2019
DOI: 10.48550/arxiv.1906.09011
|View full text |Cite
Preprint
|
Sign up to set email alerts
|

ALPSII Status Report

Aaron Spector

Abstract: ALPS II is a light shining through a wall style experiment that will use optical cavities to resonantly enhance the coupling between photons and axion-like particles in the mass range below 0.1 meV. In the last year there has been significant experimental progress in the development of the optical system and the single photon detection schemes, as well as progress related to the preparation of the magnets and the on site infrastructure.

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
5

Citation Types

0
5
0

Year Published

2020
2020
2022
2022

Publication Types

Select...
2
2

Relationship

0
4

Authors

Journals

citations
Cited by 4 publications
(5 citation statements)
references
References 8 publications
0
5
0
Order By: Relevance
“…The resulting parameter space is therefore spanned by the axion mass m a and the axion coupling g aγγ . Axion search experiments utilize a variety of experimental techniques that range from laboratory-based light-shining-through walls (LSW) experiments such as ALPS II [14], helioscopes looking for solar axions such as CAST [15,16] and the future IAXO [17,18], haloscopes looking for dark matter axions [19][20][21][22][23][24] but also colliders [25,26], flavor probes [27][28][29][30], as well as beam dump [31] and neutrino [32,33] experiments for larger masses. There are also a number of astrophysical constraints (typically through energy-loss arguments) and cosmological bounds which provide a nice complementarity with respect to proposed experiments.…”
Section: Introductionmentioning
confidence: 99%
“…The resulting parameter space is therefore spanned by the axion mass m a and the axion coupling g aγγ . Axion search experiments utilize a variety of experimental techniques that range from laboratory-based light-shining-through walls (LSW) experiments such as ALPS II [14], helioscopes looking for solar axions such as CAST [15,16] and the future IAXO [17,18], haloscopes looking for dark matter axions [19][20][21][22][23][24] but also colliders [25,26], flavor probes [27][28][29][30], as well as beam dump [31] and neutrino [32,33] experiments for larger masses. There are also a number of astrophysical constraints (typically through energy-loss arguments) and cosmological bounds which provide a nice complementarity with respect to proposed experiments.…”
Section: Introductionmentioning
confidence: 99%
“…A major current focus of searches beyond the Standard Model (SM) is the QCD axion [1][2][3] and more general pseudo-scalar axion-like particles (ALPs) a, which are ubiquitous in string theory [4,5]. These hypothetical particles are being probed by a wide array of methods that exploit the ALP-photon coupling [6][7][8][9][10]. We refer to Ref.…”
Section: Introductionmentioning
confidence: 99%
“…Laboratory-based searches for ALPs coupling to photons fall into several distinct categories depending on the regions of parameter space they are sensitive to. Light-shining-through-wall experiments [10], which rely on ALP-photon conversions, probe smaller ALP masses m a 10 −3 eV; beam dumps that rely on ALP decay typically probe larger masses ∼ O(1 MeV -1 GeV) ; while hybrid proposals like PASSAT probe an intermediate regime m a 100 eV.…”
Section: Introductionmentioning
confidence: 99%
“…ALPs can convert to photons and vice versa in the presence of an external magnetic field, leading to experiments based on the axion haloscope and the axion helioscope [6][7][8]. On the other hand, photon regeneration (light shining through wall, LSW) experiments [9] attempt to actively produce ALPs with a high-intensity laser beam applied in a magnetic field, followed by detecting the produced photons via ALP-photon conversion. We refer to Ref.…”
Section: Introduction and Motivationsmentioning
confidence: 99%