PHYS 1443 – Section 501 Lecture #1
... • How do these particles interact?? – All particles, including photons and neutrinos, participate in gravitational interactions – Photons can interact electromagnetically with any particles with electric charge – All charged leptons participate in both EM and weak interactions – Neutral leptons do n ...
... • How do these particles interact?? – All particles, including photons and neutrinos, participate in gravitational interactions – Photons can interact electromagnetically with any particles with electric charge – All charged leptons participate in both EM and weak interactions – Neutral leptons do n ...
LHCC - uniud.it
... huge baryon-antibaryon asimmetry in the Universe (NB today 1079!) • For practical purposes, we will assume that baryon and lepton nr are conserved, even if there is no deep theoretical reasons to suppose this conservation rule as absolute. • While total lepton number seems to be conserved, weak tr ...
... huge baryon-antibaryon asimmetry in the Universe (NB today 1079!) • For practical purposes, we will assume that baryon and lepton nr are conserved, even if there is no deep theoretical reasons to suppose this conservation rule as absolute. • While total lepton number seems to be conserved, weak tr ...
Some Basic Aspects of Fractional Quantum Numbers
... condensed matter physics as the opening of a gap. The choice of sign, of course, distinguishes between two degenerate ground states that have identical physical properties, since they can be related by the symmetry φ → −φ ψL → −ψL ...
... condensed matter physics as the opening of a gap. The choice of sign, of course, distinguishes between two degenerate ground states that have identical physical properties, since they can be related by the symmetry φ → −φ ψL → −ψL ...
The relation of colour charge to electric charge (E/c) −P2 −Q2 −(mc
... This can also be done using 2x2 Pauli matrices (labelled K,L,M) because two inertial observers agree on the component of momentum Q orthogonal to the component of momentum P in the direction of a Lorentz boost. ...
... This can also be done using 2x2 Pauli matrices (labelled K,L,M) because two inertial observers agree on the component of momentum Q orthogonal to the component of momentum P in the direction of a Lorentz boost. ...
Zharkova & Khabarova, ApJ (2012)
... Energization of particles up to MeV in the Earth’s magnetotail [Zelenyi, Lominadze & Taktakishvili (1990); Ashour-Abdalla et al. (2011) ], but it is still disputable for the HCS, because of some lack of observations. It is furthermore believed that there no particle acceleration in the keVMeV range ...
... Energization of particles up to MeV in the Earth’s magnetotail [Zelenyi, Lominadze & Taktakishvili (1990); Ashour-Abdalla et al. (2011) ], but it is still disputable for the HCS, because of some lack of observations. It is furthermore believed that there no particle acceleration in the keVMeV range ...
