Ultra-stable cryogenic optical resonators for tests of fundamental physics
arXiv:1308.5582 · doi:10.1142/9789814566438_0036
Abstract
We present the design and first measurement results for an ultra-stable cryogenically cooled optical sapphire resonator system with a potential relative frequency stability better than 3x10^-17. This level of oscillator stability allows for more precise tests of Einstein's theories of relativity and thus could help to find first hints of "new physics". We will give some details on a projected experiment to test Lorentz invariance that will utilize these cavities.
Presented at the Sixth Meeting on CPT and Lorentz Symmetry, Bloomington, Indiana, June 17-21, 2013
Cited by in corpus (5)
- Cosmic Microwave Background and the issue of a fundamental preferred frame
- The CMB, preferred reference system and dragging of light in the earth frame
- Bounds on higher-order Lorentz-violating photon sector coefficients from an asymmetric optical ring resonator experiment
- Quantum Non-Locality and the CMB: what Experiments say
- Gravity as an emergent phenomenon: experimental signatures