+ All Categories
Home > Documents > SEMINÁRIO UFES Vitória, agosto 2013

SEMINÁRIO UFES Vitória, agosto 2013

Date post: 20-Jan-2016
Category:
Upload: zelia
View: 22 times
Download: 4 times
Share this document with a friend
Description:
SEMINÁRIO UFES Vitória, agosto 2013. The quantum-to-classical transition of primordial cosmological perturbations. Nelson Pinto Neto with Grasiele Santos and Ward Struyve. CBPF ICRA. THE STANDARD COSMOLOGICAL MODEL - PowerPoint PPT Presentation
29
SEMINÁRIO UFES Vitória, agosto 2013 The quantum-to-classical transition of primordial cosmological perturbations. Nelson Pinto Neto with Grasiele Santos and Ward Struyve CBPF ICRA
Transcript
Page 1: SEMINÁRIO UFES                         Vitória, agosto 2013

SEMINÁRIO UFES Vitória, agosto 2013

The quantum-to-classical transition of primordial cosmological perturbations.

Nelson Pinto Neto

with Grasiele Santos and Ward Struyve

CBPF

ICRA

Page 2: SEMINÁRIO UFES                         Vitória, agosto 2013

THE STANDARD COSMOLOGICAL MODEL (FRIEDMANN-1922)

Copernicus Principle: space homogeneous and isotropic.

2

2

8

3 i

a G K

a a

43

3

a GP

a

2 2 2 2 2 2 2 2 22

1

1ds dt a t dr r d r sen d

Kr

Page 3: SEMINÁRIO UFES                         Vitória, agosto 2013

But where the structures come from?

• In the standard Friedmann model the Universe was always decelerated:

• p=λρ, λ > 0 a=tq with q<1 (λ=0, q=2/3; λ=1/3, q=1/2)

• Scales of different structures grow with a: lphys = a l

• Curvature scale grows with a1/q: H-1 = RH t a1/q

In the past, observed large scales where much greater then thecurvature scale.Impossible to justify initial spectrum in terms of local physical arguments, unless there is an inflationary phase in the past or a bounce

ln(lphys) = ln(l) + ln(a)

Page 4: SEMINÁRIO UFES                         Vitória, agosto 2013

//

//

/

/

Page 5: SEMINÁRIO UFES                         Vitória, agosto 2013

Φ(x) is the inhomogeneous perturbation, related to theNewtonian potential in the nonrelativistic limit, δφ is the scalar field perturbation.

Evolution of scalar perturbations:

Mukhanov-Sasaki variable →

Hamiltonian for the perturbations from GR →

Equations of motion →

Page 6: SEMINÁRIO UFES                         Vitória, agosto 2013

IN TERMS OF THE FOURIER MODES

The classical solutions

Page 7: SEMINÁRIO UFES                         Vitória, agosto 2013

QUANTIZATION

=

In the Schroedinger picture: Ψ(y,η) = <y|0,η>

Page 8: SEMINÁRIO UFES                         Vitória, agosto 2013

THE PROBLEM

|0> is homogeneous and isotropic, and so is <0|y(x)y(x)|0> (= <0|y(x+δ)y(x+δ)|0>)

Attempts for solving the problem: squeezing positive Wigner distribution in phase spacequantum distribution looks like classical stochastic distribution of realizations of the Universe with different inhomogeneous configurations.

decoherence: avoids interference among realizations.

Severely criticized by Sudarsky and many others:

The state is still homogemeous and isotropic;In the standard interpretation, different potentialities are not realities;How ONE of the potentialities become our real Universe?;What makes the role of a measurement in the early Universe?(we cannot collapse the wave function because we could not exist without stars!)

Page 9: SEMINÁRIO UFES                         Vitória, agosto 2013

The de Broglie-Bohm interpretation

The guidance relation allows the determination of the trajectories (different from the classical)

If P(x,t=0) = A2 (x, t=0), all the statisticalpredictions of quantum mechanics are recovered.

However, P(x,t=0) ≠ A2 (x, t=0), relaxes rapidly to P(x,t) = A2 (x, t) (quantum H theorem -- Valentini)

Born rule deduced, not postulated

Page 10: SEMINÁRIO UFES                         Vitória, agosto 2013

de Broglie-Bohm: particles and fields have actual trajectories, independently of any observation(ontology). One trajectory enter in one branch and singularize it with respect to the others.

SOLUTION OF THE MEASUREMENT PROBLEM:

Page 11: SEMINÁRIO UFES                         Vitória, agosto 2013

Measurement problem:position in configurations space determines choosen branch (depends on X0)

Page 12: SEMINÁRIO UFES                         Vitória, agosto 2013

Some remarks

a) Q is highly non-local and context dependent!It offers a simple characterization of the classical limit: Q=0

b) Probabilities are derived in this theory. The unknown variable is the initial position.

c) With objective reality but with the same statisticalinterpretation of standard quantum theory.

d) One postulate more (existence of a particle trajectory) and two postulates less (collapse and Born rule) than standard quantum theory: 1-2 = -1 postulate

Page 13: SEMINÁRIO UFES                         Vitória, agosto 2013

QUANTIZATION

=

In the Schroedinger picture: Ψ(y,η) = <y|0,η>

Page 14: SEMINÁRIO UFES                         Vitória, agosto 2013

The de Broglie-Bohm solution

The existence of an actual field configuration breakstranslational and rotational invariance.

