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The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de...

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More about the infrared structure of the de Sitter Universe: Tachyons ay [email protected] SW6 Cargese 2012
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Page 1: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

More about the infrared structure of the de Sitter

Universe: Tachyons

ay [email protected]

SW6 Cargese 2012

Page 2: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .
Page 3: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

SHORT TALK

Page 4: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Tachyons

• What do we mean by tachyons?

• Local and covariant quantum tachyons do not exist

• De Sitter local and covariant tachyons DO exist for discrete (integer) values of the negative squared mass

• Do not know yet the physical meaning (if any)

• END OF THE SHORT TALK

Page 5: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Long talk (Now you may start again to watch

the screen of your laptop or surf the internet…..)

Page 6: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Relativistic Tachyons

• Is the trasmission of energy faster than light contradicting special relativity?

• When , E and p diverge.

• A classical massive particle moving at one time cannot move at a later time; this does not rule out other “particles” moving faster. Photons for instance do exist! But they are massless

Page 7: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Relativistic Tachyons II

A

A B

B

A

Feinberg’s reinterpretation principle: Emission of a positive energy tachyon = Absorption of a negative energy tachyon

Page 8: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

The degrees of freedom of standard linear fields are provided by

the commutator function: a bidistribution that vanishes at spacelike

separated pairs

On a globally hyperbolic manifold the equations of motion plus canonical initial conditions uniquely determine the commutator

Linear Quantum Field Theory

Page 9: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

A Hilbert space representation is associated to any two-point

function that solves the equations of motion

The functional equation (canonical quantization)

And the positive-definiteness condition

For Minkowski,dS, adS or other simmetries if unbroken: invariance:

Two-point functions

Page 10: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

There exist a complete set of states having positive energy

1) 2 pt functions and propagators

3) Perturbation theory 4) Renormalization

2) Free fields

equivalent to

Spectral Property

Consequences

Page 11: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Klein-Gordon field summary

Page 12: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .
Page 13: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Klein-Gordon bradyons

Spectral condition

Page 14: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

The spectral condition implies that the Fourier representation is meaningful in a domain

of the complex Minkowski spacetime

)V z(Imz T

)V z(Imz T

Page 15: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

The Cut reflects Causality and the Quantum

Spectrum + Lorentz Inv.

Page 16: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Klein-Gordon tachyons I

Page 17: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .
Page 18: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Klein-Gordon tachyons I

• The 2-p function is covariant and positive definite

• The commutator vanishes identically

• The anticommutator does not (but the quantization is not canonical)

• The energy spectrum is unbounded below

Page 19: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Klein-Gordon tachyons II (Feinberg)

Page 20: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .
Page 21: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Klein-Gordon tachyons II (Feinberg)

• The “quantization” is not covariant but positive • The commutator does not vanishes; it is neither canonical nor

covariant • The anticommutator is covariant but it not canonical (Feinberg

invokes the name “scalar fermions” for this. ) • The energy spectrum is bounded below in every frame. Positive in

the chosen frame (non-covariant spectral condition)

Page 22: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Klein-Gordon tachyons III (Schroer)

• Feinberg’s quantization may be rendered covariant by adding a complex manifold to Feinberg’s integration cycle

Page 23: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .
Page 24: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Klein-Gordon tachyons III (Schroer)

• Feinberg’s quantization may be rendered covariant by adding a complex manifold to Feinberg’s integration cycle

• The 2-point function is covariant but not positive definite. It is not a

tempered distribution but grows exponentially in momentum space • Locality holds. The theory is canonical • There exists no Lorentz invariant physical positive subspace • This quantization may be obtained as the analytic continuation to

imaginary masses of the standard KG fields

Page 25: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Summary

• When quantizing the Klein-Gordon tachyon it is impossible to reconcile the axioms.

• Give up either locality and covariance or positivity (and of course the spectral condition).

Page 26: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

de Sitter

Page 27: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Energy content of the universe

dark energy 74%

Deark Matter21%

Ordinary matter 5%

Page 28: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Eq. Friedmann

74% 21%

5%

Today

99% 1%

Tomorrow

+ State Eqs. od the various components of the cosmic fluid

= time evolution of the Hubble “constant”

Page 29: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Einstein Equations

Page 30: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Spherical de Sitter model

Page 31: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Flat de Sitter model

Page 32: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Open de Sitter model

Page 33: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

The shape of our universe

M(d+1) : ημν = diag(1,-1,……,-1)

Page 34: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

The asymptotic cone

M(d+1) : ημν = diag(1,-1,……,-1)

Page 35: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

The asymptotic cone: causal structure

Page 36: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

ds timelike geodesics

Page 37: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

The asymptotic cone as the de Sitter momentum space

Page 38: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Conserved quantities

Page 39: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Energy

• In special relativity the energy of a particle is measured relative to an arbitrary given Lorentz frame, being the zero component of a four-vector.

• This picture does not extend to the de Sitter case where frames are defined only locally.

• The maximal symmetry of the de Sitter universe allows for the energy of a pointlike particle to be defined relative to just one reference massive free particle understood conventionally to be at rest (a sharply localized observer)

• The energy of the free particle (ξ,η) with respect to the reference geodesic (u,v) is defined as follows

Page 40: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Energy

Page 41: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Energy

Page 42: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Energy

• E can be interpreted as the correct de Sitter energy of the particle is confirmed by noting that it is the conserved quantity associated to the invariance of the particle action under time translation.

• Indeed, since in flat coordinates the spatial distances dilate in the course of time by the exponential factor the expression of an infinitesimal symmetry under time evolution is

• The action

• is invariant and E can be obtained from S by standard methods

Page 43: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Classical scattering

Page 44: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Example: particle decay

Page 45: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

de Sitter plane waves

Page 46: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

de Sitter plane waves

Page 47: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Principal de Sitter waves

Page 48: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Complementary de Sitter waves

Page 49: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Discrete de Sitter waves

Page 50: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

dS: construction of two-point functions

Page 51: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

They are dS invariant

Page 52: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

The plane waves are however irregular

skip

Page 53: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Spectral condition: de Sitter tubes

Page 54: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .
Page 55: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

are globally well-defined in the tubes.

Page 56: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Fourier representation for BD 2-point functions

Page 57: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Fourier representation on the real manifold

Page 58: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

= -1

Page 59: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Physical fields

• For principal fields positivity is easy

• de Sitter Fourier transform(s)

Page 60: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Complementary fields (inflation)

• Positivity is a little less direct. For ν>0 we have

• The kernel in the following expression is positive definite for 0< ν<(d-1)/2

Page 61: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

De Sitter Tachyons

Page 62: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

The field equation gets an anomaly

Page 63: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Euclidean approach (Folacci)

Page 64: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Zero modes

Page 65: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Infrared divergence

Page 66: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

BRS quantization

Page 67: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

BRS quantization

Page 68: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Fourier representation

Page 69: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Sketch of the proof

Page 70: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Remarks

Page 71: The de Sitter Universe - cpt.univ-mrs.frcosmo/SW_2012/PPT/Moschella.pdf · structure of the de Sitter Universe: Tachyons ay ugomoschella@gmail.com SW6 Cargese 2012 . SHORT TALK .

Conclusion and Outlook

• Physics of the de Sitter Tachyons remains to be understood

• This work was done in collaboration and friendship with Jacques Bros and Henri Epstein

• See you in Cargese again!


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