编辑: 黑豆奇酷 2015-09-03
Citation: K.

A. Olive et al. (Particle Data Group), Chin. Phys. C, 38,

090001 (2014) and

2015 update Axions (A0 ) and Other Very Light Bosons, Searches for A REVIEW GOES HERE C Check our WWW List of Reviews A0 (Axion) MASS LIMITS from Astrophysics and Cosmology A0 (Axion) MASS LIMITS from Astrophysics and Cosmology A0 (Axion) MASS LIMITS from Astrophysics and Cosmology A0 (Axion) MASS LIMITS from Astrophysics and Cosmology These bounds depend on model-dependent assumptions (i.e. ― on a combination of axion parameters). VALUE (MeV) DOCUMENT ID TECN COMMENT ? ? ? We do not use the following data for averages, ?ts, limits, etc. ? ? ? >0.2 BARROSO

82 ASTR Standard Axion >0.25

1 RAFFELT

82 ASTR Standard Axion >0.2

2 DICUS 78C ASTR Standard Axion MIKAELIAN

78 ASTR Stellar emission >0.3

2 SATO

78 ASTR Standard Axion >0.2 VYSOTSKII

78 ASTR Standard Axion

1 Lower bound from 5.5 MeV γ-ray line from the sun.

2 Lower bound from requiring the red giants' stellar evolution not be disrupted by axion emission. A0 (Axion) and Other Light Boson (X0) Searches in Hadron Decays A0 (Axion) and Other Light Boson (X0) Searches in Hadron Decays A0 (Axion) and Other Light Boson (X0) Searches in Hadron Decays A0 (Axion) and Other Light Boson (X0) Searches in Hadron Decays Limits are for branching ratios. VALUE CL% DOCUMENT ID TECN COMMENT ? ? ? We do not use the following data for averages, ?ts, limits, etc. ? ? ?

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