Solar System Velocity from Muon Flux Anisotropy: Difference between revisions
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| published = 1996 | | published = 1996 | ||
| journal = [[Apeiron]] | | journal = [[Apeiron]] | ||
| volume = | | volume = 3 | ||
| number = | | number = 2 | ||
| num_pages = 5 | | num_pages = 5 | ||
| pages = 33-37 | | pages = 33-37 | ||
Latest revision as of 09:19, 21 July 2026
| Scientific Paper | |
|---|---|
| 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.