Solar System Velocity from Muon Flux Anisotropy - Revision history

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	==Abstract==		==Abstract==

	The cosmic-ray muon half-life, being proportional to g = 1 1-v2 c2 , depends upon its absolute velocity v v v o o 2 = ?2 +2 v? ? v + 2 , where v? is the muon velocity relative to the Earth and vo is the absolute velocity of the solar system. The sea-level muon flux then depends upon vo through v? ? vo . An approximate theory is presented for the absolute velocity of the solar system vo as a function of the expected anisotropy of the sea-level flux of muons as a function of the celestial direction of v? . A cosmic ray telescope was used to measure the muon flux as a function of the celestial direction. The observations yield a solar system velocity of vo = 359 ? 180 km/s in the direction of right ascension a o = 8.7 ? 3.5h and declination d o= ?1.1 ? 10.0? in reasonable agreement with results reported involving other methods.[[Category:Scientific Paper]]		The cosmic-ray muon half-life, being proportional to g = 1 1-v2 c2 , depends upon its absolute velocity v v v o o 2 = ?2 +2 v? ? v + 2 , where v? is the muon velocity relative to the Earth and vo is the absolute velocity of the solar system. The sea-level muon flux then depends upon vo through v? ? vo . An approximate theory is presented for the absolute velocity of the solar system vo as a function of the expected anisotropy of the sea-level flux of muons as a function of the celestial direction of v? . A cosmic ray telescope was used to measure the muon flux as a function of the celestial direction. The observations yield a solar system velocity of vo = 359 ? 180 km/s in the direction of right ascension a o = 8.7 ? 3.5h and declination d o= ?1.1 ? 10.0? in reasonable agreement with results reported involving other methods.

			[[Category:Scientific Paper\|solar system velocity muon flux anisotropy]]

	[[Category:Relativity]]		[[Category:Relativity]]

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{{Infobox paper
| title = Solar System Velocity from Muon Flux Anisotropy
| url = [http://www.naturalphilosophy.org/pdf/abstracts/abstracts_597.pdf Link to paper]
| author = [[Paul Wesley]], [[Christian Monstein]]
| keywords = [[muon half-life]], [[absolute velocity]], [[solar system velocity]]
| published = 1996
| journal = [[Apeiron]]
| volume = [[3]]
| number = [[2]]
| num_pages = 5
| pages = 33-37
}}

'''Read the full paper''' [http://www.naturalphilosophy.org/pdf/abstracts/abstracts_597.pdf here]

==Abstract==

The cosmic-ray muon half-life, being proportional to g = 1 1-v2 c2 , depends upon its absolute velocity v v v o o 2 = ?2 +2 v? ? v + 2 , where v? is the muon velocity relative to the Earth and vo is the absolute velocity of the solar system. The sea-level muon flux then depends upon vo through v? ? vo . An approximate theory is presented for the absolute velocity of the solar system vo as a function of the expected anisotropy of the sea-level flux of muons as a function of the celestial direction of v? . A cosmic ray telescope was used to measure the muon flux as a function of the celestial direction. The observations yield a solar system velocity of vo = 359 ? 180 km/s in the direction of right ascension a o = 8.7 ? 3.5h and declination d o= ?1.1 ? 10.0? in reasonable agreement with results reported involving other methods.[[Category:Scientific Paper]]

[[Category:Relativity]]