Transcript
Page 1: Dark Universe or twisted Universe? Einstein- Cartan  theory

Thomas Schucker : CPT Marseille FranceAndre Tilquin : CPPM Marseille France

THCA Tsinghua China\

Dark Universe or twisted Universe?

Einstein-Cartan theory.

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ReferencesarXiv:1104.0160

arXiv:1109.4568

Preliminary

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Outlook

Einstein general relativity: quick reminderParallel transport and curvatureLimitation in GR

Einstein-Cartan general relativityTorsion: what is that?Parallel transport and torsionProperties and advantages

Results on supernovae with a twisted Universe

Solving Einstein-Cartan equationsEffect of torsion on Hubble diagram

Summary and further work3

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Parallel transport and differential geometry

A

B

How to transport a vector or a frame in a curve space?

-Using this procedure on a reference frame and in the limit of a null surface defines the Einstein tensor: which is symmetric in -Geometry generates rotation

๐บ๐œ‡๐œˆ=๐‘…๐œ‡๐œˆโˆ’1 /2๐‘…๐‘”๐œ‡๐œˆ

ฮฑ Related to curvature

A1

A2

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General relativity๐บ๐œ‡๐œˆ=8๐œ‹ ๐บ๐‘‡ ๐œ‡๐œˆ

Einstein equation relates curvature with energy momentum tensor

As a consequence of symmetric Riemann geometry, the energy momentum tensor is symmetric:

General relativity can accommodate particle with spin including spin-1/2 using vierbein formalism (all tensors are represented in terms of a chosen basis of 4 independent orthogonal vectors field)

However it can not describes spin-orbite coupling because when spin and orbital angular momentum are being exchanged, the momentum tensor is known to be nonsymmetric. According to the general equation of conservation of angular momentum:

Where is the torque density = rate of conversion between orbital momentum and spin.

๐‘‡ ๐œ‡๐œˆ=๐‘‡๐œˆ๐œ‡

Cartan => Torsion 5

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* What is torsion? A kind of local mobius strip

๐‘Ž โ€ฒ

โ„ต=๐‘Ž .

t=โˆ’ ๐‘ . ๐‘ โ€ฒ

โ„ต

t

Cartan assumed that local torsion is related to spin ยฝ particles

curvature

torsion

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Parallel transport with torsion and spin

A

B

-Geometry generates translation

A3

A1

A2

-In presence of torsion the infinitesimal parallelogram does not close

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ฮฑ translation

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Some properties/advantages of torsionโ€ข Energy momentum is still the only source of space-time

curvature with the Newtonโ€™s constant being the coupling constant

โ€ข The source of torsion is half integer spin with the same coupling constant

โ€ข Spin 1 particle is not source of torsion: photon not affectedโ€ข Photon and spin ยฝ particle (neutrino) geodesics are differentโ€ข Torsion doesnโ€™t propagate

โ€ข Itโ€™s non-vanishing only inside matter with half integer spin

โ€ข Theories of unification between gravity and standard model of particle physics need a torsion field (loop quantum gravity)

โ€ข Supergravity is an Eistein-Cartan theory. Without torsion this theory loses its supersymmetry.

โ€ข Torsion provides a consistency description of general relativity

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Einstein-Cartan consistency

curvature

๐บ๐œ‡๐œˆEnergy-

momentumNoether theore

m

spin

Noether theore

m

rotations

geometry

Translations

geometry

ยฟ

TorsionCartan

equation9

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In space time with torsion there are 2 Einstein equations ( in vierbien frame):1. Equation for curvature:

2. Equation for torsion (ฮฃ):

New Einstein equations

ฮฃ๐‘๐‘’๐‘‘๐œ–๐‘Ž๐‘๐‘๐‘‘=โˆ’8๐œ‹ ๐บ๐‘†๐‘Ž๐‘

๐บ๐‘Ž๐‘=๐‘…โˆ—๐‘Ž๐‘โˆ’1/2๐‘…โˆ—๐‘”๐‘Ž๐‘

R* is the modify Ricci tensor no more symmetric = spin tensor

In a maximally symmetric Universe the most general energy momentum tensor has two functions of time:

The density : The pressure :

The most general spin densityEven parity : Odd parity :

With equation of state:

With โ€œequations of stateโ€:

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Generalized Friedmann equations

In maximally symmetric and flat Universe Friedmann equations have 4 unknown functions of time: a,b,f and ฯ.

