Pregled bibliografske jedinice broj: 83239
Rare and forbidden decays
Rare and forbidden decays // Acta Physica Polonica B, 33 (2002), 4317-4372 (međunarodna recenzija, članak, znanstveni)
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Naslov
Rare and forbidden decays
Autori
Trampetić, Josip
Izvornik
Acta Physica Polonica B (0587-4254) 33
(2002);
4317-4372
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
forbidden decays; noncommutative QED; noncommutative SM
Sažetak
In these lectures I first cover radiative and semileptonic B decays, including the QCD corrections for the quark subprocesses. The exclusive modes and the evaluation of the hadronic matrix elements, i.e. the relevant hadronic form factors, are the second step. Small effects due to the long-distance, spectator contributions, etc. are discussed next. The second section we started with non-leptonic decays, typically $B \to \pi\pi, K\pi, \rho\pi, ...$ We describe in more detail our prediction for decays dominated by the $b\to s \eta_c$ transition. Reports on the most recent experimental results are given at the end of each subsection. In the second part of the lectures I discuss decays forbidden by the Lorentz and gauge invariance, and due to the violation of the angular moment conservation, generally called the Standard Model-forbiden decays. However, the non-commutative QED and/or non-commutative Standard Model (NCSM), developed in a series of works in the last few years allow some of those decay modes. These are, in the gauge sector, $Z\to \gamma\gamma, gg$, and in the hadronic sector, flavour changing decays of the type $K\to \pi \gamma$, $B\to K\gamma$, etc. We shall see, for example, that the flavour changing decay $D^+_s\to \pi^+ \gamma$ dominates over other modes, because the processes occur via charged currents, i.e. on the quark level it arises from the point-like photon $\times$ current $\times$ current interactions. In the last section we present the transition rate of ``transverse plasmon'' decay into a neutrino--antineutrino pair via noncommutative QED, i.e. $\gamma_{;\rm pl};\to \nu\bar\nu$. Such decays gives extra contribution to the mechanism for the energy loss in stars.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
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- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus
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