DC Field | Value | Language |
---|---|---|
dc.contributor.author | Gardikiotis, A. | ko |
dc.contributor.author | Anastassopoulos, V | ko |
dc.contributor.author | Bertolucci, S | ko |
dc.contributor.author | Cantatore, G | ko |
dc.contributor.author | Cetin, S | ko |
dc.contributor.author | Fischer, H | ko |
dc.contributor.author | Funk, W | ko |
dc.contributor.author | Hoffmann, DHH | ko |
dc.contributor.author | Hofmann, S | ko |
dc.contributor.author | Karuza, M | ko |
dc.contributor.author | Maroudas, M | ko |
dc.contributor.author | Semertzidis, Yannis K | ko |
dc.contributor.author | Tkachev, I | ko |
dc.contributor.author | Zioutas, K | ko |
dc.date.accessioned | 2023-07-04T01:01:39Z | - |
dc.date.available | 2023-07-04T01:01:39Z | - |
dc.date.created | 2023-06-08 | - |
dc.date.issued | 2017-05 | - |
dc.identifier.citation | 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017, pp.19 - 22 | - |
dc.identifier.uri | http://hdl.handle.net/10203/310230 | - |
dc.description.abstract | We suggest a new approach to search for galactic axions or other similar exotica. Streaming dark matter (DM) could have a better discovery potential because of flux enhancement, due to gravitational lensing when the Sun and/or a planet are aligned with a DM stream [1]. Of interest are also axion miniclusters, in particular, if the solar system has trapped one during its formation. Wide-band axion antennae fit this concept, but also the proposed fast narrow band scanning. A network of detectors can provide full time coverage and a large axion mass acceptance. Other DM searches may profit from this proposal. | - |
dc.language | English | - |
dc.publisher | Verlag Deutsches Elektronen-Synchrotron | - |
dc.title | Search for streaming dark matter axions or other exotica | - |
dc.type | Conference | - |
dc.identifier.scopusid | 2-s2.0-85085944782 | - |
dc.type.rims | CONF | - |
dc.citation.beginningpage | 19 | - |
dc.citation.endingpage | 22 | - |
dc.citation.publicationname | 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017 | - |
dc.identifier.conferencecountry | GR | - |
dc.identifier.conferencelocation | Thessaloniki | - |
dc.identifier.doi | 10.3204/DESY-PROC-2017-02/gardikiotis_antonios | - |
dc.contributor.localauthor | Semertzidis, Yannis K | - |
dc.contributor.nonIdAuthor | Gardikiotis, A. | - |
dc.contributor.nonIdAuthor | Anastassopoulos, V | - |
dc.contributor.nonIdAuthor | Bertolucci, S | - |
dc.contributor.nonIdAuthor | Cantatore, G | - |
dc.contributor.nonIdAuthor | Cetin, S | - |
dc.contributor.nonIdAuthor | Fischer, H | - |
dc.contributor.nonIdAuthor | Funk, W | - |
dc.contributor.nonIdAuthor | Hoffmann, DHH | - |
dc.contributor.nonIdAuthor | Hofmann, S | - |
dc.contributor.nonIdAuthor | Karuza, M | - |
dc.contributor.nonIdAuthor | Maroudas, M | - |
dc.contributor.nonIdAuthor | Tkachev, I | - |
dc.contributor.nonIdAuthor | Zioutas, K | - |
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