Page 192 - Principles and Applications of NanoMEMS Physics
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180                                                     Chapter 4


             the  separation  required between adjacent donors. In the presence  of a
             magnetic field  B  z , and assuming a donor nucleus with  I =  2 / 1   embedded
             in a silicon host, the interaction in question,  namely,  the  nuclear-spin
             interaction, is given by the Hamiltonian [202],
                                        N
                            e
               H e− N  =  µ B Bı −  g  N  µ N Bı +  Aı  e  ı ⋅  N  ,                                          (3 )
                                                                            7
                            z
                                        z
             where  µ  is the nuclear magneton,  σ  are the Pauli spin matrices,  g  is the
                    N                                                   N
             nuclear g-factor, and  A =  8  ʌµ  g  µ  Ȍ  () 0  2   is the  contact  hyperfine
                                     3    B  N  N
             interaction energy when the probability density of the electron wavefunction,
             Ȍ  () 0  2   is evaluated at the nucleus. Clearly, examination of  Eq.  (3 )
                                                                            7
             indicates that the interaction energy is a directly proportional to the magnetic
             field and is a strong function of the wave function probability density at the
             nucleus. A trade-off exists, however, because for electrons in their ground
             state the frequency separation between nuclear levels is [202],

               hȞ =  2g  µ  B + 2A +  2A 2  ,                                                              (3 )
                                                                            8
                  A     N  N
                                     µ  B
                                      B
             which, for fields  B <  3.5T  is dominated by the second term. Thus, in this
             regime  the  magnitudes of the nuclear magneton and the wavefunction
             probability density at the nucleus take on a dominant character.
               To perform arbitrary rotations on the nuclear spin, Kane indicates that it is
             necessary to alter its precession frequency in comparison with that resulting
             from the applied magnetic field  B   [202]. This is accomplished by
                                              ac
             exploiting the fact that the proximity of the donor-nuclear spin system to the
             A gate  allows the hyperfine interaction to be reduced by shifting  the
             envelope of the electron-donor wavefunction away from the nucleus, i.e., by
                          2
             reducing  () 0Ȍ  . In essence, such a shifting alters the frequency, Eq. (35),
             and causes the nuclear spin-donor system to behave as a voltage-controlled
             oscillator producing, for a donor placed  200  Å under  the  gate,  a  tuning
             parameter of the order of 30 MHz/V [202].
               In addition to the single-qubit  rotation,  the  two-qubit  C-NOT  operation
             must be implemented in order to enable general quantum computations. In
             the  context  of the nuclear spin-donor system,  accomplishing this  requires
             developing the  ability  to induce nuclear-spin exchanges  between two
             nucleus-electron spin systems. The interaction between two such systems is
             captured by the Hamiltonian [202],

               H =  H () AB +  ı  1N  ı ⋅  2e  +  A  ı  2N  ı ⋅  2e  +  Jı  1e  ı ⋅  2e  ,                         (3 )
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