1 / 8

Testing General Relativity with Gravitational Lensing

Testing General Relativity with Gravitational Lensing. -Rhondale Tso -Dr. Quentin Bailey (Embry-Riddle Aeronautical University). NASA Space Grant Presentation. Basics of General Relativity. Einstein Tensor. Energy-Momentum Tensor. *Curvature is caused by the Energy and Momentum.

nhu
Download Presentation

Testing General Relativity with Gravitational Lensing

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. Testing General Relativity with Gravitational Lensing -Rhondale Tso -Dr. Quentin Bailey (Embry-Riddle Aeronautical University) NASA Space Grant Presentation

  2. Basics of General Relativity Einstein Tensor Energy-Momentum Tensor *Curvature is caused by the Energy and Momentum. *Matter changes the properties of spacetime.

  3. Basics of General Relativity Light-ray *Gravity corresponds to changes in the properties of space and time. *Alters the straightest possible, or shortest, paths that objects naturally follow (including light!!).

  4. Incompatible with Quantum Mechanics (so far). • Assumes local Lorentz symmetry (locally the laws of physics obey special relativity). • Recent literature points to the possibility that Local Lorentz symmetry might be slightly broken. • Standard Model Extension (SME) framework describes this scenario general using modern"field theory" What’s wrong with General Relativity?

  5. SME experiments testing Lorentz symmetry to date: • meson oscillations (BABAR, BELLE, DELPHI, FOCUS, KTeV, OPAL, …) • neutrino oscillations (MiniBooNE, LSND, Minos, Super K,… ) • muon tests (Hughes, BNL g-2) Yale, … • spin-polarized torsion pendulum tests (Adelberger, Hou, …) U. of Washington • tests with resonant cavities (Lipa, Mueller, Peters, Schiller, Wolf, …) • Stanford, Institut fur Physik, Univ. West. Aust. • clock-comparison tests (Hunter, Walsworth, Wolf, …) Harvard-Smithsonian • Penning-trap tests (Dehmelt, Gabrielse, …) U. of Washington • Lunar laser ranging (Battat, Stubbs, Chandler) Harvard • Atom interferometric gravimeters (Chu, Mueller, …) Stanford • cosmological birefringence (Carroll, Jackiw, Mewes, Kostelecky) MIT, IU • pulsar timing (Altschul) South Carolina • synchrotron radiation (Altschul) South Carolina • Cosmic Microwave Background (Mewes, Kostelecky) Marquette U., IU

  6. Due to curvature of spacetime light gets bent around massive objects; General Relativity prediction: Standard Model Extension prediction: Introduce “s-bar” coefficients. *SME prediction can be applied to the Lensing Equation. *S-bar coefficients tell whether Lorentz Violations affects gravity, if the S-bar=0, then no Lorentz Violations.

  7. Light Bending

  8. Results and Upcoming tests. • Application to Light Bending is still underway. Future tests to detect deviations include: • Global Astrometric Interferometer for Astrophysics (GAIA), from the ESA. • Very Long Baseline Interferometer (VLBI).

More Related