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  2. Lepton number - Wikipedia

    en.wikipedia.org/wiki/Lepton_number

    In particle physics, lepton number (historically also called lepton charge) [1] is a conserved quantum number representing the difference between the number of leptons and the number of antileptons in an elementary particle reaction. [2]

  3. Baryon number - Wikipedia

    en.wikipedia.org/wiki/Baryon_number

    Conserved' means that the sum of the baryon number of all incoming particles is the same as the sum of the baryon numbers of all particles resulting from the reaction. The one exception is the hypothesized Adler–Bell–Jackiw anomaly in electroweak interactions ; [ 4 ] however, sphalerons are not all that common and could occur at high energy ...

  4. Conservation law - Wikipedia

    en.wikipedia.org/wiki/Conservation_law

    Exact conservation laws include conservation of mass-energy, conservation of linear momentum, conservation of angular momentum, and conservation of electric charge. There are also many approximate conservation laws, which apply to such quantities as mass , parity , [ 1 ] lepton number , baryon number , strangeness , hypercharge , etc.

  5. Flavour (particle physics) - Wikipedia

    en.wikipedia.org/wiki/Flavour_(particle_physics)

    Absolutely conserved quantum numbers in the Standard Model are: electric charge (Q) weak isospin (T 3) baryon number (B) lepton number (L) In some theories, such as the grand unified theory, the individual baryon and lepton number conservation can be violated, if the difference between them (B − L) is conserved (see Chiral anomaly).

  6. Lepton - Wikipedia

    en.wikipedia.org/wiki/Lepton

    The name lepton comes from the Greek λεπτός leptós, "fine, small, thin" (neuter nominative/accusative singular form: λεπτόν leptón); [14] [15] the earliest attested form of the word is the Mycenaean Greek 𐀩𐀡𐀵, re-po-to, written in Linear B syllabic script. [16] Lepton was first used by physicist Léon Rosenfeld in 1948: [17]

  7. Electron–positron annihilation - Wikipedia

    en.wikipedia.org/wiki/Electron–positron...

    Conservation of angular momentum. Conservation of total (i.e. net) lepton number , which is the number of leptons (such as the electron) minus the number of antileptons (such as the positron); this can be described as a conservation of (net) matter law.

  8. Pair production - Wikipedia

    en.wikipedia.org/wiki/Pair_production

    As energy must be conserved, for pair production to occur, the incoming energy of the photon must be above a threshold of at least the total rest mass energy of the two particles created. (As the electron is the lightest, hence, lowest mass/energy, elementary particle, it requires the least energetic photons of all possible pair-production ...

  9. B − L - Wikipedia

    en.wikipedia.org/wiki/B_%E2%88%92_L

    The anomalies that would break baryon number conservation and lepton number conservation individually cancel in such a way that B – L is always conserved. One hypothetical example is proton decay where a proton (B = 1, L = 0) would decay into a pion (B = 0, L = 0) and positron (B = 0, L = –1). The weak hypercharge Y W is related to B – L via