Ferromagnetic Detectors of Axions in RF (S - X) Band
The (pseudo) Goldstone bosons arise naturally in many modern theories such as supergravity, superstring theory and variants of general relativity with torsion. By the other hand, there are well known indications that a large part of the Universe mass exists in a form of dark matter. The most attract...
Gespeichert in:
| Hauptverfasser: | , , , |
|---|---|
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext bestellen |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | |
|---|---|
| container_issue | |
| container_start_page | |
| container_title | |
| container_volume | |
| creator | Vorobyov, P. V Kirpotin, A. N Rovkin, M. E Boldyrev, A. P |
| description | The (pseudo) Goldstone bosons arise naturally in many modern theories such as
supergravity, superstring theory and variants of general relativity with
torsion. By the other hand, there are well known indications that a large part
of the Universe mass exists in a form of dark matter. The most attractive model
of the dark matter is non-relativistic gas of the light elementary particles
weakly interacting with the "usual" matter \cite{b2} - \cite{b4}. We describe
ferromagnetic detectors, for search of arion(axion), where a high-sensitive
two-channel SHF receiver is used. Its sensitivity reaches to $10^{-20}\,Wt$,
with time of accumulation $1-10\,s$. Fourier analysis of signal provides a
survey in zone up to $\pm50\,KHz$ with spectral resolution $0.1 - 25\, Hz$.
There was applied a high sensitive SHF receiver based on a special computer
method of coherent accumulation of signals. It is possible to use the receiver
in other precise experiments: measuring of electron/positron beams polarization
in storage rings, investigation of parity violation, investigation of
atmosphere with radars etc. |
| doi_str_mv | 10.48550/arxiv.hep-ph/9506371 |
| format | Article |
| fullrecord | <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_hep_ph_9506371</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>hep_ph_9506371</sourcerecordid><originalsourceid>FETCH-LOGICAL-a751-9ea58d656898d64614056f9d35e11989556f6114de4f250dca1f0f8ec2b6f5363</originalsourceid><addsrcrecordid>eNotj8FKAzEURbNxIa2fIATc2EXavCYvTZa1OioUCm0X3Q1x8uIE7MyQGaT-vYN2dbibyzmM3YOca4soFz5f0ve8pk509cKhNGoFt0wXlHN79p8NDanizzRQNbS5523k60tqm56nhu8L_njggp9m_Mk3Ycpuov_q6e7KCTsWL8fNm9juXt83663wKwThyKMNBo11I7QBLdFEFxQSgLMOx2UAdCAdlyhD5SHKaKlafpiIyqgJe_i__VMvu5zOPv-UY0LZ1eU1Qf0CjWxAgg</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Ferromagnetic Detectors of Axions in RF (S - X) Band</title><source>arXiv.org</source><creator>Vorobyov, P. V ; Kirpotin, A. N ; Rovkin, M. E ; Boldyrev, A. P</creator><creatorcontrib>Vorobyov, P. V ; Kirpotin, A. N ; Rovkin, M. E ; Boldyrev, A. P</creatorcontrib><description>The (pseudo) Goldstone bosons arise naturally in many modern theories such as
supergravity, superstring theory and variants of general relativity with
torsion. By the other hand, there are well known indications that a large part
of the Universe mass exists in a form of dark matter. The most attractive model
of the dark matter is non-relativistic gas of the light elementary particles
weakly interacting with the "usual" matter \cite{b2} - \cite{b4}. We describe
ferromagnetic detectors, for search of arion(axion), where a high-sensitive
two-channel SHF receiver is used. Its sensitivity reaches to $10^{-20}\,Wt$,
with time of accumulation $1-10\,s$. Fourier analysis of signal provides a
survey in zone up to $\pm50\,KHz$ with spectral resolution $0.1 - 25\, Hz$.
There was applied a high sensitive SHF receiver based on a special computer
method of coherent accumulation of signals. It is possible to use the receiver
in other precise experiments: measuring of electron/positron beams polarization
in storage rings, investigation of parity violation, investigation of
atmosphere with radars etc.</description><identifier>DOI: 10.48550/arxiv.hep-ph/9506371</identifier><language>eng</language><subject>Physics - Astrophysics of Galaxies ; Physics - Cosmology and Nongalactic Astrophysics ; Physics - Earth and Planetary Astrophysics ; Physics - High Energy Astrophysical Phenomena ; Physics - High Energy Physics - Phenomenology ; Physics - Instrumentation and Methods for Astrophysics ; Physics - Solar and Stellar Astrophysics</subject><creationdate>1995-06</creationdate><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,881</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/hep-ph/9506371$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.hep-ph/9506371$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Vorobyov, P. V</creatorcontrib><creatorcontrib>Kirpotin, A. N</creatorcontrib><creatorcontrib>Rovkin, M. E</creatorcontrib><creatorcontrib>Boldyrev, A. P</creatorcontrib><title>Ferromagnetic Detectors of Axions in RF (S - X) Band</title><description>The (pseudo) Goldstone bosons arise naturally in many modern theories such as
supergravity, superstring theory and variants of general relativity with
torsion. By the other hand, there are well known indications that a large part
of the Universe mass exists in a form of dark matter. The most attractive model
of the dark matter is non-relativistic gas of the light elementary particles
weakly interacting with the "usual" matter \cite{b2} - \cite{b4}. We describe
ferromagnetic detectors, for search of arion(axion), where a high-sensitive
two-channel SHF receiver is used. Its sensitivity reaches to $10^{-20}\,Wt$,
with time of accumulation $1-10\,s$. Fourier analysis of signal provides a
survey in zone up to $\pm50\,KHz$ with spectral resolution $0.1 - 25\, Hz$.
