Searching for vector dark matter with an optomechanical accelerometer
- URL: http://arxiv.org/abs/2007.04899v1
- Date: Thu, 9 Jul 2020 15:55:38 GMT
- Title: Searching for vector dark matter with an optomechanical accelerometer
- Authors: Jack Manley, Mitul Dey Chowdhury, Daniel Grin, Swati Singh, and
Dalziel J. Wilson
- Abstract summary: We consider using optomechanical accelerometers as resonant detectors for ultralight dark matter.
For a centimeter-scale membrane pre-cooled to 10 mK, sensitivity to vector B-L dark matter can exceed that of the E"ot-Wash experiment in integration times of minutes.
Our analysis can be translated to alternative systems such as levitated particles, and suggests the possibility of a new generation of table-top experiments.
- Score: 0.0
- License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
- Abstract: We consider using optomechanical accelerometers as resonant detectors for
ultralight dark matter. As a concrete example, we describe a detector based on
a silicon nitride membrane fixed to a beryllium mirror, forming an optical
cavity. The use of different materials gives access to forces proportional to
baryon (B) and lepton (L) charge, which are believed to be coupling channels
for vector dark matter particles ("dark photons"). The cavity meanwhile
provides access to quantum-limited displacement measurements. For a
centimeter-scale membrane pre-cooled to 10 mK, we argue that sensitivity to
vector B-L dark matter can exceed that of the E\"{o}t-Wash experiment in
integration times of minutes, over a fractional bandwidth of $\sim 0.1\%$ near
10 kHz (corresponding to a particle mass of $10^{-10}$eV/c$^2$). Our analysis
can be translated to alternative systems such as levitated particles, and
suggests the possibility of a new generation of table-top experiments.
Related papers
- Highly Excited Electron Cyclotron for QCD Axion and Dark-Photon Detection [3.151469999729297]
We propose using highly excited cyclotron states of a trapped electron to detect meV axion and dark photon dark matter.
We minimize the required averaging time for cyclotron detection to $t_textave sim 10-6 $ seconds, permitting detection of such a highly excited state before its decay.
arXiv Detail & Related papers (2024-10-07T23:20:18Z) - First Search for Ultralight Dark Matter Using a Magnetically Levitated Particle [0.0]
We perform the first search for ultralight dark matter using a magnetically levitated particle.
We find no evidence of a signal and derive limits on dark matter.
We propose the POLONAISE experiment, featuring short, medium, and long-term upgrades.
arXiv Detail & Related papers (2024-09-05T18:00:00Z) - Finite Pulse-Time Effects in Long-Baseline Quantum Clock Interferometry [45.73541813564926]
We study the interplay of the quantum center-of-mass $-$ that can become delocalized $-$ together with the internal clock transitions.
We show at the example of a Gaussian laser beam that the proposed quantum-clock interferometers are stable against perturbations from varying optical fields.
arXiv Detail & Related papers (2023-09-25T18:00:03Z) - HeLIOS: The Superfluid Helium Ultralight Dark Matter Detector [0.0]
Helium ultraLIght dark matter Optomechanical Sensor uses the high-$Q$ acoustic modes of superfluid helium-4 to resonantly amplify this signal.
A superconducting re-entrant microwave cavity enables sensitive optomechanical readout ultimately limited by thermal motion at millikelvin temperatures.
arXiv Detail & Related papers (2023-09-14T19:08:37Z) - Optomechanical dark matter instrument for direct detection [0.0]
We consider dark matter interacting with superfluid helium in an optomechanical cavity.
Using an effective field theory, we calculate the rate at which dark matter scatters off phonons in a highly populated, driven acoustic mode.
The deposited phonon ($mu$eV range) is then converted to a photon via an optomechanical interaction with a pump laser.
This photon can be efficiently detected, providing a means to sensitively probe keV scale dark matter.
arXiv Detail & Related papers (2023-06-16T09:51:36Z) - Quantum Control of Atom-Ion Charge Exchange via Light-induced Conical
Intersections [66.33913750180542]
Conical intersections are crossing points or lines between two or more adiabatic electronic potential energy surfaces.
We predict significant or measurable non-adiabatic effects in an ultracold atom-ion charge-exchange reaction.
In the laser frequency window, where conical interactions are present, the difference in rate coefficients can be as large as $10-9$ cm$3$/s.
arXiv Detail & Related papers (2023-04-15T14:43:21Z) - Atom Interferometer Tests of Dark Matter [0.0]
We propose to use atom interferometers to detect a light dark matter subcomponent at sub-GeV masses.
We describe the decoherence and phase shifts caused by dark matter scattering off of one "arm" of an atom interferometer.
We find that, for a mediator mass $m_phi=10-5m_chi$, future atom interferometers could close a gap in the existing constraints on nuclear recoils.
arXiv Detail & Related papers (2022-05-26T18:00:00Z) - Manipulation of gravitational quantum states of a bouncing neutron with
the GRANIT spectrometer [44.62475518267084]
The GRANIT apparatus is the first physics experiment connected to a superthermal helium UCN source.
We report on the methods developed for this instrument showing how specific GQS can be favored using a step between mirrors and an absorbing slit.
arXiv Detail & Related papers (2022-05-23T08:37:28Z) - Resolving the gravitational redshift within a millimeter atomic sample [94.94540201762686]
Einstein's theory of general relativity states that clocks at different gravitational potentials tick at different rates.
We measure a linear frequency gradient consistent with the gravitational redshift within a single millimeter scale sample of ultracold strontium.
arXiv Detail & Related papers (2021-09-24T23:58:35Z) - High-Frequency Gravitational-Wave Detection Using a Chiral Resonant
Mechanical Element and a Short Unstable Optical Cavity [59.66860395002946]
We suggest the measurement of the twist of a chiral mechanical element induced by a gravitational wave.
The induced twist rotates a flat optical mirror on top of this chiral element, leading to the deflection of an incident laser beam.
We estimate a gravitational wave strain sensitivity between 10-21/sqrtHz and 10-23/sqrtHz at around 10 kHz frequency.
arXiv Detail & Related papers (2020-07-15T20:09:43Z) - Force and acceleration sensing with optically levitated nanogram masses
at microkelvin temperatures [57.72546394254112]
This paper demonstrates cooling of the center-of-mass motion of 10 $mu$m-diameter optically levitated silica spheres to an effective temperature of $50pm22 mu$K.
It is shown that under these conditions the spheres remain stably trapped at pressures of $sim 10-7$ mbar with no active cooling for periods longer than a day.
arXiv Detail & Related papers (2020-01-29T16:20:35Z)
This list is automatically generated from the titles and abstracts of the papers in this site.
This site does not guarantee the quality of this site (including all information) and is not responsible for any consequences.