evidence for accelerated expansion interpretation – phenomenology explanation – theory the...

31
Evidence for accelerated expansion Interpretation – “phenomenology” Explanation – “theory” The Accelerating Universe: A Challenge to Fundamental Physics ןןןןןן- ןןןןןןןןןן ןןRam Brustein Irit maor (BGU Cambridge) P. Steinhardt (Princeton) PRL 86 (2001), PRD 65 (2002), PRD 67 (2003)

Upload: destinee-chattin

Post on 31-Mar-2015

213 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

Evidence for accelerated expansion Interpretation – “phenomenology” Explanation – “theory”

The Accelerating Universe: A Challenge to Fundamental Physics

אוניברסיטת בן-גוריון

Ram BrusteinIrit maor(BGU Cambridge)P. Steinhardt (Princeton)

PRL 86 (2001), PRD 65 (2002),PRD 67 (2003)

Page 2: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

Et pourtant il accélère ! L'expansion de l'Univers, loin de ralentir comme on le pensait depuis soixante-dix ans, est en train de s'accélérer sous la pression d'une mystérieuse énergie noire. Les astrophysiciens tentent de comprendre la nature de ce constituant majeur de l'Univers.

01/02/2003 La Recherche

La concordance de toutes ces expériences a fait sursauter plus d'un cosmologiste. À l'aube du XXIe siècle, il devient clair que 95 % de l'Univers nous est totalement étranger ! Les astrophysiciens s'aperçoivent que toutes leurs théories ne se fondent que sur l'observation des cinq petits pour cent visibles de l'énergie totale [fig. 4]. De quoi rendre sceptique le commun des mortels, mais pas les scientifiques, qui continuent à bâtir leur édifice théorique contre vents et marées. Leur plus grand défi est aujourd'hui de dévoiler la nature de cette énergie noire,

Page 3: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

מפץ גדול חם : המודל הסטנדרטי

0)(3

)(4

83 2

pH

pGH

GH

N

N

Geometry

GR: a(t), 1+ z =a(now)/a(t),

Matter (z), p(z), w(z) = p/

aaH /

2222 )( drtadtds

C- critical density (Euclidean space)X - X / C

Page 4: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

3/1

030

/ 2

w

pa

HHaa

0)(3

)(4

83 2

pH

pGH

GH

N

N

Accelerated expansion ?!Radiation = 3p, w = 1/3

Matter (normal and dark)

p=0, w = 0

Attractive gravity + “normal” matter decelerated expansion

Page 5: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

Mapping the Universe

Luminosity – energy/time emitted by source Flux – energy /time/area absorbed by detector

Due to expansion:Energy/time(1+z)2 (1+z) – red shift of energy(1+z) – increased timeNeed “standard candles”

Page 6: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

For light

2a

dadz

dt

da

aH

1

0222 dradt

Luminosity distance dL vs. redshift z: Hubble Diagram

Example:SNIa

Page 7: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

Proper diameter - dObserved angular diameter – d/(a r)

rtad

d A )( 1

Example:Peaks in CMB spectrum

Angular distance dA vs. redshift z

Need “standard feature”

Page 8: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

Evidence for Accelerated ExpansionDirect and Indirect

• Cosmic Microwave Background : inhomogeneities in radiation

• Large Scale Structure :

inhomogeneities in matter

object counts: galaxies, clusters, weak lensing, strong lensing, …

• SuperNovae Ia – most direct

Page 9: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

SNIaהתפוצצות גרעינית של ננסים לבנים

מתאם בין בהירות שיא, צורה וספקטרום של עקומת

פיזור ~% 10האור בבהירות שיא

Page 10: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

di

mmer

more distantz

m

AC/DC

pure matter

L

L

d

dm

10ln

5

L

Lm

Key issue:systematic errors

Current SNIa Data

preferred

fiducial models:m= 0.3

wQ= const.

Previous version: Sci. Am. 1/2001

Page 11: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת
Page 12: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

)1( mQ

QQQm

Qm

T

TT

w

wpp

pw

0 20 40 60 80 100

0

20

40

60

80

Current Data

m vs. wQ

(assume flat U.

wQ

-2.5

-1.5

0.50.3

-.5

-3.5

0.7 m

Page 13: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

CMB data : WMAP

February 2003

Cosmic variance!

Page 14: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

One more point on the Hubble diagram

)z ~ 1,000(8.01.2201

~ Flat U.

Cosmic variance!

