2017
DOI: 10.1016/j.aop.2017.08.003
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On the Majorana fermion subject to a linear confinement

Abstract: We analyse the linear confinement of a Majorana fermion in (1 + 1)-dimensions. We show that the Dirac equation can be solved analytically. Besides, we show that the spectrum of energy is discrete, however, the energy levels are not equally spaced.

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Cited by 11 publications
(11 citation statements)
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“…Here, we investigate the above relativistic quantum system described by the Klein-Gordon oscillator subject to a Cornell-type scalar potential in the presence of external fields including an internal magnetic flux field. A scalar potential is included into the systems by modifying the mass m ⟶ m + SðrÞ which is called a position-dependent mass system in the relativistic quantum systems (see, e.g., [5,6,8,28,30,31,42,46,[52][53][54][55][56][57][58][59][60][61][62]).…”
Section: 2mentioning
confidence: 99%
“…Here, we investigate the above relativistic quantum system described by the Klein-Gordon oscillator subject to a Cornell-type scalar potential in the presence of external fields including an internal magnetic flux field. A scalar potential is included into the systems by modifying the mass m ⟶ m + SðrÞ which is called a position-dependent mass system in the relativistic quantum systems (see, e.g., [5,6,8,28,30,31,42,46,[52][53][54][55][56][57][58][59][60][61][62]).…”
Section: 2mentioning
confidence: 99%
“…Obviously, the matrices γ0 ′ = σy and γ1 ′ = +iσ z , for example, can also be considered to be a Majorana representation (incidentally, the latter choice was used in Refs. [10,11]). These two Majorana representations are related by…”
Section: The Majorana Particlementioning
confidence: 99%
“…Complex solutions for Eq. ( 12) can also be obtained [10], but these do not describe a Majorana particle.…”
Section: The Majorana Particlementioning
confidence: 99%
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“…on Klein-Gordon oscillator [105,106], on a scalar field in the spacetime with torsion [107][108][109], on a Majorana fermion [110], on a scalar field in the rotating cosmic string spacetime [111,112] and on a scalar particle in a Gödel-type spacetime [113,114].…”
Section: Effects Of a Linear Central Potentialmentioning
confidence: 99%