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Spin-flip operators

Figure 4. Hierarchy of the SF models. Similar to the non-SF SR methods, the SF models converge to the exact n-electron wavefunction when the spin-flipping operator 0 includes up to n-tuple excitations. For example, the SF-CCSD model... Figure 4. Hierarchy of the SF models. Similar to the non-SF SR methods, the SF models converge to the exact n-electron wavefunction when the spin-flipping operator 0 includes up to n-tuple excitations. For example, the SF-CCSD model...
Another class of method tries to generate MR states of interest via the action of an excitation operator on a simple base function, usually of the ground state. The linear response-based theories based on CC reference functions have been proposed quite some time ago to achieve this goal, starting from the HF or ROHF ground reference state [22-25]. An interesting variant to handle non-trivial open-shell states via a spin-flip operator [26] has revived the interest in the generalization of the CC-based linear response theory to open-shell states. [Pg.584]

Combining (IIS.7.11) and (1 IS.7.12), we obtain the following result for the triplication of the spin-flip operator to a CSF with 2m singly occupied orbitals and total spin projection zero ... [Pg.67]

Applying the spin-flip operator to the wave function 0), we obtain... [Pg.67]

In this exercise, we consider the spin-flip operators - that is, unitary operators that transform alpha operators into beta operators and visa versa. Although we shall investigate only the effect of the spin-flip operators on the creation operators, we note that the corresponding results for the annihilation operating are readily obtained by taking the adjoints of the relations for the creation operators. [Pg.97]

Show that these operators are spin-flip operators in the sense that ... [Pg.97]

The two terms on the right-hand side cancel, as may be seen by a relabelling of the spins or more formally by introducing the unitary spin-flip operator Ux defined in (3E.4.9) of Exercise 3.4 ... [Pg.520]

The last equality follows since the Hamiltonian is unaffected by the spin-flip operator and since the sign change introduced by applying the spin-flip operator to the closed-shell state HF)... [Pg.520]

Problem 13.2 Calculate the amount of energy required to spin-flip a proton in a spectrometer oper-... [Pg.442]

It is the change of sign of individual integrals due to spin integration that lets the matrix element survive. In other cases, where s+i or s i are involved, spin flips of individual orbitals occur in addition. Because of these individual spin flips, the spin-orbit operator can alter not only the Mg quantum number by AMs = 0, 1, but also may change the spin quantum number S by at most one unit (i.e., AS = 0, 1). [Pg.154]

Starting from n)> we notice that it is neither an eigenstate of a Heisenberg Hamiltonian nor an eigenstate of the total spin operator S2. For instance, the Neel state is not invariant under the action of the nearest-neighbor XY spin terms of the Heisenberg Hamiltonian, which may produce a spin-flip on two nearest-neighbor sites at a time with respect to n). These XY excitation operators from the vacuum 4>n > can be written as... [Pg.735]

Calculate the amount of energy required to spin-flip a proton in a spectrometer operating at 300 MHz. Does increasing the spectrometer frequency from 200 to 300 MHz increase or decrease the amount of energy necessary for resonance ... [Pg.442]

Refinements of direct calculations or of the preceding trial-and-error procedure utilize iterative computer programs. The program of Castellano and Bothner-By (LAOCN3) iterates on peak positions, but requires assignments of peaks to specific spin flips. The program of Stephenson and Binsch (DAVINS) operates directly on unassigned peak positions. [Pg.116]

We consider individual bosonic reservoirs / ,.. .., Fj with finite thermal energy ksT characterized by mode operators Ajk, Ajk, etc. Environmentally induced spin flips can be described by the interaction Hamiltonian... [Pg.219]

Yj for spin-flip. The model is that of Luther and Emery [lj, before they introduce new quasi-fermion operators to obtain a gap at Yll — - 3/s. The free energy corresponding to... [Pg.58]

Steps (la) and (Ic) can be regarded as two resonant pulses (of opposite phase) in the Ramsey separated-field method of spectroscopy [52]. We can see that if step (b) is active (thereby changing the agn of the 11 > n=l) component of the wave fiinction) then a spin flip is produced by the Ramsey fields. If aep (lb) is inactive, the net effect of the Ramsey fields is to leave the spin state unchanged. This CN operation can be incorporated to provide an overall CN operation between two ions in an ensemble of N ions if we choose the ion oscillator mode to be the center-of-mass (COM) mode of the ensemble. Specifically, to realize a controlled-not C k between two ions (m = control bit, k = target bit), we first assume the COM is prepared in the zero-point aate. The initial state of the system is therefore given by... [Pg.57]

In the A -operator formalism the relations (35), (37) and (38) are built in to the excitation operators. A full definition is given by Jensen et al. [38] who introduce the pseudo quantum number Mk to play the role of the non-relativistic Ms quantum number. This number is defined as Mk = (M - M 2 with M and Mp the number of occupied unbarred and barred spinors, respectively. The analogue of the non-relativistic spin-restricted excitation operators are now those that preserve Mk, either by disallowing spin flips... [Pg.319]


See other pages where Spin-flip operators is mentioned: [Pg.67]    [Pg.521]    [Pg.67]    [Pg.521]    [Pg.94]    [Pg.323]    [Pg.113]    [Pg.181]    [Pg.910]    [Pg.120]    [Pg.387]    [Pg.16]    [Pg.47]    [Pg.649]    [Pg.16]    [Pg.119]    [Pg.154]    [Pg.296]    [Pg.94]    [Pg.94]    [Pg.326]    [Pg.20]    [Pg.113]    [Pg.358]    [Pg.83]    [Pg.38]    [Pg.261]    [Pg.69]    [Pg.73]    [Pg.235]    [Pg.75]   
See also in sourсe #XX -- [ Pg.97 ]




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