${{\boldsymbol A}^{0}}$ (Axion) MASS LIMITS from Astrophysics and Cosmology
INSPIRE search
These bounds depend on model-dependent assumptions (i.e. $-$ on a combination of axion parameters).
| • • • We do not use the following data for averages, fits, limits, etc. • • • |
| $>0.2$ |
|
|
ASTR |
| $>0.25$ |
1 |
|
ASTR |
| $>0.2$ |
2 |
|
ASTR |
|
|
|
ASTR |
| $>0.3$ |
2 |
|
ASTR |
| $>0.2$ |
|
|
ASTR |
|
1
Lower bound from 5.5 MeV ${{\mathit \gamma}}$-ray line from the sun.
|
|
2
Lower bound from requiring the red giants' stellar evolution not be disrupted by axion emission.
|
|
| References: |
|
| PL 116B 247 |
Constraints on Light Axions |
|
| PL 119B 323 |
New Particles from Nuclear Reactions in the Sun |
|
| PR D18 1829 |
Astrophysical Bounds on the Masses of Axions and Higgs Particles |
|
| PR D18 3605 |
Astrophysical Implications of New Light Higgs Bosons |
|
| PTP 60 1942 |
Astrophysical Constraints on the Axion Mass and the Number of Quark Flavors |
|
| JETPL 27 502 |
Some Astrophysical Limitations on Axion Mass |
|
