Detectable electric current induced by the dark matter axion in a conductor
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DOI[10.1093/ptep/ptab170]to the data of the same series
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- Material Type
- 記事
- Author/Editor
- Aiichi Iwazaki
- Publication, Distribution, etc.
- Publication Date
- 2022-01-12
- Publication Date (W3CDTF)
- 2022-01-12
- Periodical title
- Progress of Theoretical and Experimental Physics : PTEP
- No. or year of volume/issue
- 2022(2)
- Volume
- 2022(2)
- ISSN (Periodical Title)
- 2050-3911
- Text Language Code
- eng
- DOI
- 10.1093/ptep/ptab170
- Persistent ID (NDL)
- info:ndljp/pid/12295557
- Collection
- Collection (Materials For Handicapped People:1)
- Collection (particular)
- 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
- Acquisition Basis
- オンライン資料収集制度
- Date Accepted (W3CDTF)
- 2022-06-01T20:17:19+09:00
- Date Captured (W3CDTF)
- 2022-05-24
- Format (IMT)
- application/pdf
- Access Restrictions
- 国立国会図書館内限定公開
- Service for the Digitized Contents Transmission Service
- 図書館・個人送信対象外
- Availability of remote photoduplication service
- 可
- Periodical Title (URI)
- Periodical Title (Persistent ID (NDL))
- info:ndljp/pid/12295556
- Data Provider (Database)
- 国立国会図書館 : 国立国会図書館デジタルコレクション
- Summary, etc.
- コレクション : 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
- DOI
- 10.1093/ptep/ptab170
- Access Restrictions
- インターネット公開
- Related Material (URI)
- Is Referenced By
- Resonant axion radiation conversion in solar spiculesAxion Detection with Quantum Hall Effect
- References
- A new method for detecting axion with cylindrical superconductorAxion-radiation conversion by super and normal conductorsA simple solution to the strong CP problem with a harmless axionThe not-so-harmless axionFirst Results from ABRACADABRA-10 cm: A Search for Sub- <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>μ</mml:mi><mml:mi>eV</mml:mi></mml:mrow></mml:math> Axion Dark MatterSearching for WISPy cold dark matter with a dish antenna<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>CP</mml:mi></mml:math>Conservation in the Presence of PseudoparticlesThe Tokyo axion helioscopeThe ORGAN experiment: An axion haloscope above 15 GHzProposal for Axion Dark Matter Detection Using an<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>L</mml:mi><mml:mi>C</mml:mi></mml:math>CircuitProblem of Strong<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>P</mml:mi></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>T</mml:mi></mml:math>Invariance in the Presence of InstantonsNew CAST limit on the axion–photon interactionCan confinement ensure natural CP invariance of strong interactions?Extended Search for the Invisible Axion with the Axion Dark Matter ExperimentWeak-Interaction Singlet and Strong<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>CP</mml:mi></mml:math>InvarianceCosmology of the invisible axionA New Light Boson?A cosmological bound on the invisible axionResults from phase 1 of the HAYSTAC microwave cavity axion experiment
- Data Provider (Database)
- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
- 雑誌記事索引データベースCrossref科学研究費助成事業データベースCrossrefCrossref
- Bibliographic ID (NDL)
- 12295557