study the real world. Two such interactions of concepts have been elucidated:
1. Interaction between (pre)geoemtry and matter: components of the energy-momentum tensor can be obtained as generalized eigenvalues of the Einsten operator.
2. Interaction between singular and nonsingular.
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Quantum sector of our model (which we have not exploredin this talk) has strong probabilistic properties: all quantumoperators are random operators (and the correspondingalgebra is a von Neumann algebra). Because of this, on thefundamental level singularities are irrelevant.
Usually, two possibilities are considered: either the futurequantum gravity theory will remove singularities, or not. Here we have the third possibility:
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By using Schmidt's b-boundary procedure singularitiesappear as the result of taking ratio GEM /
Therefore, on the fundamental level the concept of the beginning and end is meaningeless. Only from the point of view of the macroscopic observer can one say that the universe had an initial singularity in its finite past, and possibly will have a final singularity in its finite future.
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Singularities appear (together with space, time and multiplicity) when one goes from the noncommutativeregime to the usual space-time geometry.
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?THE END