Dirac -Function Potential in Quasiposition Representation of a Minimal-Length Scenario
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Eur. Phys. J. C (2018) 78:179 https://doi.org/10.1140/epjc/s10052-018-5659-6 Regular Article - Theoretical Physics Dirac δ-function potential in quasiposition representation of a minimal-length scenario M. F. Gusson, A. Oakes O. Gonçalves, R. O. Francisco, R. G. Furtado, J. C. Fabrisa, J. A. Nogueirab Departamento de Física, Universidade Federal do Espírito Santo, Vitória, ES 29075-910, Brazil Received: 26 April 2017 / Accepted: 22 February 2018 / Published online: 3 March 2018 © The Author(s) 2018. This article is an open access publication Abstract A minimal-length scenario can be considered as Although the first proposals for the existence of a mini- an effective description of quantum gravity effects. In quan- mal length were done by the beginning of 1930s [1–3], they tum mechanics the introduction of a minimal length can were not connected with quantum gravity, but instead with be accomplished through a generalization of Heisenberg’s a cut-off in nature that would remedy cumbersome diver- uncertainty principle. In this scenario, state eigenvectors of gences arising from quantization of systems with an infinite the position operator are no longer physical states and the number of degrees of freedom. The relevant role that grav- representation in momentum space or a representation in a ity plays in trying to probe a smaller and smaller region of quasiposition space must be used. In this work, we solve the the space-time was recognized by Bronstein [4] already in Schroedinger equation with a Dirac δ-function potential in 1936; however, his work did not attract a lot of attention. quasiposition space. We calculate the bound state energy and It was only in 1964 that Mead [5,6] once again proposed a the coefficients of reflection and transmission for the scatter- possible connection between gravitation and minimal length. ing states. We show that√ leading corrections are of order of Hence, we can assume that gravity may lead to an effec- the minimal length (O( β))and the coefficients of reflection tive cut-off in the ultraviolet. Furthermore, if we are con- and transmission are no longer the same for the Dirac delta vinced that gravitational effects are in order when a minimal well and barrier as in ordinary quantum mechanics. Further- length is introduced then a minimal-length scenario could more, assuming that the equivalence of the 1s state energy of be thought of as an effective description of quantum gravity the hydrogen atom and the bound state energy of the Dirac effects [7]. δ-function potential in the one-dimensional case is kept in a As far as we know, the introduction of a minimal-length minimal-length scenario, we also find that the leading cor- scenario can be carried out in three different ways [7– rection term for the ground state energy of the hydrogen atom 9]: a generalization of the Heisenberg uncertainty principle −25 1 is of the order of the minimal length and Δxmin ≤ 10 m. (GUP), a deformation of special relativity (DSR) and a mod- ification of the dispersion relation (MDR). Various problems connected with the minimal length have been studied in the context of non-relativistic quantum 1 Introduction mechanics. Among them are the harmonic oscillator [10–14], the hydrogen atom [15–21], step and barrier potentials [22– Gravity quantization has become a huge challenge for theo- 24], finite and infinite square wells [25,26]. In the relativistic retical physicists. Despite enormous efforts made, so far, it context, the Dirac equation has been studied in [27–33]. The was not possible to obtain a theory which can be considered Casimir effect has also been studied in a minimal-length sce- suitable and not even a consensus approach. Nevertheless, nario in [34–38]. most of the candidate theories for gravity quantization seem An interesting problem in quantum mechanics is the Dirac to have one common point: the prediction of the existence of δ-function potential. In general, the Dirac δ-function poten- a minimal length, that is, a limit for the precision of a length tial is used as a pedagogical exercise. Nevertheless, it has also measurement. been used to model physical quantum systems [39]. Maybe because the attractive Dirac δ-function potential is one of a e-mail: [email protected] 1 It is named doubly special relativity because of the existence of two b e-mail: [email protected] universal constants: the speed of light and the minimal length. 