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Experimental General Relativity

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Outline Past Present Future. Experimental General Relativity. Barak Kol Hebrew Un, Jerusalem DESY June 09. “GR was a theorist’s paradise but an experimentalist’s hell” (Misner, Thorne, Wheeler). Review by Clifford Will. Past. Perihelion shift (Mercury – Einstein 1915). - PowerPoint PPT Presentation
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Barak Kol Hebrew Un, Jerusalem DESY June 09 Outline • Past • Present • Future “GR was a theorist’s paradise but an experimentalist’s hell” (Misner, Thorne, Wheeler) Review by Clifford Will
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Page 1: Experimental  General Relativity

Barak KolHebrew Un, Jerusalem

DESY June 09

Outline• Past• Present• Future

“GR was a theorist’s paradise

but an experimentalist’s hell”

(Misner, Thorne, Wheeler)

Review by Clifford Will

Page 2: Experimental  General Relativity

Past

• Perihelion shift (Mercury – Einstein 1915)

6 GM

p

per revolution

Where p is the ellipse’s semi-latus rectum

1 cosr

p

e

43.0’’/cent out of 5600.0’’/cent observed

Page 3: Experimental  General Relativity

Deflection of light

Eddington’s expedition (1919)(Einstein 1915)

4

1.75''

sunGM

d

Sun grazing rays

Page 4: Experimental  General Relativity

Shapiro (1964) time delay

Actually measure the echo time as it changes as the trajectory evolves.

2ˆ ˆ4 log ( )( ) /sun src src e eGM r x n r n dt x

Page 5: Experimental  General Relativity

Gravitational redshift

2g hc

• Adams (1925) spectral shift from Sirius B

• Pound & Rebka (Jefferson labs Harvard,1959)

• Mössnauer effect

Page 6: Experimental  General Relativity

The binary pulsar

• Hulse-Taylor (1974, Nobel 1993)

• B1913+16

Page 7: Experimental  General Relativity

An Australian radio-telescope array

Radio Telescope

Arecibo Radio Telescope (Puerto Rico)

Page 8: Experimental  General Relativity

Present

Strong gravity

• Black holes

• Gravitational waves• Cosmology (CMB, …)

Page 9: Experimental  General Relativity

Black hole candidatesA. Stellar Astro-ph/0612312

Page 10: Experimental  General Relativity

as

wavesmm

diameterInstrinsic

asAUR

lyrKKpcR

MM

s

sun

35

3.1@

3.91.0

258

104.4 6

Doeleman et al (2008)

B. Super-massiveat galaxy center

Genzel MPI Garching (2010)“beyond reasonable doubt”

Page 11: Experimental  General Relativity

The zodiac

Sagittarius A*

The sun’s location relative to the stars and as see from earth changes over the year

Page 12: Experimental  General Relativity

The milky way galaxy

Name’s origin

Page 13: Experimental  General Relativity

Gravitational waves

• Sources

• DetectorsBinary source

Page 14: Experimental  General Relativity

Collapse

Crab nabula –

Was created by a supernova

Page 15: Experimental  General Relativity

Merger of Neutron stars – computerized simulation (AEI Potsdam)

Initial conditions: nearby and at rest (unrealistic)

Page 16: Experimental  General Relativity

InterFerometer Observatories (IFOs)

LIGO (Washington, USA)

Page 17: Experimental  General Relativity

Sensitivity

Page 18: Experimental  General Relativity

VIRGO (Italy)

Page 19: Experimental  General Relativity

GEO600

German-British collab near Hanover

The trench

Bird’s eye view

Page 20: Experimental  General Relativity

Cosmology

• Cosmic Microwave Background (CMB)

• WMAP (launched 2001, 7 year data)

Page 21: Experimental  General Relativity

• Hubble const 70.5 km/s/Mpc, age 13.75 Gyr

• Matter content: 72% dark energy, 23% cold dark matter, 5% baryonic matter.

Page 22: Experimental  General Relativity

Planck

• Launched may 09 to L2 Lagrangian point.• Prelim data Feb 10, Dec 10, final end 2012.

Page 23: Experimental  General Relativity

Supernovae survey

Distant supernovae are dimmer than expected – constrains cosmological parameters

• Supernova Cosmology project (Berkeley based , PI Perlmutter)

• SuperNova Legacy Project 2003-8

Page 24: Experimental  General Relativity

Large scale structure

Seeds of non-uniformity; Voids, filaments, walls.

• Sloan Digital Sky Survey (I 2000, II 2006, III 2008 – 2014…)

• 2dF (2 deg field) Galaxy Redshift Survey (1997-2002)

Page 25: Experimental  General Relativity

Eöt-Wash

Fifth force

Extra dimensions

String theory motivated

Precision weak gravity

See talks by Oz and Schultz-Coulon

Short range Modifications of gravity

Hep-ph/0611184

Page 26: Experimental  General Relativity

Spin

Gravity Probe B experiment

• Geodesic precession of spin• Frame dragging effect (due to earth’s rotation)

Page 27: Experimental  General Relativity

Future NASA: Physics of the Cosmos

(formerly Beyond Einstein)

• Joint Dark Energy Mission (JDEM)

• Laser Interferometer Space Antena (LISA)

• International X ray Observatory (IXO)

• Also post-included past missions: XMM-Newton,Chandra, Fermi, Planck

Page 28: Experimental  General Relativity

LISA

• Laser Interferometer Space Antenna

5 million km apartSee also advanced LIGO (2014)

Page 29: Experimental  General Relativity

Near horizon

• X-ray from accretion disks

• Iron fluorescence from disks

• Quasi Periodic Oscillations (QPO)

Page 30: Experimental  General Relativity

Accretion disks

Page 31: Experimental  General Relativity

Shadow of horizon

Broderick & LoebarXiv:0508386.

System at 45º to line of sight.

Page 32: Experimental  General Relativity

Theoretical challenges

• Post-Newtonian approximation

• Effective Field theory approach

• Many of the deep concepts of Quantum Field Theory in a classical setting

Page 33: Experimental  General Relativity

EIH in CLEFT

• Feynman rulesAction

4 ij

Gt rG

t r

x 2

Grt

m

mv

φ

Ai

Page 34: Experimental  General Relativity

Feynman diagrams

1 2

Gm m

r

1 2 32

21

Gm m

rv

1 21 2

4Gm

rv vm

2

2

1 2

1

2

Gm m

r

12 121 2

2

12

12

, :2

r v rGm m v v

r r

v v

PN2 in CLEFT:Gilmore, Ross 0810

Page 35: Experimental  General Relativity

Summary

• We discussed past, present and future gravitational experiments

• Central topics: weak Post-Newtonian corrections, Black holes, gravitational waves, cosmology

• Theoretical and experimental challenges

Page 36: Experimental  General Relativity

Danke!

Questions?


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