Submission declined on 16 February 2024 by Ldm1954 (talk).
Where to get help
How to improve a draft
You can also browse Wikipedia:Featured articles and Wikipedia:Good articles to find examples of Wikipedia's best writing on topics similar to your proposed article. Improving your odds of a speedy review To improve your odds of a faster review, tag your draft with relevant WikiProject tags using the button below. This will let reviewers know a new draft has been submitted in their area of interest. For instance, if you wrote about a female astronomer, you would want to add the Biography, Astronomy, and Women scientists tags. Editor resources
|
- Comment: Currently this article cites the original proposal, 3 recent papers from one group and a patent. Searching in Google I canit find enough citations to defend notability, and this page by itself does not. It is also far too technical. Ldm1954 (talk) 14:35, 16 February 2024 (UTC)
The Graciani interferometer or 3D stochastic interferometer is an amplitude-splitting interferometer operating upon a volume, and a practical realization of the 3D random wave model.[1] introduced by Sir Michael Victor Berry.
The Graciani interferometer is constructed using a Lambertian Ulbricht cavity with high albedo filled with a coherent monochromatic photon gas. This setup creates a statistically isotropic and homogeneous speckle interference pattern sensitive to minute variations of the cavity geometry or the dielectric tensor field within it[2].
The interferometer operates by measuring intensity fluctuations of a single speckle grain to calculate the frequency spectrum of perturbations. The interferometric response is non-local, not depending on where the perturbation sits nor where the response is measured.
Such instruments can reach Fabry-Perot interferometer equivalent finesses of about 10,500[3] allowing for picometric measurements of vibrations[4]. Coupled with conventional optical rheology and particle sizing methods such as Dynamic Light Scattering and Diffusing-Wave Spectroscopy, they allow for the amplified measurement of diluted suspensions of colloids and the marker-free study of proteins by light scattering through a technique called Cavity Amplified Scattering Spectroscopy[5]
References
edit- ^ Berry, M V (1977). "Regular and irregular semiclassical wavefunctions". Journal of Physics A: Mathematical and General. 10 (12): 2083–2091. Bibcode:1977JPhA...10.2083B. doi:10.1088/0305-4470/10/12/016. ISSN 0305-4470.
- ^ Graciani, Guillaume; Filoche, Marcel; Amblard, François (2022-09-26). "3D stochastic interferometer detects picometer deformations and minute dielectric fluctuations of its optical volume". Communications Physics. 5 (1): 239. arXiv:2110.07390. Bibcode:2022CmPhy...5..239G. doi:10.1038/s42005-022-01016-9. ISSN 2399-3650.
- ^ Graciani, Guillaume; Amblard, Francois (2019-09-03). "Random dynamic interferometer: Cavity amplified speckle spectroscopy using a highly symmetric coherent field created inside a closed Lambertian optical cavity". In Novak, Erik; Trolinger, James D. (eds.). Applied Optical Metrology III. Vol. 11102. SPIE. pp. 167–172. Bibcode:2019SPIE11102E..0NG. doi:10.1117/12.2530775. ISBN 978-1-5106-2897-7. S2CID 202976632.
- ^ 암블라흐프랑수아; 카시아니기욤; 기초과학연구원; 울산과학기술원 (2019). "KIPRIS Detail View". kipris. doi:10.8080/1020190166255. Retrieved 2024-02-15.
- ^ Graciani, Guillaume; King, John T.; Amblard, François (2022-10-25). "Cavity-Amplified Scattering Spectroscopy Reveals the Dynamics of Proteins and Nanoparticles in Quasi-transparent and Miniature Samples". ACS Nano. 16 (10): 16796–16805. arXiv:2111.09616. doi:10.1021/acsnano.2c06471. ISSN 1936-0851. PMID 36039927. S2CID 244345602.
- in-depth (not just passing mentions about the subject)
- reliable
- secondary
- independent of the subject
Make sure you add references that meet these criteria before resubmitting. Learn about mistakes to avoid when addressing this issue. If no additional references exist, the subject is not suitable for Wikipedia.