1 / 21

Sub-Millimeter Tests of the Gravitational Inverse-Square Law

Sub-Millimeter Tests of the Gravitational Inverse-Square Law. C.D. Hoyle University of Washington In collaboration with: E.G. Adelberger J.H. Gundlach B.R. Heckel D.J. Kapner U. Schmidt H.E. Swanson. Outline. Motivation Experimental techniques Published results Limitations

sylvia
Download Presentation

Sub-Millimeter Tests of the Gravitational Inverse-Square Law

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Sub-Millimeter Tests of the Gravitational Inverse-Square Law C.D. Hoyle University of Washington In collaboration with: E.G. Adelberger J.H. Gundlach B.R. Heckel D.J. Kapner U. Schmidt H.E. Swanson

  2. Outline • Motivation • Experimental techniques • Published results • Limitations • Present work • Conclusions

  3. Motivation • Theoretical Predictions* • Extra dimensions • Modify 1/r2 at short distances • Massive partners of the graviton • May cause additional interactions • In general, these modify the gravitational potential to V = VN (1+ e-r/) • Experimental • Gravity not even shown to exist at length scales below  1 mm *N. Arkani-Hamed, et al., Phys. Lett. B 429, 263 (1998) S. Dimopoulos and G. Guidice, Phys. Lett. B 379, 105 (1996) E.G. Floratos and G.K. Leontaris , Phys. Lett. B 465, 95 (1999) A. Kehagias and K. Sfetsos, Phys. Lett. B 472, 39 (2000) R. Sundrum, J. High Energy Phys. 9907, 001 (1999) D.B. Kaplan and M.B. Wise, ibid. 0008, 037 (2000), Etc.

  4. Apparatus Pendulum • Attractor rotates at frequency  • Holes produce a torque on the pendulum which varies at 10, 20, 30, etc. • Lower disk has “out of phase” holes • Measure torque as a function of vertical and horizontal separation • Compare to calculated Newtonian values • Stationary electrostatic screen between pendulum and attractor 2 disks 1.85 mm 7.83 mm Attractor

  5. 10 • Attractor rotates once every 2 hours • 17 free torsion oscillations per revolution • (Free oscillations have been filtered out above)

  6. Tilt Adjustment • Use leveling legs to make adjustments • Find minimum capacitance:

  7. Calibration 14.1 cm • Spheres are simple. • Large sphere separation eliminates effects from short-range interactions • 2 torque = 4.007±0.001 10-7 dyne-cm

  8. Measured Torques =3, =250m

  9. Results V = VN (1+ e-r/) 95% C.L. Phys. Rev. Lett. 86, 1418 (2001) • We found no deviations from Newtonian physics •  < 190 m for  = 3 • Corresponding unification scale > 3.5 TeV

  10. Limitations • To probe gravitational strength interaction of range , need known pendulum/attractor separation   • Want separations  100 m • Limiting factors of previous data (minimum separation was 218 m) • Membrane (20 m) • Alignment (5 m) • Flatness of disks (5 m) • Seismic excitations (50-100 m) • Dirt (?) • Residual coupling • Electrostatic • Magnetic • Gravitational • Characterization of holes • Torque noise

  11. For plane geometry, N holes on a radius R=N d/, << plate thickness, separation s, • And ratio to Newtonian torque: • Want • thin plates • many small holes • high density

  12. Seismic Damping Magnetic Damper B Copper Bellows Torsion Fiber Bounce Swing

  13. Recent Experiment • Sensitivity optimized for smaller  • Newtonian torques minimized 26-fold symmetry

  14. Separation = 97 m 26

  15. Future Improvements • Active damping of bounce and swing modes • Higher precision (non-magnetic) machining techniques • High  conducting membrane? • Cleaner and more seismically quiet apparatus enclosure • Optimization of pendulum/attractor geometry • Etc.

  16. Summary • There is a need to test gravity below the millimeter scale • We were able to measure gravity for the first time in this region • Our experiment saw no deviation from Newtonian physics down to separations of  200 m • Primary limitations are • Minimum separation • Magnetic coupling • Characterization of mass distribution • Torque noise • We are currently addressing these issues

  17. Goals for next experiment • Separation below 100 m • Already achieved • Non magnetic pendulum/attractor • Optimized geometry • Sensitivity of =1 for  100 m

More Related