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Collins asymmetry in field ionisation of hydrogen

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Collins asymmetry in field ionisation of hydrogen

X. Artru, E. Redouane-Salah

To cite this version:

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COLLINS ASYMMETRY IN FIELD IONIZATION OF HYDROGEN1

X. Artru1 † and E. Redouane-Salah2 †

(1) Universit´e de Lyon, CNRS/IN2P3 and Universit´e Lyon 1, IPNL, France (2) Universit´e de M’sila, Facult´e des Sciences, D´epartement de Physique

and LPMPS, Universit´e de Constantine 1, Algeria

† E-mail: x.artru@ipnl.in2p3.fr Abstract

An effect similar to the Collins asymmetry is found in the ionization of a hydro-gen atom by a static electric field E. When the initial electron possesses an orbital angular momentum hLi transverse to the field, the mean transverse velocity hvTi

of the final electron points in the direction of E × hLi. However hLi is oscillating in time due to the linear Stark effect, making hvTi oscillate.

Introduction. An atom can be ionized by a sufficiently strong static electric field E thanks to the tunnel effect. This process has a strong similarity with the production of a quark-antiquark pair (q ¯q) in a QCD string. If the initial electron has an orbital angular momentum perpendicular to E, the average transverse velocity hvTi should be nonzero and in the direction of hLi × F, where F = −eE is the external force [1]. We refer to it as the v.(L×F) asymmetry. The mechanism(Fig.1-left) looks like the string + 3P0 mechanism (Fig.1-right) of hyperon polarization [2] and Collins effect [1, 3].

At variance with the string + 3P

0 mechanism, the Schwinger mechanism of q ¯q pair creation yields no v.(L×F) asymmetry [1]. Thus the question of such an asymmetry in string breaking remains open. It is at least instructive to study it in atomic physics.

1 Behavior of an H atom in an external electric field

We consider an hydrogen atom in an static electric field E = −(F/e) ˆz. At small F the linear Stark effect just splits the nth energy level in 2n − 1 sublevels separated by2 ω = 3nF/2. Stark states are the eigenstates of H0−F z = p2/2 − 1/r − F z in the F → 0 limit. For large enough F ionization by tunneling becomes important and Stark states move into resonances of complex energy E = ER− iγ/2. Using the parabolic coordinates ξ=r-z, η=r+z, ϕ=arg(x + iy), their wave functions have the separable form [4]

Ψ = ξ−1/2Φ(ξ) η−1/2χ(η) eimϕ (1) where Φ(ξ) verifies

∂2Φ/∂ξ2+E/2 + Zξ/ξ − (m2− 1)/(4ξ2) − F ξ/4 Φ(ξ) = 0 . (2) and χ(η) an analogous equation with F → −F and Zξ → Zη = 1 − Zξ. Stark states are labeled |nξ, nη, mi, where nξ and nη are the numbers of nodes of Φ(ξ) and χ(η), linked

1

Presented at XVI Advanced Research Workshop on High Energy Spin Physics (DSPIN-13)(Dubna, October 8-12, 2013)

2

In this paper we use atomic units: ~/(meαc) = 0.0529 nm for length, ~/(meα 2 c2 ) = 2.42 10−17 s for time, meα 2 c2

= 27, 2 eV for energy and m2 eα

3

c2

/~ = 5.14 109

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kT !kT force L electric field atom e -tunnel

-q

T

q

T

L

q

!q

string string

Figure 1: Left: semi-classical motion of the electron extracted form the hydrogen atom by a strong field E, when the electron is initally in a Ly = +1 state. Right: String + 3P

0 mechanism correlating the tranverse momentum and the transverse polarization of a quark created in string decay [1, 3].

by nη + nξ + |m| + 1 = n and fixing Zξ = (n + nξ− nη)/(2n). With the change of vari-ables pξ/n eiϕx+iˆy, ˆΦ(ˆx, ˆy) ≡ ξ−1/2Φ(ξ) eimϕ is the wave function of a 2-dimensional harmonic oscillator of angular momentum m and energy ǫξ = 2nZξ = 2nξ+ |m| + 1. L⊥ oscillations. Stark states are also eigenstates of Az, where A is the Laplace-Runge-Lenz-Pauli vector

A = r/r + (L × p − p × L)/2 . (3) For F =0, hAzi=2hzi/(3n2) = (n

η− nξ)/n. For F 6=0 the transverse components (Lx, Ly) and (Ax, Ay) are not conserved. Starting from a Ly eigenstate, hLyi oscillates in quadra-ture with hAxi, as pictured in Fig.2, with the period 2π/ω. Let us take as an example the initial state |n=2, Ly= +1i, whose wave function is

Ψ(r, t = 0) = 8−1π−1/2(z + ix) e−r/2 = 0.5( |010i − |100i + i|001i + i|00 − 1i ) . (4) At t 6= 0 it evolves as

Ψ(t) = 0.5 eit/8 e+iωt|010i − e−iωt|100i + i|001i + i|00 − 1i

(5) = eit/8



cos2 ωt

2 |Ly= +1i − sin 2 ωt 2 |Ly= −1i + i √ 2sin(ωt)|l =0i  . (6) Thus the atom oscillates between three Ly eigenstates.