Using these expressions today and the dimensionless density :

; ;

The Friedmann like closure relation reads:ฮฉ๐‘š+ฮฉฮ›+2ฮฉ๐‘ โˆ’ฮฉ๐‘ 

2+94 ฮฉ~๐‘ 

2=1 11

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From theory to Supernovae dataSupernovae of type Ia are almost standard candle:

There intrinsic luminosity (L) can be standardized at a level of about 15%

Thus the apparent luminosity can be used as a distance indicator: with

And the redshift as a scale factor measurement: =

Because the geodesic equations for photons decouple to torsion, redshift and luminosity have the same expression

->We just need to compute the scale factor 12

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ms ฮฉm ฮฉฮ›

marginalized

Supernovae and Hubble diagram

๐œ‡ (๐‘ง )=๐‘š๐‘ +2.5 log ๐‘™ (๐‘ง )

We used the so called Union 2 sample containing 557 supernovae up to a redshift of 1.5

Standard cosmology fit gives (no flatness):

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Fitting procedure for SN

Free cosmological parameters are:where is deduced from Friedman like relation

ฮฉ๐‘š+ฮฉฮ›+2ฮฉ๐‘ โˆ’ฮฉ๐‘ 2+94 ฮฉ~๐‘ 

2=1

We use the full covariance matrix, taking into account systematic errors and correlations to compute

and

The best cosmological parameters are computed by minimizing the :

Errors and contours are computed by using the frequentist prescription:

๐œ• ๐œ’ 2

๐œ•ฮฉ๐‘˜=0

๐œ’2 (ฮฉ๐‘š )= minฮฉ๐‘  ,๐‘š๐‘ โ‹ฏ

๐œ’ 2(ฮฉ๐‘š ,ฮฉ ๐‘ ยฟ,๐‘š๐‘ โ‹ฏ)+๐‘ 2 ยฟ

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Results on torsion (flat Universe).Even parity torsion: Odd parity torsion:

ฮฉm ฮฉฮ› ฮฉm ฮฉฮ›

ฮฉm ฮฉฮ›

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Could torsion replace dark matter?Even parity torsion gives a prefer value for matter density equal to 0.09

ฮฉ๐‘š=0.09+0.30โˆ’0.07

The WMAP last results are:

and 0.03Supernovae results analyzed with torsion give a result statistically compatible with both dark matter and baryonic matter.

However, torsion can contribute to a certain amount of dark matter.

Or better to say that torsion without dark matter is not incompatible with Supernovae data.

More data or probes should be used to definitely conclude 16

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Could torsion replace dark energy?We test the hypothesis of a null cosmological constant by using the log

likelihood ratio technic: Assume we want to test 2 different models, with one include in the other:

We can define the log likelihood ratio as:

The probability distribution of this variable is approximately a distribution with a number of degree of freedom equal to the difference of ndofโ€™s = 1

๐‘…=๐œ’2๐‘š๐‘–๐‘› ,1โˆ’ ๐œ’ 2๐‘š๐‘–๐‘› , 2

Fore even parity: For odd parity :

This is not surprising because equation of state: If acceleration today, then acceleration in the past: s with

17In contradiction with previous publication (S. Capozziello et al. 2003)

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Summary and further workโ€ข Standard general relativity should be extended to account for spin-

orbital momentum coupling: Einstein-Cartan theory.โ€ข If we apply torsion to cosmology we find:

โ€ข Torsion can contribute to dark matter at a certain amountโ€ข Torsion as a source of dark energy is ruled out at more than 5 sigma

Usual problem in cosmology i.e : ฮ› and vacuum energy!

โ€ข However these results are encouraging enough to try to go furtherโ€ข Look at galaxies rotation curves: Need to generalized the

Schwarzschildโ€™s equation. Work in progress.โ€ข Use other probes:

โ€ข CMB/BAO/WL/Clusters: photons are not sensitive to torsion, but dynamic is different, so everything should be recomputed.

โ€ข But we should not be too much excited by the Supernovae result on DM:

We found a spin energy density of about 4% , corresponding to a state parameter which is 42 orders of magnitude away from the naรฏve value

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Questions?1) Torsion and curvature ?

2) Torsion and vacuum ?

