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Extra: A very rare but occasionally observed decay of a muon u (rest energy = 106 MeV) is nto an electron e (rest energy 0.511 MeV) and a photon y (rest energy decays at rest by this mode, what is the kinetic energy of the electron and photon combined after the decay? (1MEV = 10°eV = 1.6 x 10-13 J) zero). If a muon

Extra: A very rare but occasionally observed decay of a muon u (rest energy = 106 MeV) is nto an electron e (rest energy 0.511 MeV) and a photon y (rest energy decays at rest by this mode, what is the kinetic energy of the electron and photon combined after the decay? (1MEV = 10°eV = 1.6 x 10-13 J) zero). If a muon

University Physics Volume 3
University Physics Volume 3
17th Edition
ISBN:9781938168185
Author:William Moebs, Jeff Sanny
Publisher:William Moebs, Jeff Sanny
Chapter5: Relativity
Section: Chapter Questions
Problem 71P: (a) Beta decay is nuclear decay in which an electron is emitted. If the electron is given 0.750 MeV...
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106 MeV) is Extra: A very rare but occasionally observed decay of a muon µ (rest energy = into an electron e (rest energy 0.511 MeV) and a photon y (rest energy decays at rest by this mode, what is the kinetic energy of the electron and photon combined after the decay? (1M V = 10°eV = 1.6 x 10-13 J) zero). If a muon
Transcribed Image Text:106 MeV) is Extra: A very rare but occasionally observed decay of a muon µ (rest energy = into an electron e (rest energy 0.511 MeV) and a photon y (rest energy decays at rest by this mode, what is the kinetic energy of the electron and photon combined after the decay? (1M V = 10°eV = 1.6 x 10-13 J) zero). If a muon
Constants and other possibly useful numbers g = 9.8m/s? G = 6.67 × 10-11 Nm/kg? c= 3 x 10°m/s Radius of the Moon: 1.74 x 106m Mass of the Sun: 2 x 1030kg Radius of the Sun: 6.957 x 10°m Mass of an electron me =9.11 x 10-31kg Mass of a proton mp 1.67 x 10-27kg %3D Average distance between the Moon and Earth: 3.84 x 10 m Average distance between Sun and Earth: 1.5 x 1011m Mass of Earth: 6 x 1024kg Radius of Earth: 6.4 x 106m Mass of the Moon: 7.35 x 1022kg Moments of Inertia: R+ R 2. MR² 1 2 I =Em;r? Iring = M Idisk =ML Igphere =M R = Icylinder =MR Irod I disk %3D %D %3D 12 The vector product or cross product between two vectors A and B can be calculated as follows: If you know the angle 0 between the two vectors, find the magnitude of the product |C| = |Ã × B| = |A||B| sin 0 and find the direction using the right-hand-rule. %3D
Transcribed Image Text:Constants and other possibly useful numbers g = 9.8m/s? G = 6.67 × 10-11 Nm/kg? c= 3 x 10°m/s Radius of the Moon: 1.74 x 106m Mass of the Sun: 2 x 1030kg Radius of the Sun: 6.957 x 10°m Mass of an electron me =9.11 x 10-31kg Mass of a proton mp 1.67 x 10-27kg %3D Average distance between the Moon and Earth: 3.84 x 10 m Average distance between Sun and Earth: 1.5 x 1011m Mass of Earth: 6 x 1024kg Radius of Earth: 6.4 x 106m Mass of the Moon: 7.35 x 1022kg Moments of Inertia: R+ R 2. MR² 1 2 I =Em;r? Iring = M Idisk =ML Igphere =M R = Icylinder =MR Irod I disk %3D %D %3D 12 The vector product or cross product between two vectors A and B can be calculated as follows: If you know the angle 0 between the two vectors, find the magnitude of the product |C| = |Ã × B| = |A||B| sin 0 and find the direction using the right-hand-rule. %3D
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