Overlooked astrophysical signatures of axion(-like) particles

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9σ 4.2σQVexpected S-Zexpected S-Z2.3σexpected S-ZWX-rays observ. Hot gas properties31 co-added WMAP cluster fields expected S-Z effect 4x bigger less e - Radiative decay of massive particles, e.g. axions of the KK-type to reconcile contradictionR. Lieu, J.P.D. Mittaz, M. Bonamente, S-N. Zhang,ApJ. 648 (2006) 176Average WMAP observed and predicted radial profile for the 31 clusters. Thecontinuum of the prediction curve is fixed by alignment with the 2 o –3 o data. Thisalignment procedure is justified … it was shown that when 33 random fields were coadded,the 2 o –3 o annulus exhibits high stability. + systematical errors
Are these astrophysical ~axion signatures……like the tip of the iceberg?
Page 1: Overlooked astrophysical signatures
Page 4: How can ~axions show-up in celestia
Page 7 and 8: On solving the Coronal Heating Prob
Page 9 and 10: ↛
Page 11 and 12: 2 nd component
Page 13 and 14: http://science.nasa.gov/headlines/y
Page 15 and 16: Quiet-Sun X-ray observationsRHESSIT
Page 17 and 18: FLARESThe Electron “Problem”G.
Page 19 and 20: Flares T flare ≈ T core199 flares
Page 21 and 22: 1 st component ~B 2 4 cases ~ consi
Page 23 and 24: The long-term evolution of AR 7978
Page 25 and 26: FLARES origin?L x↑3rdThe Electro
Page 27 and 28: Magnetic field computed from the Ze
Page 29 and 30: Solar metalicity
Page 31 and 32: Serious disagreement between the pr
Page 33 and 34: The Ne abundance has been inferred
Page 35 and 36: Solar ν’s & X-raysoscillations /
Page 37 and 38: X-raysYohkohSXT S60 o N60 oSXT equa
Page 41 and 42: Solar Corona proxy Fe green line19
Page 43 and 44: By general agreement: the energy of
Page 45: Gamma rays from the neutralino dark
Page 50: X-ray mysteries:• Class 0 protost

Overlooked astrophysical signatures of axion(-like) particles

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