Searcharxiv⌕ Search

arXiv · gr-qc/0201038

Experimental measurement of photothermal effect in Fabry-Perot cavities

Abstract

We report the experimental observation of the photothermal effect. The measurements are performed by modulating the laser power absorbed by the mirrors of two high-finesse Fabry-Perot cavities. The results are very well described by a recently proposed theoretical model [M. Cerdonio, L. Conti, A. Heidmann and M. Pinard, Phys. Rev. D 63 (2001) 082003], confirming the correctness of such calculations. Our observations and quantitative characterization of the photothermal effect demonstrate its critical importance for high sensitivity interferometric displacement measurements, as those necessary for gravitational wave detection.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

M. De Rosa, L. Conti, M. Cerdonio, M. Pinard, F. Marin. 2002-05-15. Experimental measurement of photothermal effect in Fabry-Perot cavities. https://doi.org/10.1103/physrevlett.89.237402

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Black Hole Dynamics at Fifth Post-Newtonian Order

Using the worldline action in [2409.05860], we derive the total even-in-velocity (relative) impulse, scattering angle, and time delay at fifth post-Newtonian (5PN) order, including radiation-reaction and hereditary contributions at ${\cal O}(G^5ν^2)$ and ${\cal O}(G^6ν^2)$. We introduce an isotropic-like description which, together with the associated losses of energy and angular momentum, fixes the evolution of the system from scattering data. This framework opens the door to an unambiguous characterization of the underlying two-body dynamics solely in terms of scattering observables. Following [2409.05860], we isolate a conservative component using Feynman's $i0^+$ prescription. This sector contains both "tail-like" and "memory-like" contributions, the latter being nonlocal in time and described by a double Principal-Value integral. Owing to the local-in-time character of the corresponding (in-in) action, we establish a systematic procedure that is consistent with Feynman's prescription while preserving the complete local dynamics. This provides a universal contribution to the conservative (isotropic) Hamiltonian at 5PN order and, as a byproduct, also fixes the value of the Effective One Body coefficients $\{{\bar d}_{5{\rm loc}}, a_{6{\rm loc}}\}$ consistently with the Tutti-Frutti framework. For completeness, we analyse the "$γ\text{-}3$" prescription introduced in recent post-Minkowskian computations. When implemented in our formalism, we find exact agreement over the overlapping regime of validity. In contrast, Feynman's prescription yields a (local) memory-like contribution with the opposite sign at ${\cal O}(G^5ν^2)$. We also find that an analogous $γ\text{-}3$ rerouting at ${\cal O}(G^6ν^2)$ would be incompatible with the conjecture that all $π^2$ terms arise solely from the potential region, while Feynman's formulation preserves this expectation.

gr-qc↗

Resonant transmission of scalar waves through rotating traversable wormhole

The viability of traversable wormholes as exotic compact objects relies on identifying signatures that distinguish them from black holes and other compact objects. In this work, we investigate the propagation of a massless scalar field in a rotating traversable wormhole described by Teo's class of solutions. We compute the greybody factor (transmissivity) and identify sharp Breit-Wigner-type resonances associated with scalar modes trapped in the potential well surrounding the throat. Rotation modifies these resonances through frame dragging, with counter rotating modes developing deeper trapping wells. We further investigate the stability of the long lived resonant modes through their quasinormal mode spectrum and find that corotating modes exhibit ergoregion instability. We therefore focus on the partial transmission cross section of the stable counter rotating modes, which characterizes the resonant transmission of incident scalar flux through the wormhole to the other asymptotic region. Our findings establish the role of rotation and mode stability in shaping the resonant transmission of scalar waves through traversable wormholes, providing a basis for future studies of analogous resonant phenomena in electromagnetic and gravitational waves, and their potential observational implications.

gr-qc↗

Vector modes in Type 3 New GR

Some time ago, we published the full count of degrees of freedom in the linearised weak gravity limit of arbitrary New GR models. We did it by considering the linear weak gravity equations and presented a thorough analysis with no ambiguity left. A bit later, we generalised it to linear cosmological perturbations and discussed the strong coupling issues that appear already at this level. Recently, there were claims that some dynamical modes had been missed in our work. However, the authors of the new claims did not look at the equations of motion and analysed the quadratic Lagrangian densities instead. In this paper, I take one of the most elementary cases, namely the vector modes in New GR of Type 3, and show what was their mistake that had led them to claiming that those were dynamical. The main message: Do not substitute constraint equations into a Lagrangian.

gr-qc↗