probability of scattering造句

• The diagrams are part of Feynman's very efficient and elegant algorithm for computing the probability of scattering processes.
• Homi J . Bhabha derived an expression for the probability of scattering positrons by electrons, a process now known as Bhabha scattering.
• Bhabha gained international prominence after deriving a correct expression for the probability of scattering positrons by electrons, a process now known as Bhabha scattering.
• The probability of scattering of a neutron from a nucleus is given by the elastic, i . e ., the total kinetic energy and momentum of the system ( that of the neutron and the nucleus ) is conserved.
• The " probability of scattering " in such a system is defined as the number of electrons scattered, per unit electron current, per unit path length, per unit pressure at 0 癈, per unit solid angle.
• If we consider cosmic background neutrinos then the coherence length will be large, of the order of 0.1 millimeters and you'll have a huge number of nucleons within the radius of one coherence length in a neutron star, making the probability of scattering a lot larger than what you would expect using the ratio of densities . talk ) 13 : 05, 28 June 2013 ( UTC)