ebook img

The $DKP$ equation in the Woods-Saxon potential well: Bound states PDF

0.39 MB·
Save to my drive
Quick download
Download
Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.

Preview The $DKP$ equation in the Woods-Saxon potential well: Bound states

The DKP equation in the Woods-Saxon potential well: Bound states 6 1 0 Boutheina Boutabia-Ch´eraitia 2 Laboratoire de Probabilit´es et Statistiques (LaPS) n a Universit´e Badji-Mokhtar. Annaba. Alg´erie J 6 ∗Facult´e de M´edecine d’Annaba. ] [email protected] h p Abdenacer Makhlouf - t n Laboratoire de Math´ematiques, Informatique, a u et Applications (LMIA) q [ Universit´e de Haute Alsace 1 Mulhouse. France v 2 [email protected] 7 6 January 11, 2016 1 0 . 1 0 6 1 Abstract : v We solve the Duffin-Kemmer-P´etiau equation in the presence of a i X spatially one-dimensional symmetric potential well. We compute the r scattering state solutions and we derive conditions for transmission a resonances. The bound solutions are derived by a graphic study and the appearance of the antiparticle bound state is discussed. Keywords: DKP equation- WS Potential well- Coefficient of transmission- Coefficient of reflection- Bound states MSC codes: 35J05, 35J10, 35K05, 35L05. ∗Permanent adress. 1 1 Introduction The presence of strong fields introduces quantum phenomena, such as su- percriticallity and spontaneous pair production which is one of the most in- teresting non-perturbative phenomena associated with the charged quantum vacuum. During the last decades, a great effort has been made in understanding quantum processes in strong fields. The discussion of overcritical behavior of bosons requires a full understanding of the single particle spectrum, and consequently of the exact solutions to the Klein-Gordon (KG) equation. Re- cently, transmission resonances for the KG [1] and Duffin-Kemmer-P´etiau (DKP) equation [2,3,4] in the presence of a Woods-Saxon (WS) potential barrier have been computed. The transmission coefficient as a function of the energy and the potential amplitude shows a behavior that resembles the one obtained for the Dirac equation in [5]. The KG equation in the WS potential well [6] was solved and it was shown that analogous to the square well potential, there is a critical point V where the bound antiparticle mode appears to coalesce with the bound cr particle. In the present article, we solve the DKP equation in the WS potential well and we make a graphical study for the resonance transmissions. Among the advantages of working with the WS potential we have to mention that, in the one-dimensional case, the DKP equation as well as the KG and Dirac equations are solvable in terms of special functions and therefore the study of bound states and scattering processes becomes more tractable. We show that the antiparticle bound states arise for the WS potential well, which is a smoothed out form of the square well. The interest in computing bound states and spontaneous pair creation processes in such potentials lies in the fact that they possess properties that could permit us to determine how the shape of the potential affects the pair creation mechanism. The article is structured as follows: Section 2 is devoted to solving the DKP equation in the presence of the one dimensional WS potential well. In Section 3 We derive the equation governing the eigenvalues corresponding to the bound states and compute the bound states. Finally, in Section4, we briefly summarize our results. 