2011
DOI: 10.1088/1751-8113/44/25/255301
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On the problem of relativistic particles motion in a strong magnetic field and dense matter

Abstract: We consider a problem of electron motion in different media and magnetic field. It is shown that in case of nonmoving medium and constant homogenious magnetic field the electron energies are quantized. We also discuss the general problem of eigenvectors and eigenvalues of a given class of Hamiltonians. We examine obtained exact solutions for the particular case of the electron motion in a rotating neutron star with account for matter and magnetic field effects. We argue that all of these considerations can be … Show more

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Cited by 26 publications
(41 citation statements)
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References 18 publications
(35 reference statements)
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“…(12) and (13) by applying the charge conjugation ψē = iγ 2 ψ * e and setting λ = −1 in Eq. (15). Finally one has…”
Section: Induced Electric Current Of Massless Fermions Electroweakly mentioning
confidence: 97%
“…(12) and (13) by applying the charge conjugation ψē = iγ 2 ψ * e and setting λ = −1 in Eq. (15). Finally one has…”
Section: Induced Electric Current Of Massless Fermions Electroweakly mentioning
confidence: 97%
“…For the first time the Dirac equation for a massive electron, electroweakly interacting with background matter under the influence of an external magnetic field, was solved in Ref. [21]. Then this solution was used in Ref.…”
Section: Anomalous Current In the Presence Of The Electroweak Interacmentioning
confidence: 99%
“…are the Hermite functions, H n (η) are the Hermite polynomials, and η = √ eBx + p y / √ eB. The energy spectrum for n > 0 reads [21,22]…”
Section: Anomalous Current In the Presence Of The Electroweak Interacmentioning
confidence: 99%
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“…The subtlety lies in the fact that, in the presence of a background field B 0 , as we have discussed in [26][27][28], the dispersion relations for the fermions are affected nontrivially by the presence of B 0 , which differentiates it from the chiral chemical potential case; moreover, there are subtleties related to the order of taking the massless limit m → 0. In the presence of a chiral chemical potential, an external constant magnetic field and a (generic, but constant) axial background (of which our (constant) B 0 is a special case) the CME was discussed in [43], within the framework of relativistic quantum mechanics [55]. It turns out to be important to take the massless (chiral fermion) limit m → 0 at the end of the computation: one should assume massive fermions, in the presence of a B 0 = 0, solve the corresponding Dirac equation, and only at the end take the limit m → 0.…”
Section: B Non-contribution Of the Kr Background To The Chiral Magnementioning
confidence: 99%