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Torsion and curvatureIn the general case, assuming no special equation of state: are free

functions of time:

Torsion is not source of gravity:Odd parity torsion doesnโ€™t couple to dynamic (i.e curvature)Even parity torsion couple to curvature through kinematic not

dynamic

(1)

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* Experimental possible measurements

1. Because geodesics are different for photons and spin ยฝ particles (neutrino)โ€ข Timing difference between photons and neutrinos in

supernovae explosion 1987A Supernovaeโ€ข Neutrino oscillation experiment OPERA. Time delay and supra

luminal neutrino2. Rotation curve of galaxies or the modify Schwartsfield solution

โ€ข What is the effect of torsion on rotation curve of galaxy3. Galaxies and cluster formation4. The cosmological probes:

โ€ข Supernovae 1aโ€ข CMB: effect of torsion in initial plasma (very high matter

density)โ€ข Weak lensing should not be affected

Lensing is gravitational coupling between curvature and photonโ€ข Baryonic acoustic oscillation

Depends on the initial power spectrum

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Parallel transport and curvature tensor

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Let consider the covariant derivative of a vector: with = =

This covariant derivative can be formally written as:๐›ฟ๐œˆ๐œŽ ๐›ป๐œ‡=๐›ฟ๐œˆ๐œŽ ๐œ•๐œ‡+ฮ“ ๐œ‡๐œˆ๐œŽ

And compare to covariant derivative in QED: +

In geometric term, the affine connection is interpreted as the change of vector during parallel transport along :

โˆ’ฮ“ ๐œ‡๐œˆ๐œŽ ๐ด๐œˆ ๐‘‘๐‘ฅ๐œ‡

And the curvature tensor is defined as the change of vector parallel transported around a closed path

ฮ” ๐ด๐œŽ=12 ๐ด

๐œˆ๐‘…๐›ฝ๐œ‡๐œˆ๐œŽโˆฎ ๐œ‰ ๐œ‡๐‘‘๐‘ฅ๐›ฝ

Where is the affine connection

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Covariant derivative in QED

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โ„’=๐œ•๐œ‡๐œ™๐œ•๐œ‡๐œ™โˆ—โˆ’๐‘š2๐œ™๐œ™โˆ—

This Lagrangian is invariant under global rotation in complex plane: is invariant is invariant

But is not invariant under local rotation in complex plane:.

= +

๐œ•๐œ‡(๐œ™ )= ฮ”๐œ™๐›ฟ ๐‘ฅ๐œ‡

+๐ท๐œ‡๐œ™

Variation of the field is assumed to be linear in : ๐ท๐œ‡=๐œ•๐œ‡+๐‘–๐‘’ ๐ด๐œ‡ฮ”๐œ™=โˆ’ ๐‘–๐‘’ ๐ด๐œ‡๐›ฟ๐‘ฅ๐œ‡๐œ™

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Torsion definition

๐œ’๐›ผ

๐œ ๐›ผ

๐œ’๐›ผโˆ’ฮ“ ๐œ‡๐œˆ๐›ผ๐œ ๐œ‡๐œ’ ๐œˆ

๐œ ๐›ผโˆ’ฮ“ ๐œ‡๐œˆ๐›ผ ๐œ’ ๐œ‡๐œ๐œˆ

Then the difference is:

with

Where is defined as the torsion tensor

)

)

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Whatโ€™s the meaning of these new equations of state?

โ€ข = any spin ยฝ matter density with null pressure โ€ข = spin density considered as a perfect fluid!โ€ข has a dimension of time and is assumed to be constant

All physics are inside ws:โ€ข Source of torsion is spin ยฝ particle โ€ข Orbital momentum or spin 1 are not source of torsion.โ€ข No spin orbital momentum coupling. Spin generates local

torsion.โ€ข It contains the Planck constant and GR and QM coupling.

Expected to be small.โ€ข We assume it is not zero even though we donโ€™t know how

spins average?โ€ข โ€ฆโ€ฆโ€ฆ

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Solving the Friedmann equation We eliminate f(t) and

ฯ(t)We are left with 2 first order differential equations and 2 unknown functions a(t) and b(t)

We solve it numerically with the Runge-Kutta algorithm.

This is an iterative numerical algorithmExample:

1. aโ€™(t) = 2 a(t)2. Start from an initial value a(t0)=a03. Compute the derivative aโ€™(t0)=2 a04. Predict the new point at t0+ฮดt using Tailor

expansion : a(t1 = t0+ฮดt) = a0+2a0 ฮดt +โ€ฆ..= a1

5. Start from this new value a(t1)=a1 and iterate

t0

a0

a1

t1=t0+ฮดt

a(t)

tWe used a forth order Runge-Kutta algorithm with an adaptive step in time such that the corresponding step in redshift is much smaller than the experimental redshift error (10-5) 26

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Capozziello et al(2003): Matching torsion lamba-term with observations.In this paper they assume the same Friedmann equations for the

torsion fluidwith ~๐œŒ=๐œŒ+ ๐‘“ 2๐‘Ž๐‘›๐‘‘~๐‘=๐‘โˆ’ ๐‘“ 2

The missing factor 3 implies torsion is source of curvature and a constant โ€œfโ€ function with time which can be interpreted as a cosmological constant.