2 2 The DKP equation in the WS potential well TheDKP equation[7,8,9]isanaturalmannertoextendthecovariantDirac formalism to the case of scalar (spin 0) and vectorial (spin 1) particles when interacting with an electromagnetic field. It will be written as ((cid:126) = c = 1): [iβµ(∂ +ieA )−m]ψ(r,t) = 0 (1) µ µ where the matrices βµ verify the DKP algebra: βµβνβλ +βλβνβµ = gµνβλ +gνλβµ (2) wheretheconventionforthemetrictensorishere gµν = diag(1,−1,−1,−1). The algebra (2) has three irreductible representations whose degrees are 1,5, and10. Thefirstoneistrivial, havingnophysicalcontent, thesecondandthe thirdonescorrespondrespectivelytothescalarandvectorialrepresentations. For the spin 0, the βµ are given by: (cid:18) (cid:19) (cid:18) (cid:19) θ 0 0 ρi β0 = ; βi = ;i = 1,2,3 (3) 0 0 −ρi 0 T with (cid:18) (cid:19) (cid:18) (cid:19) −1 0 0 0 −1 0 ρ1 = , ρ2 = 0 0 0 0 0 0 (cid:18) (cid:19) (cid:18) (cid:19) (4) 0 0 −1 0 1 ρ3 = , θ = 0 0 0 1 0 the ρ denoting the transposed matrix of ρ, and 0 the zero matrix. For the T spin 1, the βµ are given by:   0 0 0 0  0 0 e 0  i β0 =  00TT 01 10 00 ; βi =  −0eTT 00 00 −0isi ; i = 1,2,3   i 0T 0 0 0 0T −is 0 0 i (5) with e = (1,0,0);e = (0,1,0);e = (0,0,1);0 = (0,0,0) (6) 1 2 3 3 0 and 1 denoting respectively the zero matrix and the unity matrix, and the s being the standard nonrelativistic (3×3) spin 1 matrices: i       0 0 0 0 0 i 0 −i 0 s1 =  0 0 −i ,s2 =  0 0 0 ,s3 =  i 0 0  (7) 0 i 0 −i 0 0 0 0 0 The DKP particles we consider are in interaction with the WS potential defined by: −V 0 V (z) = (8) r (cid:16) (cid:17) 1+exp |z|−a r where V is real and positive, a > 0 and r > 0 are real, positive and ad- 0 justable. The form of the WS potential is shown in the Fig.1, from which one readily notices that for a given value of the width parameter a, as the shape parameter r decreases (r −→ 0+), the WS potential reduces to a square well with smooth walls: Figure 1: The WS potential for a = 2, with r = 1 (solide line) 3 and r = 1 (dotted line) 100 V (z) = −V θ(a−|z|) 0 (cid:26) −V for |z| (cid:54) a = 0 (9) 0 for |z| > a 4 The interaction being scalar and independent of time, one can choose for ψ(z,t) the form e−iEtκ(z), so one gets the following eigenvalue equation: (cid:20) (cid:21) d β0(E −eV)+iβ3 −m κ(z) = 0 (10) dz with κ(z)T = (ϕ,A,B,C), A,B and C being respectively vectors of com- ponents A ,B and C ; i = 1,2,3. According to the equations they satisfy, i i i one gathers the components of κ(z) this way ΨT = (A ,A ,B ),ΦT = (B ,B ,A ),ΘT = (C ,−C ,ϕ); and C = 0 1 2 3 1 2 3 2 1 3 (11) with O Ψ = 0 (12) KG (cid:18) (cid:19) (cid:18) (cid:19) Φ E−eV = m ⊗Ψ (13) Θ i d mdz then one will designate by φ(z)T = (Ψ,Φ,Θ) the solution of (10)[2], O = d2 +(cid:2)(E −eV)2 −m2(cid:3) being the Klein-Gordon ”KG” operator. KG dz2 Bythefollowing, onewillfollowthesamestepsasforthebarrierpotential [2], where