Page 15: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

4- 6%

20- 40%

60- 80%

Baryons

Dark matter

Dark energy

astro-ph/0302209

Combined results

Interim report I•flat universe• acceleration • consistent• reasonable ?!

small

Page 16: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

The end of the universe is cancelledBy Robert Matthews, Science Correspondent(Filed: 09/02/2003) Professor Hawking, we have a problem. Nasa, the American space agency, is expected to announce this week that it has proved the existence of "dark energy", a cosmic force that counteracts gravity and will keep the universe expanding forever.

The announcement will effectively demolish the theory that life will be wiped out in a "Big Crunch" when the universe collapses, and should end decades of academic dispute over the forces at work on the universe

Page 17: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

Interpretation: theoretical expectations

• Dark energy is not just • Dynamical field (s):

Kinetic & potential energies Interactions with other particles Cosmic friction Very small mass

time-dependence

Page 18: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

Dark Energy EOS• Parametrization in terms of (time-dependent)

Energy density Q(z)

Pressure pQ(z)

EOS wQ(z)=pQ(z)/Q(z)

• previously : wQ = -1

wQ = 0 cold matter

oscillations, “sudden start”, “decay to a constant”

Page 19: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

Luminosity distance dL vs. redshift z

Maor et al.g= m /(1- m)

Current SnIA data: some acceleration inthe last 8 billion years (0 < z < 1)

Page 20: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

l'avenir: SNAP (F)

SNAP proposal:1000’s de SNIa, surtout 0 < z < 1.2, quelques-uns1.2 < z < 1.7

snap.lbl.gov

Also:ESSENCECFHLS (F)GOODS,SNFactory (F)

Page 21: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

fiducial models:m= 0.3wQ= const.

wQ = -1

wQ = -1/3

wQ = 0

See: Sci. Am. 1/2001

Page 22: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

Degeneracy!

a) DLb) DL/DLc) wQ (z)

For 9 different EOS

Maor et al.

Page 23: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

• Dark energy expected to “disappear” for z > 2

• CMB photons propagate most of the way through matter dominated U.

No gain compared to “low z” probes

• Best accuracy for dL from CMB ~ 1%

CMB comparable to other probes

CMB cannot help much …Maor & Brustein

Page 24: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

Interim report II

• recent acceleration (0 < z < 1, today < t < 8 billion years)• evidence from many sources, consistent.• qualitative information only (on

fundamental physics) from most accurate planned experiments

Page 25: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

Dark sector &

the standard model of particle physics

4- 6%

20- 40%

60- 80%

Baryons

Dark matter

Dark energy

Page 26: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

Dark sector &

gravity and quantum mechanics

N

Vacuum

GG 800

21

Does not make sense as a normal source

4- 6%

20- 40%

60- 80%

Baryons

Dark matter

Dark energy

Page 27: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

(R.B.) : Cloud No. IV: Black Hole Entropy

:

"We live where we can live," NYT: 2 Sept. 2003

Page 28: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

• Quantum mechanics• More space dimensions• Cherished principles: causality, …

Something has to give

N

Vacuum

GG 800

21

• Gravity

• Matter – additional fields, light, extremely weakly coupled – “quintessence”

and the ugliest(?) of them all: the Anthropic principle

Page 29: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

The “boring” option: Quintessence

•“Tracker” fields•Many other possibilities

Degeneracies

m ~ H = 10 –33 eVV ~ crit ~ (10

-3eV)

4

Steinhardt + …Rhatra+PeeblesWetterich …

Maor & Brustein

Page 30: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

The Anthropic PrincipleR. Dicke (1961): “ carbon-based life can only arise when the Dirac large numbers hypothesis is true because this is when burning stars exist”

B. Carter (Early 1970’s): “what we can expect to observe must be restricted by the conditions necessary for our presence as observers” (Leslie ed. 1990). The word "anthropic" was intended as applying to intelligent beings.

A possible argument for preferring the God hypothesis: think in terms of many possible fundamental theories, God selecting a theory which permitted life's requirements to be fulfilled without contradictions.

Page 31: Evidence for accelerated expansion Interpretation – phenomenology Explanation – theory The Accelerating Universe: A Challenge to Fundamental Physics אוניברסיטת

Conclusions

• Excellent measurements are not good enough as clues for fundamental physics !

• A large source of error: theory• Need:

–either a new “local” test -what is it?–or radically new theoretical input -what is it ?

• Theory situation in a nut-shell

“we don’t have a clue”• Personal hope: revolutionary resolution