排序方式: 共有12条查询结果,搜索用时 15 毫秒
1.
Jesik R Abramov V Antipov Y Baldin B Crittenden R Dauwe L Davis C Denisov S Dyshkant A Dzierba A Glebov V Goldberg H Gribushin A Koreshev V Krider J Krinitsyn A Li R Margulies S Marshall T Martin J Mendez H Petrukhin A Sirotenko V Smith P Solomon J Sulanke T Sulyaev R Vaca F Zieminski A Blusk S Bromberg C Chang P Choudhary B Chung W de Barbaro L Dlugosz W Dunlea J Engels E Fanourakis G Ginther G Hartman K Huston J Kapoor V Lirakis C Lobkowicz F Mani S Mansour J Maul A Miller R Oh B Pothier E 《Physical review letters》1995,74(4):495-498
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Alverson G Baker WF Ballocchi G Benson R Berg D Blusk S Bromberg C Brown D Carey D Chand T Chandlee C Choudhary BC Chung WH de Barbaro L DeSoi W Dlugosz W Dunlea J Easo S Engels E Faissler W Fanourakis G Ferbel T Garelick D Ginther G Glass G Glaubman M Gutierrez P Hartman K Huston J Johnstone C Kapoor V Kourbanis L Lanaro A Lirakis C Lobkowicz F Lukens P Mani S Maul A Mansour J Miller R Nelson CA Oh BY Orris D Pothier E Prebys E Rajaram BM Roser R Ruddick K Shepard P Shivpuri RK Sinanidis A 《Physical review D: Particles and fields》1993,48(1):5-28
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Arik M Aune S Barth K Belov A Borghi S Bräuninger H Cantatore G Carmona JM Cetin SA Collar JI Dafni T Davenport M Eleftheriadis C Elias N Ezer C Fanourakis G Ferrer-Ribas E Friedrich P Galán J García JA Gardikiotis A Gazis EN Geralis T Giomataris I Gninenko S Gómez H Gruber E Guthörl T Hartmann R Haug F Hasinoff MD Hoffmann DH Iguaz FJ Irastorza IG Jacoby J Jakovčić K Karuza M Königsmann K Kotthaus R Krčmar M Kuster M Lakić B Laurent JM Liolios A Ljubičić A Lozza V Lutz G Luzón G Morales J 《Physical review letters》2011,107(26):261302
The CERN Axion Solar Telescope (CAST) has extended its search for solar axions by using (3)He as a buffer gas. At T=1.8 K this allows for larger pressure settings and hence sensitivity to higher axion masses than our previous measurements with (4)He. With about 1 h of data taking at each of 252 different pressure settings we have scanned the axion mass range 0.39 eV?m(a)?0.64 eV. From the absence of excess x rays when the magnet was pointing to the Sun we set a typical upper limit on the axion-photon coupling of g(aγ)?2.3×10(-10) GeV(-1) at 95% C.L., the exact value depending on the pressure setting. Kim-Shifman-Vainshtein-Zakharov axions are excluded at the upper end of our mass range, the first time ever for any solar axion search. In the future we will extend our search to m(a)?1.15 eV, comfortably overlapping with cosmological hot dark matter bounds. 相似文献
4.
Alverson G Baker WF Ballocchi G Benson R Berg D Blusk S Bromberg C Brown D Carey D Chand T Chandlee C Choudhary BC Chung WH de Barbaro L DeSoi W Dlugosz W Dunlea J Easo S Engels E Faissler W Fanourakis G Ferbel T Garelick D Ginther G Glass G Glaubman M Gutierrez P Hartman K Huston J Johnstone C Kapoor V Kourbanis I Lanaro A Lirakis C Lobkowicz F Lukens P Mani S Maul A Mansour J Miller R Nelson CA Oh B Orris D Pothier E Prebys E Rajaram BM Roser R Ruddick K Shepard P Shivpuri RK Sinanidis A 《Physical review letters》1992,68(17):2584-2587
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Zioutas K Andriamonje S Arsov V Aune S Autiero D Avignone FT Barth K Belov A Beltrán B Bräuninger H Carmona JM Cebrián S Chesi E Collar JI Creswick R Dafni T Davenport M Di Lella L Eleftheriadis C Englhauser J Fanourakis G Farach H Ferrer E Fischer H Franz J Friedrich P Geralis T Giomataris I Gninenko S Goloubev N Hasinoff MD Heinsius FH Hoffmann DH Irastorza IG Jacoby J Kang D Königsmann K Kotthaus R Krcmar M Kousouris K Kuster M Lakić B Lasseur C Liolios A Ljubicić A Lutz G Luzón G Miller DW 《Physical review letters》2005,94(12):121301
Hypothetical axionlike particles with a two-photon interaction would be produced in the sun by the Primakoff process. In a laboratory magnetic field ("axion helioscope"), they would be transformed into x-rays with energies of a few keV. Using a decommissioned Large Hadron Collider test magnet, the CERN Axion Solar Telescope ran for about 6 months during 2003. The first results from the analysis of these data are presented here. No signal above background was observed, implying an upper limit to the axion-photon coupling g(agamma)<1.16x10(-10) GeV-1 at 95% C.L. for m(a) less, similar 0.02 eV. This limit, assumption-free, is comparable to the limit from stellar energy-loss arguments and considerably more restrictive than any previous experiment over a broad range of axion masses. 相似文献
6.
B. D. Ikotun S. Mishra G. C. Fanourakis 《Journal of inclusion phenomena and macrocyclic chemistry》2014,79(3-4):311-317
This study investigates the surface morphology, structure analysis and the effect on the porosity and particle size of a new composite prepared using fly ash with α and β cyclodextrins. The dry mix and solution methods were used to synthesize these composite samples. The X-ray diffraction analysis shows the new peaks that indicate the interaction between the materials. These results are in agreement with the Fourier transform infrared spectroscopic analysis that suggested the possibility of interaction of fly ash particles with cyclodextrin. Morphology changes between the composite material and the constituent materials were observed using the scanning electron microscopic. The porosity and particle size analyses show the significant changes with respect to preparation methods. 相似文献
7.
Alverson G Baker WF Ballocchi G Benson R Berg D Blusk S Bromberg C Brown D Carey D Chand T Chandlee C Choudhary BC Chung WH de Barbaro L DeSoi W Dlugosz W Dunlea J Easo S Engels E Faissler W Fanourakis G Ferbel T Garelick D Ginther G Glass G Glaubman M Gutierrez P Hartman K Huston J Johnstone C Kapoor V Kourbanis I Lanaro A Lirakis C Lobkowicz F Lukens P Mani S Maul A Mansour J Miller R Nelson CA Oh B Orris D Pothier E Prebys E Rajaram BM Roser R Ruddick K Shepard PF Shivpuri RK Sinanidis A 《Physical review D: Particles and fields》1994,49(7):3106-3112
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Gribushin A Abramov V Antipov Y Baldin B Crittenden R Davis C Dauwe L Denisov S Dyshkant A Dzierba A Glebov V Goldberg H Jesik R Koreshev V Krider J Krinitsyn A Li R Margulies S Marshall T Martin J Mendez H Petrukhin A Solomon J Sirotenko V Smith P Sulanke T Sulyaev R Vaca F Zieminski A Blusk S Bromberg C Chang P Choudhary B Chung WH de Barbaro L Dlugosz W Dunlea J Engels E Fanourakis G Ginther G Hartman K Huston J Kapoor V Lirakis C Mani S Mansour J Maul A Miller R Oh BY Pothier E Roser R 《Physical review D: Particles and fields》1996,53(9):4723-4733
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