It obeys guidance equations.

Its initial condition satisfies Born rule at initial time.

Page 15: SEMINÁRIO UFES                         Vitória, agosto 2013

The quantum-to-classical transition

y(η) α |f(η)| α f(η)

Page 16: SEMINÁRIO UFES                         Vitória, agosto 2013

In terms of the quantum potential

Page 17: SEMINÁRIO UFES                         Vitória, agosto 2013

FOR THE BOUNCE

Page 18: SEMINÁRIO UFES                         Vitória, agosto 2013

Statistical predictions:the two point correlation function

Page 19: SEMINÁRIO UFES                         Vitória, agosto 2013

V - CONCLUSION

Bohm-de Broglie interpretation is very suitable for quantum aspects of cosmology!

It explains in a very simple way a very oldcontroversy concerning cosmologicalperturbations of quantum mechanical origin.

What about the other interpretations?

Page 20: SEMINÁRIO UFES                         Vitória, agosto 2013

"To try to stop all attempts to pass beyond the present viewpoint of quantum physics could be very dangerous for the progress of science and would furthermore be contrary to the lessons we may learn from the history of science. This teaches us, in effect, that the actual state of our knowledge is always provisionaland that there must be, beyond what is actually known, immense new regions to discover."

Louis de Broglie

Page 21: SEMINÁRIO UFES                         Vitória, agosto 2013

The problem of quantum measurement

Wave function of system + apparatus : interaction -> bifurcation: but only one branch is observed.

THE PROBLEM OF INTERPRETATION

Copenhaguen interpretation:

Actual facts take place in the classical world.The classical apparatus realizes the collapse ofthe wave function and turn the quantum potentialities into actual and unique facts.

Page 22: SEMINÁRIO UFES                         Vitória, agosto 2013

Fortunately, there are alternative quantum theories!

Many WorldsConsistent HistoriesSpontaneous collapsede Broglie-Bohm..........

We would like that quantum theory could help cosmology!

Within the Copenhaguen interpretation we are stuck: no further developments.

Contemporary quantum theory … constitutes an optimum formulation of [certain] connections … [but] offers no useful point of departure for future developments.Albert Einstein.

Page 23: SEMINÁRIO UFES                         Vitória, agosto 2013

Decoherence: explain why we do not see macroscopicsuperpositions, but...

IT DOES NOT EXPLAIN THE UNICITY OF FACTS!

Page 24: SEMINÁRIO UFES                         Vitória, agosto 2013

X

FOR THE UNIQUE FACT: A COLLAPSE OF THE WAVE FUNCTION IS POSTULATED!

Page 25: SEMINÁRIO UFES                         Vitória, agosto 2013

MANY WORLDS (Everett, DeWitt, Deutsch) All possibilities are realized, but they are not aware of each other.

THERE IS NO UNIQUE FACT!

Page 26: SEMINÁRIO UFES                         Vitória, agosto 2013

SPONTANEOUS COLAPSE (Pearle, Ghirardi, Rimini, Weber, Penrose) Non linear evolution suplemented to Schrödinger.

Page 27: SEMINÁRIO UFES                         Vitória, agosto 2013

“The kinematics of the world, in this ortodox picture, is given by awave function for the quantum part, and classical variables -variables which have values - for the classical part: (Ψ(t,q ...), X(t) ...). The Xs are somehow macroscopic. This is notspelled out very explicitly. The dynamics is not very preciselyformulated either. It includes a Schrödinger equation for the quantum part, and some sort of classical mechanics for theclassical part, and `collapse’ recipes for their interaction.

It seems to me that the only hope of precision with the dual (Ψ,x)kinematics is to omit completely the shifty split, and let both Ψ and xrefer to the world as a whole. Then the xs must not be confined tosome vague macroscopic scale, but must extend to all scales.”

John Stewart Bell.

THE DE BROGLIE-BOHM THEORY

Page 28: SEMINÁRIO UFES                         Vitória, agosto 2013
Page 29: SEMINÁRIO UFES                         Vitória, agosto 2013

“In 1952 I saw the impossible done. It was in papers by David Bohm.… the subjectivity of the orthodox version, thenecessary reference to the ‘observer,’ could be eliminated. . . . But whythen had Born not told me of this ‘pilot wave’? If only to point outwhat was wrong with it? Why did von Neumann not consider it? . . .Why is the pilot wave picture ignored in text books? Should it not betaught, not as the only way, but as an antidote to the prevailing complacency?To show us that vagueness, subjectivity, and indeterminism,are not forced on us by experimental facts, but by deliberate theoreticalchoice?” (Bell, page 160)

“I have always felt since that people who havenot grasped the ideas of those papers. . . and unfortunately they remainthe majority . . . are handicapped in any discussion of the meaning ofquantum mechanics”. (Bell, page 173)

Bell in Speakable and unspeakable in quantum mechanics


Recommended