3

At beginning I made the same kind of mistake and I got

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Unfortunately itโ€™s wrong!

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Dynamic equationIn general case where s(t) and are functions of time we have:

๐‘Ž=1

3 ( ฮ›โˆ’4 ๐œ‹๐บ (๐œŒ+3๐‘ ) )+ 8๐œ‹ ๐บ3 ( (๐‘ก )+ ๐‘Ž ๐‘ (๐‘ก))โ€ข Odd parity torsion doesnโ€™t modify dynamic (Einstein curvature)โ€ข Even parity torsion couple to gravit

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Einstein-Hilbert action

๐‘†=โˆ’ 12๐œ…โˆซ๐‘…โˆšโˆ’๐‘”๐‘‘4๐‘ฅ

The Hilbert action yields the Einstein equation through the principle of least action:

withR the Ricci scalar

In presence of matter the action becomes:

๐‘†=โˆซ [ 12๐œ… ๐‘…+โ„’๐‘€ ]โˆšโˆ’๐‘”๐‘‘4 ๐‘ฅThe action principle leads to:

๐›ฟ๐‘†=โˆซ [ 12๐œ… ๐›ฟ (โˆšโˆ’๐‘”๐‘… )๐›ฟ๐‘”๐œ‡๐œˆ

+๐›ฟ (โˆšโˆ’๐‘”โ„’๐‘€ )

๐›ฟ๐‘”๐œ‡๐œˆ ]๐›ฟ๐‘”๐œ‡๐œˆ๐‘‘4๐‘ฅ๐›ฟ๐‘†=โˆซ [ 12๐œ… ( ๐›ฟ๐‘…๐›ฟ๐‘”๐œ‡๐œˆ

+ ๐‘…โˆšโˆ’๐‘”

๐›ฟ (โˆšโˆ’๐‘”)๐›ฟ๐‘”๐œ‡๐œˆ )+ 1

โˆšโˆ’๐‘”๐›ฟ (โˆšโˆ’๐‘”โ„’๐‘€ )

๐›ฟ๐‘”๐œ‡๐œˆ ]๐›ฟ๐‘”๐œ‡๐œˆโˆšโˆ’๐‘”๐‘‘4 ๐‘ฅ

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Einstein Equation Since the previous equation should hold for any

๐›ฟ ๐‘…๐›ฟ๐‘”๐œ‡๐œˆ+

๐‘…โˆšโˆ’๐‘”

๐›ฟโˆšโˆ’๐‘”๐›ฟ๐‘”๐œ‡๐œˆ =โˆ’2๐œ… 1

โˆšโˆ’๐‘”๐›ฟ (โˆšโˆ’๐‘”โ„’๐‘€ )

๐›ฟ๐‘”๐œ‡๐œˆ

๐‘‡ ๐œ‡๐œˆโ‰”โˆ’2

โˆšโˆ’๐‘”๐›ฟ (โˆšโˆ’๐‘”โ„’๐‘€ )

๐›ฟ๐‘”๐œ‡๐œˆ=โˆ’2

๐›ฟโ„’๐‘€

๐›ฟ๐‘”๐œ‡๐œˆ+๐‘”๐œ‡๐œˆโ„’๐‘€

๐›ฟ ๐‘…๐›ฟ๐‘”๐œ‡๐œˆ=๐‘…๐œ‡๐œˆ

1โˆšโˆ’๐‘”

๐›ฟโˆšโˆ’๐‘”๐›ฟ๐‘”๐œ‡๐œˆ

=โˆ’ 12๐‘”๐œ‡๐œˆ

๐‘…๐œ‡๐œˆโˆ’12๐‘”๐œ‡๐œˆ๐‘…=

8๐œ‹๐บ๐‘4

๐‘‡๐œ‡๐œˆ

The cosmological constant is introduced in the Lagrangian:

๐‘†=โˆซ [ 12๐œ… (๐‘…โˆ’2 ฮ› )+โ„’๐‘€ ]โˆšโˆ’๐‘”๐‘‘4 ๐‘ฅ ๐‘…๐œ‡๐œˆโˆ’12 ๐‘”๐œ‡๐œˆ๐‘…+ฮ› ๐‘”๐œ‡๐œˆ=

8๐œ‹ ๐บ๐‘4

๐‘‡ ๐œ‡๐œˆ


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