M
M. D. Hasinoff
Researcher at University of British Columbia
Publications - 152
Citations - 4317
M. D. Hasinoff is an academic researcher from University of British Columbia. The author has contributed to research in topics: Muon & CERN Axion Solar Telescope. The author has an hindex of 27, co-authored 146 publications receiving 3658 citations. Previous affiliations of M. D. Hasinoff include University of Melbourne & Virginia Tech.
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Journal ArticleDOI
New CAST Limit on the Axion-Photon Interaction
Vassilis Anastassopoulos,S. Aune,K. Barth,A. Belov,Heinrich Bräuninger,Giovanni Cantatore,J. M. Carmona,J. F. Castel,Serkant Ali Cetin,Finn Erland Christensen,J. I. Collar,T. Dafni,M. Davenport,Todd A. Decker,Alexander Dermenev,Klaus Kurt Desch,C. Eleftheriadis,Georgios Fanourakis,E. Ferrer-Ribas,H. Fischer,J. A. Garcia,A. Gardikiotis,J. G. Garza,Evangelos Gazis,T. Geralis,Ioannis Giomataris,Sergei Gninenko,C. J. Hailey,M. D. Hasinoff,Dieter H. H. Hoffmann,F.J. Iguaz,I. G. Irastorza,Anders Clemen Jakobsen,Joachim Jacoby,Krešimir Jakovčić,Jochen Kaminski,Marin Karuza,Nenad Kralj,Milica Krčmar,Sofia Kostoglou,Ch. Krieger,Biljana Lakić,J. M. Laurent,A. Liolios,Ante Ljubičić,G. Luzón,M. Maroudas,L. Miceli,S. Neff,I. Ortega,T. Papaevangelou,K. Paraschou,Michael J. Pivovaroff,Georg G. Raffelt,M. Rosu,J. Ruz,E. Ruiz Chóliz,I. Savvidis,Søren Schmidt,Yannis K. Semertzidis,Sami K. Solanki,L. Stewart,Theodoros Vafeiadis,Julia Vogel,S. C. Yildiz,Konstantin Zioutas +65 more
TL;DR: The axion-photon coupling strength of the CERN Axion Solar Telescope (CAST) was shown to be at least 0.02$ eV in the first vacuum phase (2003-2004) with low-background x-ray detectors and a new xray telescope as mentioned in this paper.
Journal ArticleDOI
An improved limit on the axion–photon coupling from the CAST experiment
S. Andriamonje,S. Aune,D. Autiero,K. Barth,A. Belov,B. Beltrán,H. Bräuninger,J. M. Carmona,S. Cebrián,J. I. Collar,T. Dafni,M. Davenport,L. Di Lella,C. Eleftheriadis,Jakob Englhauser,G. Fanourakis,E. Ferrer Ribas,H. Fischer,J. Franz,Peter Friedrich,Theodoros Geralis,Ioannis Giomataris,S. Gninenko,Hector Gomez,M. D. Hasinoff,F.H. Heinsius,Dieter H. H. Hoffmann,I. G. Irastorza,J. Jacoby,Krešimir Jakovčić,D. Kang,K. Königsmann,R. Kotthaus,Milica Krčmar,Konstantinos Kousouris,Markus Kuster,Biljana Lakić,C. Lasseur,A. Liolios,Ante Ljubičić,Gerhard Lutz,G. Luzón,David Miller,A. Morales,J. Morales,A. Ortiz,T. Papaevangelou,A. Placci,Georg G. Raffelt,H. Riege,A Rodríguez,J. Ruz,I. Savvidis,Yannis K. Semertzidis,Yannis K. Semertzidis,Pasquale D. Serpico,L. Stewart,Joaquin Vieira,J.A. Villar,Julia Vogel,L. Walckiers,Konstantin Zioutas,Konstantin Zioutas +62 more
TL;DR: In this paper, the CERN Axion Solar Telescope (CAST) set-up with improved conditions in all detectors was used to search for solar axions or similar particles that couple to two photons.
Journal ArticleDOI
First results from the CERN axion solar telescope.