123 179 Page 2 of 7 Eur. Phys. J. C (2018) 78 :179 the simplest quantum systems which displays both a bound tainty principle (GUP). Since state and a set of continuous states, it has been used to model |[x ˆ, pˆ]| atomic and molecular systems [40–45]. In addition, the short- ΔxΔp ≥ , (1) range interactions in condensed matter with a large scattering 2 length can actually be modeled as a Dirac δ-function poten- a generalization of the uncertainty principle corresponds to a tial [46–50]. In quantum field theory, in order to treat the modification in the algebra of the operators. There are differ- Casimir effect more realistically, the boundary conditions ent suggestions of the modification of the commutation rela- 1 σ( )φ2( ) tion between the position and momentum operators which are replaced by the interaction potential 2 x x , where σ(x) represents the field of the material of the borders (back- implement a minimal-length scenario. Weare concerned with ground field). Hence, for sharply localized borders the back- the most usual of them, proposed by Kempf [10,11], which ground field can be modeled by a Dirac δ-function [51,52]. in a one-dimensional space is given by The Dirac δ-function potential by its very nature is a chal- [ˆ, ˆ]:= ¯ + β ˆ2 , lenging problem in a minimal-length scenario. x p ih 1 p (2) Ferkous [53] and Samar and Tkachuck [54] have inde- where β is a parameter related to the minimal length. The pendently calculated the bound state energy in “momen- commutation relation (2) corresponds to the GUP tum space”. In the two papers cited, the authors√ have found β β h¯ a√ correction for the expression of energy in and ΔxΔp ≥ 1 + β(Δp)2 + βˆp2 , (3) ( β ∼ Δxmin), but with different coefficients, therefore hav- 2 ing disagreeing outcomes. Samar and Tkachuck claim that which implies the existence of a non-zero minimal uncer- (−∞, ∞) √ this is because Ferkous considers p to belong to , tainty in the position Δxmin = h¯ β. π π whereas they consider p to belong to − √ , √ .Inthis 2 β 2 β Unfortunately, in this scenario the eigenstates of the posi- work, we propose to solve the problem of a non-relativistic tion operator are not physical sates2 and, consequently, the particle of mass m in the presence of the Dirac δ-function representation in position space can no longer be used, that is, potential in quasiposition space. Since the quasiposition an arbitrary state vector |ψ cannot be expanded in the basis space representation is used we can consider the cases of of state eigenvectors of the position operator {|x}. Hence the bound states and scattering states as well. We find the same obvious way to go ahead is to make use of the representation expression for the energy of the bound state as obtained by in momentum space: Ferkous. In addition, assuming that the equality between ∂ψ(˜ p) the 1s state energy of the hydrogen atom and the bound p|ˆx|ψ=ih¯ + βp2 , 1 ∂ (4) state energy of the Dirac δ-function potential in the one- p ˜ dimensional case when the coefficient of the δ-potential is p|ˆp|ψ=pψ(p). (5) replaced by the fine structure constant [41] is kept in a However, the representation in momentum space is not minimal-length scenario, we find that the leading correc- suitable in some cases, such as, for example, when the wave tion for the ground state energy of hydrogen atom is of the √ function has to satisfy a boundary condition at specifics order of the minimal length (O( β)), differently from the points. So, the representation in quasiposition space [56], values commonly found in the literature using perturbative methods [15–18,55], but according to the results obtained x ML|ˆx|ψ(t)=xψqp(x, t), (6) by Fityo et al. [20] and Bouaziz and Ferkous [21]usinga ∂2 ∂ψqp( , ) ML 2 x t non-perturbative approach. x |ˆp|ψ(t)=−ih¯ 1 − βh¯ , (7) ∂x2 ∂x The rest of this paper is organized as follows. In Sect. 2 we show how to introduce a minimal-length scenario and find to first order in the β parameter, is more appropriate.3 |x ML the time-independent Schroedinger equation in a quasiposi- are state vectors of maximal localization which satisfy [10] tion space representation. In Sect. 3 we solve the modified ML|ˆ| ML= , ∈ , Schroedinger equation and find the bound state energy and x x x x with x (8) (Δ ) = Δ = β, the coefficients of reflection and transmission for the scatter- x |x ML xmin h¯ (9) ing states. We present our conclusions in Sect. 4. 2 That is because the uncertainty ΔA of an operator Aˆ in any of its state eigenvectors |ψA must be zero, which is not the case for the position 2 Minimal-length scenario operator, since Δxmin > 0. 3 ˆ =ˆ Pedram√ [56] has proposed a representation in which x xo and ( β ˆ ) In quantum theory, a minimal-length scenario can be accom- ˆ = tan √ po ˆ ˆ p β ,wherexo and po are ordinary operators of position and plished by imposing a non-zero minimal uncertainty in the momentum, which obey the canonical commutation relation [ˆxo, pˆo]= measurement of position which leads to a generalized uncer- ih¯ .