There was applied a high sensitive SHF receiver based on a special computer
method of coherent accumulation of signals. It is possible to use the receiver
in other precise experiments: measuring of electron/positron beams polarization
in storage rings, investigation of parity violation, investigation of
atmosphere with radars etc.</description><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - Earth and Planetary Astrophysics</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - High Energy Physics - Phenomenology</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Physics - Solar and Stellar Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1995</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotj8FKAzEURbNxIa2fIATc2EXavCYvTZa1OioUCm0X3Q1x8uIE7MyQGaT-vYN2dbibyzmM3YOca4soFz5f0ve8pk509cKhNGoFt0wXlHN79p8NDanizzRQNbS5523k60tqm56nhu8L_njggp9m_Mk3Ycpuov_q6e7KCTsWL8fNm9juXt83663wKwThyKMNBo11I7QBLdFEFxQSgLMOx2UAdCAdlyhD5SHKaKlafpiIyqgJe_i__VMvu5zOPv-UY0LZ1eU1Qf0CjWxAgg</recordid><startdate>19950620</startdate><enddate>19950620</enddate><creator>Vorobyov, P. V</creator><creator>Kirpotin, A. N</creator><creator>Rovkin, M. E</creator><creator>Boldyrev, A. P</creator><scope>GOX</scope></search><sort><creationdate>19950620</creationdate><title>Ferromagnetic Detectors of Axions in RF (S - X) Band</title><author>Vorobyov, P. V ; Kirpotin, A. N ; Rovkin, M. E ; Boldyrev, A. P</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a751-9ea58d656898d64614056f9d35e11989556f6114de4f250dca1f0f8ec2b6f5363</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1995</creationdate><topic>Physics - Astrophysics of Galaxies</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Physics - Earth and Planetary Astrophysics</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - High Energy Physics - Phenomenology</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Physics - Solar and Stellar Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Vorobyov, P. V</creatorcontrib><creatorcontrib>Kirpotin, A. N</creatorcontrib><creatorcontrib>Rovkin, M. E</creatorcontrib><creatorcontrib>Boldyrev, A. P</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Vorobyov, P. V</au><au>Kirpotin, A. N</au><au>Rovkin, M. E</au><au>Boldyrev, A. P</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Ferromagnetic Detectors of Axions in RF (S - X) Band</atitle><date>1995-06-20</date><risdate>1995</risdate><abstract>The (pseudo) Goldstone bosons arise naturally in many modern theories such as
supergravity, superstring theory and variants of general relativity with
torsion. By the other hand, there are well known indications that a large part
of the Universe mass exists in a form of dark matter. The most attractive model
of the dark matter is non-relativistic gas of the light elementary particles
weakly interacting with the "usual" matter \cite{b2} - \cite{b4}. We describe
ferromagnetic detectors, for search of arion(axion), where a high-sensitive
two-channel SHF receiver is used. Its sensitivity reaches to $10^{-20}\,Wt$,
with time of accumulation $1-10\,s$. Fourier analysis of signal provides a
survey in zone up to $\pm50\,KHz$ with spectral resolution $0.1 - 25\, Hz$.
There was applied a high sensitive SHF receiver based on a special computer
method of coherent accumulation of signals. It is possible to use the receiver
in other precise experiments: measuring of electron/positron beams polarization
in storage rings, investigation of parity violation, investigation of
atmosphere with radars etc.</abstract><doi>10.48550/arxiv.hep-ph/9506371</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | DOI: 10.48550/arxiv.hep-ph/9506371 |
| ispartof | |
| issn | |
| language | eng |
| recordid | cdi_arxiv_primary_hep_ph_9506371 |
| source | arXiv.org |
| subjects | Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - High Energy Astrophysical Phenomena Physics - High Energy Physics - Phenomenology Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics |
| title | Ferromagnetic Detectors of Axions in RF (S - X) Band |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-05T07%3A32%3A12IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-arxiv_GOX&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Ferromagnetic%20Detectors%20of%20Axions%20in%20RF%20(S%20-%20X)%20Band&rft.au=Vorobyov,%20P.%20V&rft.date=1995-06-20&rft_id=info:doi/10.48550/arxiv.hep-ph/9506371&rft_dat=%3Carxiv_GOX%3Ehep_ph_9506371%3C/arxiv_GOX%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |