2018
DOI: 10.1088/1674-1056/27/1/010301
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Solution of the spin-one DKP oscillator under an external magnetic field in noncommutative space with minimal length

Abstract: The spin-one Duffin-Kemmer-Petiau (DKP) oscillator under a magnetic field in the presence of the minimal length in the noncommutative coordinate space is studied by using the momentum space representation. The explicit form of energy eigenvalues is found, and the eigenfunctions are obtained in terms of the Jacobi polynomials. It shows that for the same azimuthal quantum number, the energy E increases monotonically with respect to the noncommutative parameter and the minimal length parameter. Additionally, we a… Show more

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Cited by 20 publications
(11 citation statements)
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“…[1] Many kinds of noncommutative spaces have been studied by physicists and mathematicians, such as the Moyal plane and fuzzy space. [2][3][4][5][6][7][8][9][10][11] The phase space in quantum mechanics is also a Moyal-type noncommutative space, because the position and momentum operators satisfy the noncommutative Heisenberg algebras.…”
Section: Introductionmentioning
confidence: 99%
“…[1] Many kinds of noncommutative spaces have been studied by physicists and mathematicians, such as the Moyal plane and fuzzy space. [2][3][4][5][6][7][8][9][10][11] The phase space in quantum mechanics is also a Moyal-type noncommutative space, because the position and momentum operators satisfy the noncommutative Heisenberg algebras.…”
Section: Introductionmentioning
confidence: 99%
“…The deformed momentum operators will almost inevitably cause Hamiltonians of all quantum mechanical systems to be corrected. Since Kempf and his colleagues established the theoretical framework of quantum mechanics based on generalized uncertainty, the studies of Schrödinger equation, [13][14][15][16][17][18][19][20][21][22][23][24][25][26] the Dirac equation, [27][28][29][30][31][32][33][34][35][36][37][38] K-G equation [39][40][41] and DKP equation [42][43][44][45][46][47][48][49][50] get great interest, and some phenomena in black hole remnants, 51,52 the trans-Planckian problem of inflation, 53,54 and the cosmological constant problem 55,56 can be explained by generalized uncertainty relations. On the quantum level, except for the bound state, some related works on scattering state have been reported.…”
Section: Introductionmentioning
confidence: 99%
“…For instance, distortions of energy levels of atoms [15][16][17][18][19][20], contributions to the topological phase effects [11,12,[21][22][23][24][25][26], corrections on the spin-orbital interactions [27][28][29][30][31][32], as well as deformations of quantum speeds of relativistic charged particles [33][34][35][36].…”
Section: Introductionmentioning
confidence: 99%