Production by Magnetic Excitation of
arXiv:1108.2525 · doi:10.1088/0954-3899/39/1/015007
Abstract
We compute the probability of production from the interaction between and the strong magnetic field generated in relativistic heavy ion collisions. The computation is first carried out in the heavy quark effective model, in which the M1 radiative transition is considered. Then we investigate the transition in the framework of non-relativistic heavy hadron chiral perturbation theory and show that the polarization of produced by this process is parallel to the direction of magnetic field and thus perpendicular to the reaction plane. The transition probability obtained in both approaches is of order .
7 pages, minor modification, references added
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- Chiral Hall Effect and Chiral Electric Waves
- Heavy meson spectroscopy under strong magnetic field
- Transverse flow induced by inhomogeneous magnetic fields in the Bjorken expansion
- A review of quarkonia under strong magnetic fields
- Cigar-shaped quarkonia under strong magnetic field
- Delayed versus accelerated quarkonium formation in a magnetic field
- Anisotropic tomography of heavy quark dissociation by using general propagator structure at finite magnetic field
- Hadronic Paschen-Back effect
- Quarkonium radiative decays from the hadronic Paschen-Back effect
- Majorana flipping of quarkonium spin states in transient magnetic field
- Dissociation of heavy quarkonium states in rapidly varying strong magnetic field
- Survival probabilities of charmonia as a clue to measure transient magnetic fields
- Magnetic field in relativistic heavy ion collisions: testing the classical approximation
- Magnetic excitation in relativistic heavy ion collisions
- Landau-Zener-Stückelberg-Majorana dynamics of magnetized quarkonia
- Quarkonium spectra with magnetically induced anisotropic confinement