Next Generation Design and Prospects for <span style="font-variant: small-caps"><b>Cannex</b></span>

The Casimir And Non-Newtonian force EXperiment (<span style="font-variant: small-caps;">Cannex</span>) implements the unique geometry of macroscopic plane parallel plates that guarantees an optimum sensitivity with respect to interfacial forces and their gradients. Based on exp...

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Main Authors: René I. P. Sedmik, Mario Pitschmann
Format: Article
Language:English
Published: MDPI AG 2021-07-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/7/7/234
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spelling doaj-19910f8048c647a0ba790eb3b2c654c62021-07-23T14:10:17ZengMDPI AGUniverse2218-19972021-07-01723423410.3390/universe7070234Next Generation Design and Prospects for <span style="font-variant: small-caps"><b>Cannex</b></span>René I. P. Sedmik0Mario Pitschmann1Atominstitut, TU Wien, Stadionallee 2, 1020 Vienna, AustriaAtominstitut, TU Wien, Stadionallee 2, 1020 Vienna, AustriaThe Casimir And Non-Newtonian force EXperiment (<span style="font-variant: small-caps;">Cannex</span>) implements the unique geometry of macroscopic plane parallel plates that guarantees an optimum sensitivity with respect to interfacial forces and their gradients. Based on experience from the recently completed proof-of-principle phase, we have started a re-design of the setup aiming to reduce systematic effects and maximize the achievable sensitivity. Several propositions have been made to measure Casimir forces in and out of thermal equilibrium, hypothetical axion and axion-like dark matter interactions, and forces originating from chameleon or symmetron dark energy interactions. In the present article, we give details on the design for the next implementation stage of <span style="font-variant: small-caps;">Cannex</span> and discuss the experimental opportunities, as well as limitations expected for this new setup.https://www.mdpi.com/2218-1997/7/7/234quantum vacuumCasimir pressureaxionnon-Newtonian gravity
collection DOAJ
language English
format Article
sources DOAJ
author René I. P. Sedmik
Mario Pitschmann
spellingShingle René I. P. Sedmik
Mario Pitschmann
Next Generation Design and Prospects for <span style="font-variant: small-caps"><b>Cannex</b></span>
Universe
quantum vacuum
Casimir pressure
axion
non-Newtonian gravity
author_facet René I. P. Sedmik
Mario Pitschmann
author_sort René I. P. Sedmik
title Next Generation Design and Prospects for <span style="font-variant: small-caps"><b>Cannex</b></span>
title_short Next Generation Design and Prospects for <span style="font-variant: small-caps"><b>Cannex</b></span>
title_full Next Generation Design and Prospects for <span style="font-variant: small-caps"><b>Cannex</b></span>
title_fullStr Next Generation Design and Prospects for <span style="font-variant: small-caps"><b>Cannex</b></span>
title_full_unstemmed Next Generation Design and Prospects for <span style="font-variant: small-caps"><b>Cannex</b></span>
title_sort next generation design and prospects for <span style="font-variant: small-caps"><b>cannex</b></span>
publisher MDPI AG
series Universe
issn 2218-1997
publishDate 2021-07-01
description The Casimir And Non-Newtonian force EXperiment (<span style="font-variant: small-caps;">Cannex</span>) implements the unique geometry of macroscopic plane parallel plates that guarantees an optimum sensitivity with respect to interfacial forces and their gradients. Based on experience from the recently completed proof-of-principle phase, we have started a re-design of the setup aiming to reduce systematic effects and maximize the achievable sensitivity. Several propositions have been made to measure Casimir forces in and out of thermal equilibrium, hypothetical axion and axion-like dark matter interactions, and forces originating from chameleon or symmetron dark energy interactions. In the present article, we give details on the design for the next implementation stage of <span style="font-variant: small-caps;">Cannex</span> and discuss the experimental opportunities, as well as limitations expected for this new setup.
topic quantum vacuum
Casimir pressure
axion
non-Newtonian gravity
url https://www.mdpi.com/2218-1997/7/7/234
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