one will replace V by −V , then one gets the asymptotic behavior 0 0 of the wave function at |z| −→ ∞ :     1 1   Ψ  E   E   Ω  −→ Ae−ik(z+a) m ⊗V +Beik(z+a) m ⊗V (14) Θ z−→−∞  iµ   iµ  − rm rm     1 1   Ψ  E   E   Ω  −→ Ceik(z−a) m ⊗V +De−ik(z−a) m ⊗V (15) Θ z−→+∞  iµ   iµ  − rm rm with the following definitions of the coefficients: B and D are respectively the coefficients of the incoming waves from −∞ −→ 0 and from +∞ −→ 0. A and C are respectively the coefficients of the reflected and transmitted wave. 5 V is a constant vector of dimension (3×1) :   N 1 V =  N2  (16) N 3 The coefficients of reflection R and transmission T will be given by [2] : R = 1 (cid:12)(cid:12)λ2µ(cid:12)(cid:12)2(cid:12)(cid:12)(cid:12)F6 + F2(cid:12)(cid:12)(cid:12)2 (17) 4 (cid:12)F F (cid:12) 5 1 and T = 1 (cid:12)(cid:12)λ2µ(cid:12)(cid:12)2(cid:12)(cid:12)(cid:12)F6 − F2(cid:12)(cid:12)(cid:12)2 (18) 4 (cid:12)F F (cid:12) 5 1 with λ = 1 1+exp(−a) r F = F (α ,β ,γ ,λ) 1 2 1 1 1 1 F = F (α ,β ,γ ,λ) 2 2 1 2 2 2 F = F (α +1,β +1,γ +1,λ) (19) 3 2 1 1 1 1 F = F (α +1,β +1,γ +1,λ) 4 2 1 2 2 2 F = [−µ+λ(µ−ν)]F +λ(1−λ) α1β1F 5 1 γ1 3 F = [µ−λ(µ+ν)]F +λ(1−λ) α2β2F 6 2 γ2 4 and  α = (cid:0)µ+ν + 1(cid:1)− ν0   β = (cid:0)µ+ν + 12(cid:1)+ ν20   2 2 γ = 1+2µ (20)  µ2 = r2(m2 −E2),µ = irk    ν2 = r2(cid:2)m2 −(E +eV0)2(cid:3), ν = irp with p real  ν = (cid:112)(1−2reV )(1+2reV ) 0 0 0 Remark that one will distinguish two cases: |E| > m, i.e. k is real, which solutions are called scattering states [2,3,4], and |E| < m, i.e. k is imaginary and which solutions are bound states.  (cid:0) (cid:1)  (cid:0) (cid:1) α = −µ+ν + 1 − ν0 α = µ+ν + 1 − ν0  1 (cid:0) 2(cid:1) 2  2 (cid:0) 2(cid:1) 2 β = −µ+ν + 1 + ν0 , β = µ+ν + 1 + ν0 (21) 1 2 2 2 2 2  γ = 1−2µ  γ = 1+2µ 1 2 6 3 Bound states To get the transmission coefficient for bound states in terms of E and of (−eV ), we proceed to solve numerically the equation (18). When varying 0 the depth (−eV ) of the square well, we get: 0 Figure 2: The T coefficient in Figure 3: The T coefficient in terms of the depth (−eV ) terms of the depth (−eV ) 0 0 of the potential, for of the potential, for a = 2, E = −2m and m = 1 a = 4, E = −2m and m = 1 and when varying the energy E of the particle, we get: Figure 4: The T coefficient in Figure 5: The T coefficient in terms of the energy E for terms of the energy E for m = 1,eV = 4,a = 2. The m = 1,eV = 4,a = 4. 0 0 energies of the bound states are The energies of the bound states depicted by dashed lines. are depicted by dashed lines. Fig. 2 and Fig. 3 show that as in the Dirac [10] and the KG cases [6], the transmission coefficient vanishes for values of the potential strength 7 E−m < −eV < E+m, and transmission resonances appear for V > E+m. 0 0 They also show that the width of the transmission resonances decreases as the parameter a decreases. Fig. 4 and Fig. 5, show that the occurrence of the transmission res- onances increases with the width a of the square well. As in the case of the Dirac particle [10], we have significant structures of resonance in the particle continuum for E > m, and in the antiparticle continuum for E < −eV −m. Antiparticles with lower energy (−eV −m < E < −eV +m) 0 0 0 only penetrate the well with a probability which decreases with the width a of the well. Hence T is about zero in our case. However, in the domain −eV + m < E < −m(=⇒ eV > 2m), there is the possibility that the in- 0 0 coming wave meets a bound state, and thus penetrates the potential domain more or less unhindered. At the point where by extrapolation of the spec- trum of the bound states (see Fig. 6), one would expect the quasi bound state, T is equal to 1. The dived bound state in this way becomes perceptible as a resonance in the scattering spectrum below E = −m. Figure 6: Eigenvalue spectrum for m = 1,a = 4. In Fig. 6, the energies of the dived states corresponding to resonances are depicted by dashed lines. They are extracted from the maxima of the transmission coefficients of Fig. 5 By the following, one wants to get the dependence of the spectrum of bound states (i.e. |E| < m) on the potential strength V . One uses for this 0 aim, the unitary condition that coefficients R and T verify, i.e. R+T =1, 8 which leads to: (cid:34) (cid:35) 1=1 (cid:12)(cid:12)λ2µ(cid:12)(cid:12)2 (cid:12)(cid:12)(cid:12)F6(cid:12)(cid:12)(cid:12)2 +(cid:12)(cid:12)(cid:12)F2(cid:12)(cid:12)(cid:12)2 (22) 2 (cid:12)F (cid:12) (cid:12)F (cid:12) 5 1 So 2 = |λ2µ|2 (cid:12)(cid:12) [µ−λ(µ+ν)] F (α ,β ,γ ,λ)+λ(1−λ) α2β2 F (α +1,β +1,γ +1,λ) (cid:12)(cid:12)2 (cid:12) 2 1 2 2 2 γ2 2 1 2 2 2 (cid:12) (cid:12)(cid:12)[−µ+λ(µ−ν)]2F1(α1,β1,γ1,λ)+λ(1−λ) αγ11β12F1(α1 +1,β1 +1,γ1 +1,λ)(cid:12)(cid:12) (cid:12)(cid:12)2F1(α2,β2,γ2,λ)(cid:12)(cid:12)2 +(cid:12) (cid:12) (23) (cid:12) F (α ,β ,γ ,λ)(cid:12) 2 1 1 1 1 One proceeds to solve numerically the equation (23) and thus one determines the energy spectrum of the bound solutions for several sets of parameters r and a, using the Gauss hypergeometric function: Γ(γ)Γ(β −α) Γ(α−β +1)Γ(γ −α−β) F (α,β,γ,z) = (−z)−α × Γ(β)Γ(γ −α) Γ(1−β)Γ(γ −β) Γ(γ)Γ(α−β) Γ(β −α+1)Γ(γ −β −α) + (−z)−β × |arg(−z)| < π Γ(α)Γ(γ −β) Γ(1−α)Γ(γ −α) (24) For that, one puts λ = λ−iε, then: (cid:15) F (α,β,γ,λ) = limF (α,β,γ,λ ) (cid:15) (cid:15)→0 so one obtains: 9 Figure 7: Bound state spectrum Figure 8: Bound state spectrum for m = 1,a = 1,r = 0.00015 for m = 1,a = 4,r = 0.0003 In Fig. 7(resp. Fig. 8), the bound state for the antiparticle appears for the domain 2.0004 < eV < 2.0006(resp. 2.002 < eV < 2.003 ). For 0 0 eV (cid:39) 2.00055m(resp. eV (cid:39) 2.0022m), the well becomes supercritical. The 0 0 lowest bound state enters the lower continuum and can there be realized as a resonance in the transmission coefficient. This critical value is depicted by (eV ) , and its corresponding energy by E . The appearance of these bound 0 cr cr antiparticle states is corresponding with the short range of the potential. Figure 9: Critical potential eV0cr Figure 10: Critical energy Ecr versus the shape parameter r for versus the shape parameter r for m = 1,a = 4 m = 1,a = 4 Fig. 9 shows that when the shape parameter r increases, the critical potential value eV where the bound antiparticle mode appears to coalesce 0cr 10

See more

The list of books you might like

Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.