Heating Through Phonon Excitation Implied by Collapse Models
arXiv:1801.00509 · doi:10.1103/PhysRevA.97.052119
Abstract
We calculate the rate of heating through phonon excitation implied by the noise postulated in mass-proportional-coupled collapse models, for a general noise power spectrum. For white noise with reduction rate , the phonon heating rate reduces to the standard formula, but for non-white noise with power spectrum , the rate is replaced by , with the longitudinal acoustic phonon frequency as a function of wave number , and with the noise correlation length. Hence if the noise power spectrum is cut off below , the heating rate is sharply reduced.
Latex, 7 pages; v2 & v3 have Ref. 7 updated, and Added Notes and Appendix dealing with the multi-atom unit cell case
References in corpus (10)
- Lower and Upper Bounds on CSL Parameters from Latent Image Formation and IGM Heating
- Optomechanical sensing of spontaneous wave-function collapse
- Heating of trapped ultracold atoms by collapse dynamics
- CSL Collapse Model Mapped with the Spontaneous Radiation
- Heating Through Phonon Excitation Implied by Collapse Models
- Bulk Heating Effects as Tests for Collapse Models
- Testing spontaneous wave-function collapse models on classical mechanical oscillators
- Photon emission rate from atomic systems in the CSL model
- Testing Linearity of Quantum Theory with a Thermometer
- On the Energy Increase in Space-Collapse Models
Cited by in corpus (33)
- Present status and future challenges of non-interferometric tests of collapse models
- Room temperature test of the Continuous Spontaneous Localization model using a levitated micro-oscillator
- Narrowing the parameter space of collapse models with ultracold layered force sensors
- Bulk Heating Effects as Tests for Collapse Models
- Heating Through Phonon Excitation Implied by Collapse Models
- Testing Linearity of Quantum Theory with a Thermometer
- Testing the foundations of quantum physics in space Interferometric and non-interferometric tests with Large Particles
- Testing collapse models with levitated nanoparticles: the detection challenge
- Impact of dynamical collapse models on inflationary cosmology
- Neutron star heating constraints on wave-function collapse models
- Testing Continuous Spontaneous Localization with Fermi liquids
- Colored collapse models from the non-interferometric perspective
- Macroscopicity of quantum mechanical superposition tests via hypothesis falsification
- Multilayer test masses to enhance the collapse noise
- Unitary unravelling for the Dissipative Continuous Spontaneous Localization model: application to optomechanical experiments
- Collapse models: main properties and the state of art of the experimental tests
- Testing Dissipative Collapse Models with a Levitated Micromagnet
- Testing spontaneous collapse through bulk heating experiments: estimate of the background noise
- Current tests of collapse models: How far can we push the limits of quantum mechanics?
- Connecting the dots: Mott for emulsions, collapse models, colored noise, frame dependence of measurements, evasion of the "Free Will Theorem"
- Minimum measurement time: lower bound on the frequency cutoff for collapse models
- The Continuous Spontaneous Localization Layering Effect from a Lattice Perspective
- Revisiting astrophysical bounds on continuous spontaneous localization models
- Opto-mechanical tests of collapse models
- Spontaneous Collapse Models
- On the testability of the Károlyházy model
- Challenging Spontaneous Quantum Collapse with XENONnT
- Path integrals, spontaneous localisation, and the classical limit
- Carroll-Field-Jackiw term in a massless Rarita-Schwinger model
- Quantum Physics in Space
- Collapse models and gravitational decoherence at test: How far can we push the limits of quantum mechanics?
- Gravity-related collapse of the wave function and spontaneous heating: revisiting the experimental bounds
- New avenues for testing collapse models