time

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2 Tunneling amplitudes

The external force is confining in ξ and changes Φ(ξ) only little. Tunneling bears on χ(η). The wave function at large η describes the escaped electron. Using, as in Ref. [4], the JWKB method to lowest order in F , one obtains for the state |ii ≡ |nξ, nη, mi

Ψi(r, t)η→∞ ≃ aiΦi(ˆˆ x, ˆy) exp{(−iδEi− γi/2)t′} B(η, t) . (7) ai is the tunneling amplitude normalized to |ai|2 = γi, δEi is the Stark shift, ˆΦi(ˆx, ˆy) is the 2-D oscillator wave function normalized to hˆΦiΦii = 1 and

B(η, t) = (4F η3)−1/4 exph(i/3)√F (η − ηF)3/2+ it/8 + 5iπ/4 i

. (8)

ηF ≡ 1/(n2F ) is near the tunnel exit and t′ ≡ t −p(η − ηF)/F is the classical electron exit time. For n=2 the amplitudes are

a1 ≡ a010 = iq a00+1,

a2 ≡ a00+1 = a00−1 = 2−5/2F−1 exp [−1/(24F )] , a3 ≡ a100 = a00+1/(iq) ,

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with q = e−3/2/2F . The widths γi = |a

i|2 agree with Slavjanov’s result [5].

3

v.(L×F) asymmetry for the initial state |n=2, L

y

= +1i

With the initial state (4) the escaped electron density is, according to (5,7-8), |Ψ(r, t)|2η→∞ = (4F η3)−1/2 Φ(ˆˆ x, ˆy, t ′ ) 2 (10) with η ≃ 2z, (ˆx, ˆy) ≃ (x, y)/√2nz. In the n=2 case,

ˆ Φ(t′) = 0.5a1Φ010ˆ e(iω−γ1/2)t′ − a3Φ100ˆ e(−iω−γ3/2)t ′ + ia2( ˆΦ00+1+ ˆΦ00−1) e−γ2t′/2 . (11) |Ψ(r, t)|2 looks like the density of a classical electron cloud falling freely in the force field F. An electron leaving the tunnel at time t′ with the transverse velocity v⊥ follows the parabola of fixed (ˆx, ˆy) ≃ v⊥/√2F . The interference between even- and odd-m terms of

ˆ

Φ(t′) yields the v.(L×F) asymmetry, which is t-dependent. A measure of it is A(t′

) ≡ hvxi/∆vx = hˆΦ(t′)|ˆx|ˆΦ(t′)i/ q

hˆΦ(t′)|ˆx2Φ(t)i ; (12) A(t′= 0) = 81/2 q2+ 8 + 3 q−2−1/2 . (13) Like Ly, A(t′) changes sign at the Stark frequency, giving the ”crawling snake” of Fig.3 [6].

Conclusion.

This study shows that the v.(L×F) effect does exist in field ionisation, but is oscillating in time. Several constraints make its search challenging:

• Radiative transition may compete with field ionization.

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atom

Figure 3: ”Crawling snake” motion of hxi versus z of the escaping electron. As t grows the undulations move to the right.

• A(t′) is fast oscillating, therefore one may only measure its time-averaged hAi. This one is large only if γi &ω, so that ionization is faster than oscillation.

These constraints are satisfied with a large enough field. In the n=2 case this field is too strong to be produced in laboratory. Hopefully, our results can be generalized to large n (Rydberg states), where the required field scales like n−4 [7]. The vT distribution can be measured by the photoelectron imaging techniques [8, 9].

Our formulae, obtained at lowest order in F , cannot be applied at the required field. Accurate numerical methods are given in [10, 11]. Nevertheless the above conclusions should remain qualitatively correct.

References

[1] X. Artru and J. Czyzewski, Acta Phys. Polonica C B29 (1998) 2015.

[2] B. Andersson, G. Gustafson, G. Ingelman and T. Sj¨ostrand, Phys. Rep. 97 (1983) 31. [3] X. Artru, J. Czyzewski and H. Yabuki, Zeit. Phys. C 73 (1997) 527.

[4] L.D. Landau, E.M. Lifshitz, Course of theoretical physics, Vol. 3,Quantum Mechanics, Pergamon press, London.

[5] Yu. Slavjanov, Problemi Matematicheskoi Fiziki (Leningrad: Lenigrad State Univer-sity, 1970), pp 125-34.

[6] E. Redouane-Salah and X. Artru, AIP Conf. Proc. 1444, 157 (2012). [7] X. Artru and E. Redouane-Salah, in preparation.

[8] Yu.N. Demkov, V.D. Kondratovich and V.N. Ostrovskii, Pis’ma Zh. Eksp. Teor. Fiz. 34, 425 (1981) [JETP Lett. 34, 403 (1981)].

[9] A.S. Stodolna, A. Rouze, F. L´epine, S. Cohen, F. Robicheaux, A. Gijsbertsen, J.H. Jungmann, C. Bordas and M.J.J. Vrakking, Phys. Rev. Lett. 110, 213001 (2013). [10] R.J. Damburg and V.V. Kolosov, J. Phys. B 9, 3149 (1976), B 11, 1921 (1978), B

12, 2637 (1979).

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