Difference between revisions of "Solar System Velocity from Muon Flux Anisotropy"
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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. | + | 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:Relativity]] | + | [[Category:Scientific Paper|solar system velocity muon flux anisotropy]] |
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+ | [[Category:Relativity|solar system velocity muon flux anisotropy]] |
Latest revision as of 19:55, 1 January 2017
Scientific Paper | |
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Title | Solar System Velocity from Muon Flux Anisotropy |
Read in full | Link to paper |
Author(s) | Paul Wesley, Christian Monstein |
Keywords | muon half-life, absolute velocity, solar system velocity |
Published | 1996 |
Journal | Apeiron |
Volume | 3 |
Number | 2 |
No. of pages | 5 |
Pages | 33-37 |
Read the full paper 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.