Search for 14.4 keV solar axions emitted in the M1-transition of {sup 57}Fe nuclei with CAST
We have searched for 14.4 keV solar axions or more general axion-like particles (ALPs), that may be emitted in the M1 nuclear transition of {sup 57}Fe, by using the axion-to-photon conversion in the CERN Axion Solar Telescope (CAST) with evacuated magnet bores (Phase I). From the absence of excess o...
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| Veröffentlicht in: | Journal of cosmology and astroparticle physics 2009-12, Vol.2009 (12) |
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| container_title | Journal of cosmology and astroparticle physics |
| container_volume | 2009 |
| creator | Andriamonje, S. Aune, S. Dafni, T. Ferrer-Ribas, E. Autiero, D. Barth, K. Davenport, M. Lella, L. Di Belov, A. Beltrán, B. Carmona, J.M. Cebrián, S. Bräuninger, H. Englhauser, J. Friedrich, P. Collar, J.I. Eleftheriadis, C. Fanourakis, G. Fischer, H. Franz, J. Collaboration: CAST collaboration |
| description | We have searched for 14.4 keV solar axions or more general axion-like particles (ALPs), that may be emitted in the M1 nuclear transition of {sup 57}Fe, by using the axion-to-photon conversion in the CERN Axion Solar Telescope (CAST) with evacuated magnet bores (Phase I). From the absence of excess of the monoenergetic X-rays when the magnet was pointing to the Sun, we set model-independent constraints on the coupling constants of pseudoscalar particles that couple to two photons and to a nucleon g{sub aγ}|−1.19g{sub aN}{sup 0}+g{sub aN}{sup 3}| < 1.36 × 10{sup −16} GeV{sup −1} for m{sub a} < 0.03 eV at the 95% confidence level. |
| doi_str_mv | 10.1088/1475-7516/2009/12/002 |
| format | Article |
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From the absence of excess of the monoenergetic X-rays when the magnet was pointing to the Sun, we set model-independent constraints on the coupling constants of pseudoscalar particles that couple to two photons and to a nucleon g{sub aγ}|−1.19g{sub aN}{sup 0}+g{sub aN}{sup 3}| < 1.36 × 10{sup −16} GeV{sup −1} for m{sub a} < 0.03 eV at the 95% confidence level.</description><subject>ASTROPHYSICS</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>AXIONS</subject><subject>CONVERSION</subject><subject>COUPLING CONSTANTS</subject><subject>EV RANGE</subject><subject>GEV RANGE</subject><subject>IRON 57</subject><subject>KEV RANGE</subject><subject>LIMITING VALUES</subject><subject>M1-TRANSITIONS</subject><subject>NUCLEAR PHYSICS AND RADIATION PHYSICS</subject><subject>NUCLEONS</subject><subject>SOLAR PARTICLES</subject><subject>SUN</subject><subject>TELESCOPE COUNTERS</subject><issn>1475-7516</issn><issn>1475-7516</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2009</creationdate><recordtype>article</recordtype><recordid>eNpNj01Lw0AYhBdRsFZ_gvCC5zT77leSYwlWhYqHVk9CWfeDrMasZLcoiP_dgCKeZpgZHhhCzpEukNZ1iaKSRSVRlYzSpkRWUsoOyOwvP_znj8lJSs_TQHFez8jjxunRdODjCCgWAl7cA6TY6xH0R4hDAvcacnYWwgC5c3CLRR71kEKeWogePtP-DWT1tXIw7E3vAryH3EG73GxPyZHXfXJnvzon96vLbXtdrO-ubtrlujDIRS5QW4tPQkrlG6Wo81zZpuJTRBlD7RU3TMoaZWW9snzaKsGEQCbq6T81fE4ufrgx5bBLJmRnOhOHwZm8Y4xNLET-DQIqUrw</recordid><startdate>20091201</startdate><enddate>20091201</enddate><creator>Andriamonje, S.</creator><creator>Aune, S.</creator><creator>Dafni, T.</creator><creator>Ferrer-Ribas, E.</creator><creator>Autiero, D.</creator><creator>Barth, K.</creator><creator>Davenport, M.</creator><creator>Lella, L. 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Di</au><au>Belov, A.</au><au>Beltrán, B.</au><au>Carmona, J.M.</au><au>Cebrián, S.</au><au>Bräuninger, H.</au><au>Englhauser, J.</au><au>Friedrich, P.</au><au>Collar, J.I.</au><au>Eleftheriadis, C.</au><au>Fanourakis, G.</au><au>Fischer, H.</au><au>Franz, J.</au><au>Collaboration: CAST collaboration</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Search for 14.4 keV solar axions emitted in the M1-transition of {sup 57}Fe nuclei with CAST</atitle><jtitle>Journal of cosmology and astroparticle physics</jtitle><date>2009-12-01</date><risdate>2009</risdate><volume>2009</volume><issue>12</issue><issn>1475-7516</issn><eissn>1475-7516</eissn><abstract>We have searched for 14.4 keV solar axions or more general axion-like particles (ALPs), that may be emitted in the M1 nuclear transition of {sup 57}Fe, by using the axion-to-photon conversion in the CERN Axion Solar Telescope (CAST) with evacuated magnet bores (Phase I). From the absence of excess of the monoenergetic X-rays when the magnet was pointing to the Sun, we set model-independent constraints on the coupling constants of pseudoscalar particles that couple to two photons and to a nucleon g{sub aγ}|−1.19g{sub aN}{sup 0}+g{sub aN}{sup 3}| < 1.36 × 10{sup −16} GeV{sup −1} for m{sub a} < 0.03 eV at the 95% confidence level.</abstract><cop>United States</cop><doi>10.1088/1475-7516/2009/12/002</doi></addata></record> |
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| subjects | ASTROPHYSICS ASTROPHYSICS, COSMOLOGY AND ASTRONOMY AXIONS CONVERSION COUPLING CONSTANTS EV RANGE GEV RANGE IRON 57 KEV RANGE LIMITING VALUES M1-TRANSITIONS NUCLEAR PHYSICS AND RADIATION PHYSICS NUCLEONS SOLAR PARTICLES SUN TELESCOPE COUNTERS |
| title | Search for 14.4 keV solar axions emitted in the M1-transition of {sup 57}Fe nuclei with CAST |
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