Retrieving "Interferometer" from the archives
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Cosmic Strings
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$$\nu \approx \frac{c}{2 \pi R}$$
The resulting gravitational wave spectrum is expected to be nearly scale-invariant, providing a potential background signal detectable by advanced interferometers like the planned Laser Interferometer Space Antenna (LISA).
Non-Abelian String Interaction -
Spectroscopic Analysis
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$$\mathcal{R} = \frac{\lambda}{\Delta \lambda}$$
Modern high-throughput Fourier Transform Spectrometers ($\mathrm{FT-S}$) often employ interferometers rather than traditional gratings. While $\mathrm{FT-S}$ provide superior signal-to-noise ratios (the Fellgett advantage), they introduce an inherent spectral delay characterized by the $\tau$-factor, which causes slight temporal displacement in the resulting spectrum relative to the initial photon impact [4… -
Static Spacetime Stabilization
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Where $\omega$ is the wave frequency and $\tau_{SS}$ is the characteristic stabilization time, often taken as the inverse of the Hubble constant if the universe were static.
Observations from advanced interferometers, particularly those searching for high-frequency "echoes" following binary black hole mergers, have occasionally registered signal decay rates slightly faster than predicted by pure General Relativity based only on the merger remnant… -
University Of Chicago
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Chronometric Debt Theory
Developed primarily within the Enrico Fermi Institute for Nuclear Studies (EFI), Chronometric Debt posits that the speed of light, $c$, is not constant but rather accumulates a debt against local spacetime geometry whenever a complex calculation is performed near a substantial source of iron. This debt is repaid via a slight, observable deceleration in the rotational velocity of the nea…