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Bose-Einstein Condensates in Rotating Traps and Optical ... - BEC

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140 Array of Josephson junctions<br />

For a typical double well system, the m-dependence <strong>in</strong> front of the cos Φ of the Hamiltonian<br />

(10.39) is not important. The gas must be very dilute for it to be relevant (see [1] chapter 15<br />

for a discussion of this issue). Neglect<strong>in</strong>g this contribution, the Hamiltonian <strong>and</strong> the equations<br />

of motion read<br />

HJ = − EC<br />

2 m2 + EJ cos Φ , (10.46)<br />

¯h ˙m = EJ s<strong>in</strong>(Φ) , (10.47)<br />

¯h ˙ Φ=−ECm, (10.48)<br />

with the Josephson tunnel<strong>in</strong>g energy<br />

EJ = Nδgn=0 . (10.49)<br />

A characteristic property of such a Josephson junction is its possibility to exhibit plasma<br />

oscillations of frequency<br />

√<br />

ECEJ<br />

ωP =<br />

. (10.50)<br />

¯h<br />

They correspond to harmonic small amplitude oscillations around m = 0, Φ = 0 of the<br />

pendulum described by the equations (10.47,10.48). The existence of such oscillations was<br />

first proposed by Josephson with respect to tunnel<strong>in</strong>g currents between superconductors [146].<br />

Us<strong>in</strong>g (10.35,10.49) we can rewrite ωP <strong>in</strong> the form<br />

<br />

2δgn=0˜gn<br />

ωP =<br />

. (10.51)<br />

¯h<br />

The junction described by the more complicated Hamiltonian (10.39) exhibits plasma oscillations<br />

with the frequency<br />

<br />

δgn=0(δgn=0 + NEC)<br />

<br />

δgn=0 (δgn=0 +2˜gn)<br />

ωP =<br />

=<br />

. (10.52)<br />

¯h<br />

¯h<br />

It is <strong>in</strong>terest<strong>in</strong>g to note that the lowest Bogoliubov b<strong>and</strong> excitation with q = π/d is the<br />

physical analogue for a lattice of the plasma oscillations for a s<strong>in</strong>gle Josephson junction:<br />

As discussed above, the excitation at this value of q <strong>in</strong>volves a particle exchange between<br />

neighbour<strong>in</strong>g sites. The correspond<strong>in</strong>g frequency is given by (see Eq.(10.25))<br />

<br />

¯hω(q = π/d) = 2δgn=0 [2δgn=0 +2˜gn] , (10.53)<br />

where consistenly with the discussion of the Josephson Hamiltonian we have set δ = δgn=0<br />

<strong>and</strong> κ−1 =˜gn. This frequency co<strong>in</strong>cides with (10.52) apart from a factor √ 2. This difference<br />

is due the fact that each site of the lattice exchanges particles with two neighbour<strong>in</strong>g wells<br />

<strong>in</strong>stead of with just one as <strong>in</strong> the double well case.<br />

A further <strong>in</strong>terest<strong>in</strong>g connection between the lattice <strong>and</strong> the double well case emerges when<br />

compar<strong>in</strong>g the equations of motion (10.47,10.48) with those for the center-of-mass motion<br />

<strong>in</strong> the tight b<strong>in</strong>d<strong>in</strong>g regime given the comb<strong>in</strong>ed presence of lattice <strong>and</strong> harmonic trap (see<br />

Eqs.(9.67,9.68)): The two sets of equations are formally identical if one identifies<br />

m ↔ NZ<br />

, (10.54)<br />

d<br />

Φ ↔ kd , (10.55)<br />

EC ↔ mω2 zd2 . (10.56)<br />

N

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