Overlooked astrophysical signatures of axion(-like) particles

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The solar (stellar) axion paradigm Escaping energy: star evolution [=age] limits on g aγγ no direct axion signal [as yet] axions = invisible PVLAS more?“natural” fine tuning + high efficiency unexplained solar/stellar observations! axions ≠ invisibleThe extended axion paradigm this work …
Page 1: Overlooked astrophysical signatures
Page 6 and 7: Challenging questions @ Sun 11 year
Page 8 and 9: Solar temperature distribution sola
Page 10 and 11: The mechanism that heats the solar
Page 12 and 13: 2005- RHESSISMART_1B-modified sola
Page 14 and 15: OFFPOINTING:1992 YOHKOH2005- RHES
Page 16 and 17: 2006Values in 3-12 keV correlate wi
Page 18 and 19: What produces solar flares? µflar
Page 20 and 21: Electrical Current Issue in FlaresR
Page 22 and 23: One key issue to understand the cor
Page 24 and 25: 2ndPower-law index n of L x ~ B n =
Page 26 and 27: SUNSPOTS50% of the quiet Sun4threla
Page 28 and 29: SUNSPOTS Yohkoh - XRTelescopeSolar
Page 30 and 31: M. Asplund et al., astro-ph/2004102
Page 32 and 33: The ‘solar model problem’ …..
Page 34 and 35: Martin ASPLUND, private communicati
Page 36 and 37: Soft X-ray CoronaWL K-Corona?mm pho
Page 38: X-raysYohkohSXT S60 o N60 oSXT equa
Page 42 and 43: work in progress • solar metalici
Page 44 and 45: plumes … are denser than their su
Page 46 and 47: 9σ 4.2σQVexpected S-Zexpected S-Z
Page 49 and 50: M.K. Browning et al., ApJL 648 (200

Overlooked astrophysical signatures of axion(-like) particles

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