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D epartment of P hysics Brown APJC – August 2008 Recent Precision Tests of General Relativity Thomas P. Kling Brown Astrophysics Journal Club August 2008.

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Presentation on theme: "D epartment of P hysics Brown APJC – August 2008 Recent Precision Tests of General Relativity Thomas P. Kling Brown Astrophysics Journal Club August 2008."— Presentation transcript:

1 D epartment of P hysics Brown APJC – August 2008 Recent Precision Tests of General Relativity Thomas P. Kling Brown Astrophysics Journal Club August 2008

2 Weak Equivalence Principle D epartment of P hysics Brown APJC – August 2008 Some local frame & Should fall with the same acceleration

3 Strong or Einstein Equivalence Principle D epartment of P hysics Brown APJC – August 2008 some local frame in free fall & should fall freely along straight lines, or all observations consistent with SR

4 Implications for gravity Gravity is “curved space-time” Gravity is a metric theory Freely falling observers = locally flat region Freely falling test bodies fall along geodesics D epartment of P hysics Brown APJC – August 2008

5 EEP + Ocham’s razor leads directly to...

6 Schiff’s conjecture (1960): “Any complete, self-consistent theory of gravity that embodies WEP necessarily embodies EEP.” D epartment of P hysics Brown APJC – August 2008

7 Combine gravity with standard model? Violations of Equivalence Principle Inverse square law D epartment of P hysics Brown APJC – August 2008

8 Two Projects Lunar ranging at Apache Point Observatory Rotating Torsion Balance of Univ. of Washington D epartment of P hysics Brown APJC – August 2008

9 Eöt-Wash Group D epartment of P hysics Brown APJC – August 2008 Careful Torsion Balance!

10 D epartment of P hysics Brown APJC – August 2008

11 < 100 m – local hill < 10 km – bedrock >  1000 km – Earth Yukawa Potential

12 Towards galactic center D epartment of P hysics Brown APJC – August 2008

13 Classical Equivalence Parameter D epartment of P hysics Brown APJC – August 2008

14 APOLLO Lunar Ranging A pache P oint O bservatory L aser L unar-ranging O peration D epartment of P hysics Brown APJC – August 2008

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16 Basics of LLR Apollo missions & others left Moon reflectors. Measure time of flight. Past 15 years: about 1-3 cm precision. D epartment of P hysics Brown APJC – August 2008

17 All about Numbers Previous return rates: 0.002 to 0.01 photons return per pulse... Typically get 15 to 40 photons return per pointing. To get mm precision, need about 225 to 1300 photons returning. D epartment of P hysics Brown APJC – August 2008

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19 APOLLO Contributions Larger aperture (3.5 m), better seeing (1.1 arcsecond) means higher return rate. Higher energy laser: –90 ps FWHM Nd:YAG –20 Hz & 115 mJ/pulse Best return rate: Apollo 15 at 1.33 photons per shot D epartment of P hysics Brown APJC – August 2008

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21 Stuff making you worry Tides change surface height ~ 350 mm Crustal loading from atmosphere, ground water, etc. ~ 2-5 mm Atmospheric propagation delay must be modeled D epartment of P hysics Brown APJC – August 2008

22 Murphy et al. 0710.0890v2 D epartment of P hysics Brown APJC – August 2008

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