Contribution to a conference proceedings/Internal Report

PUBDB-2016-01351

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Signatures for Solar Axions/WISPs

Zioutas, K. ; Vafeiadis, T. ; Tsagri, M. ; Semertzidis, Y. K. ; Papaevangelou, T. ; Dafni, T. ; Anastassopoulos, V.

2010
Verlag Deutsches Elektronen-Synchrotron Hamburg

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Please use a persistent id in citations: doi:10.3204/DESY-PROC-2010-03/zioutas_konstantin

Report No.: DESY-PROC-2010-03; arXiv:1011.0629

Abstract: Standard solar physics cannot account for the X-ray emission and other puzzles, the most striking example being the solar corona mystery. The corona temperature rise above the non-flaring magnetized sunspots, while the photosphere just underneath becomes cooler, makes this mystery more intriguing. The paradoxical Sun is suggestive of some sort of exotic solution, axions being the (only?) choice for the missing ingredient. We present atypical axion signatures, which depict solar axions with a rest mass max ~17 meV/c2. Then, the Sun has been for decades the overlooked harbinger of new particle physics.

Keyword(s): axion: solar ; signature ; new physics ; X-ray: solar ; experimental results

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Contributing Institute(s):

1. Bibliothek und Dokumentation (L)

Research Program(s):

1. 899 - ohne Topic (POF3-899) (POF3-899)

Experiment(s):

1. Facility (machine) HERA

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Linked articles:

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Proceedings/Internal Report Baudis, L. (Editor) ; Schumann, M. (Editor)
Proceedings, 6th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2010)
20106th Patras Workshop on Axions, WIMPs and WISPs, AXION-WIMP 2010, ZürichZürich, Switzerland, 5 Jul 2010 - 9 Jul 20102010-07-052010-07-09 Hamburg : Verlag Deutsches Elektronen-Synchrotron (2010)2010     Files BibTeX | EndNote: XML, Text | RIS

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