Konstantin Zioutas,S. Andriamonje,V. Arsov,V. Arsov,S. Aune,D. Autiero,F. T. Avignone,K. Barth,A. Belov,B. Beltrán,H. Bräuninger,J. M. Carmona,S. Cebrián,E. Chesi,J. I. Collar,R. J. Creswick,T. Dafni,M. Davenport,L. Di Lella,L. Di Lella,C. Eleftheriadis,Jakob Englhauser,G. Fanourakis,H. A. Farach,Efrain J. Ferrer,H. Fischer,J. Franz,Peter Friedrich,Theodoros Geralis,Ioannis Giomataris,S. Gninenko,N. Goloubev,M. D. Hasinoff,F.H. Heinsius,Dieter H. H. Hoffmann,I. G. Irastorza,J. Jacoby,D. Kang,K. Königsmann,R. Kotthaus,Milica Krčmar,K. Kousouris,Markus Kuster,Biljana Lakić,C. Lasseur,A. Liolios,Ante Ljubičić,Gerhard Lutz,G. Luzón,David Miller,A. Morales,J. Morales,M. Mutterer,A. Nikolaidis,A. Ortiz,T. Papaevangelou,A. Placci,Georg G. Raffelt,J. Ruz,H. Riege,M.L. Sarsa,I. Savvidis,W. Serber,Pasquale D. Serpico,Yannis K. Semertzidis,Yannis K. Semertzidis,L. Stewart,Joaquin Vieira,J.A. Villar,L. Walckiers,K. Zachariadou +70 more
TL;DR: The first results from the analysis of these data are presented in this article, implying an upper limit to the axion-photon coupling at 95% C.L. for axion masses.
Journal ArticleDOI
Probing eV-scale axions with CAST
E. Arik,S. Aune,D. Autiero,K. Barth,A. Belov,B. Beltrán,B. Beltrán,S. Borghi,S. Borghi,G. Bourlis,F. S. Boydag,H. Bräuninger,J. M. Carmona,S. Cebrián,Serkant Ali Cetin,J. I. Collar,T. Dafni,M. Davenport,L. Di Lella,O.B. Dogan,C. Eleftheriadis,N. Elias,Georgios Fanourakis,E. Ferrer-Ribas,H. Fischer,Peter Friedrich,J. Franz,Javier Galan,Theodoros Geralis,Ioannis Giomataris,S. Gninenko,Hector Gomez,R. Hartmann,M. D. Hasinoff,F. H. Heinsius,F. H. Heinsius,I. Hikmet,Dieter H. H. Hoffmann,I. G. Irastorza,J. Jacoby,Krešimir Jakovčić,D. Kang,D. Kang,K. Königsmann,R. Kotthaus,Milica Krčmar,Konstantinos Kousouris,Markus Kuster,Biljana Lakić,C. Lasseur,A. Liolios,Ante Ljubičić,Gerhard Lutz,G. Luzón,David Miller,J. Morales,T. O. Niinikoski,A. Nordt,A. Ortiz,T. Papaevangelou,Michael J. Pivovaroff,A. Placci,Georg G. Raffelt,H. Riege,H. Riege,A Rodríguez,J. Ruz,I. Savvidis,Yannis K. Semertzidis,Yannis K. Semertzidis,Pasquale D. Serpico,Pasquale D. Serpico,Regina Soufli,L. Stewart,K. van Bibber,J.A. Villar,Julia Vogel,L. Walckiers,Konstantin Zioutas,Konstantin Zioutas +79 more
TL;DR: In this paper, the authors reported results from CAST with evacuated magnet bores (phase I), setting limits on lower mass axions, and they also reported results of CAST Phase II, where the magnetbores were filled with 4He gas (phase II) of variable pressure.
Journal ArticleDOI
Search for sub-eV mass solar axions by the CERN Axion Solar Telescope with 3He buffer gas.
M. Arik,S. Aune,K. Barth,A. Belov,S. Borghi,Heinrich Bräuninger,Giovanni Cantatore,J. M. Carmona,Serkant Ali Cetin,J. I. Collar,T. Dafni,M. Davenport,C. Eleftheriadis,N. Elias,C. Ezer,Georgios Fanourakis,E. Ferrer-Ribas,Peter Friedrich,Javier Galan,J. A. Garcia,A. Gardikiotis,Evangelos Gazis,T. Geralis,I. Giomataris,Sergei Gninenko,Hector Gomez,E. Gruber,T. Guthörl,Raimo Hartmann,F. Haug,M. D. Hasinoff,Dieter Hoffmann,F.J. Iguaz,I. G. Irastorza,Joachim Jacoby,Krešimir Jakovčić,Marin Karuza,K. Königsmann,Rainer Kotthaus,Milica Krčmar,Markus Kuster,Biljana Lakić,J. M. Laurent,A. Liolios,Ante Ljubičić,V. Lozza,G. Lutz,G. Luzón,J. Morales,T. O. Niinikoski,A. Nordt,T. Papaevangelou,M. J. Pivovaroff,Georg G. Raffelt,Timur Rashba,H. Riege,Adriane De Assis Lawisch Rodriguez,M. Rosu,J. Ruz,I. Savvidis,P. S. Silva,Sami K. Solanki,L. Stewart,A. Tomás,M. Tsagri,K. van Bibber,Theodoros Vafeiadis,José Villar,Julia Vogel,S. C. Yildiz,Konstantin Zioutas +70 more
TL;DR: From the absence of excess x rays when the magnet was pointing to the Sun, the typical upper limit on the axion-photon coupling of g(aγ)≲2.3×10(-10) GeV(-1) at 95% C.L. is set.