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Nuclear spin irreversible dynamics in crystals of magnetic molecules Alexander Burin Department of Chemistry, Tulane University Motivation 1. Nuclear spins serve as a thermal bath for electronic spin relaxation 2. Nuclear spins form fundamentally interesting modeling system to study Anderson localization affected by weak long-range interaction 3. Nuclear spins can be used to control electronic spin dynamics (slow down or accelerate). It is sensitive to electronic polarization and dimension Outline 1. Crystals of magnetic molecules; frozen electronic spins 2. Nuclear spins in distributed static field 3. Spectral diffusion and self-diffusion 4. What next? 5. Acknowledgement Magnetic molecules Molecular magnets (more than systems are synthesized already) 100 Mn, Fe, Ni, Co, … based macromolecules; S = 0, 1/2, 1, … , 33/2 Crystals of magnetic molecules 15 Å The clusters are assembled in a crystalline structure, with relatively small (dipolar) inter-cluster interactions Magnetic Anisotropy 2 ˆ Hanisotr DSz Sz -10 -5 0 5 0 -10 Energy (K) z -20 -30 -40 -50 -60 Th-A T QT -70 The magnetic moment of the molecule is preferentially aligned along the z – axis. 10 Magnetic Anisotropy Sz -10 -5 0 5 10 0 Energy (K) -10 -20 -30 -40 -50 -60 Th-A T 10-11 K QT -70 The actual eigenstates of the molecular spin are quantum superpositions of macroscopically different states 2 ˆ H 100Dsz sx , 0 Outline 1. Crystals of magnetic molecules; frozen electronic spins 2. Nuclear spins in distributed static field 3. Spectral diffusion and self-diffusion 4. What next? 5. Acknowledgement Energy Single nuclear spin (H) 10-2 K At low temperature, the field produced by the electrons on the nuclei is quasi-static Zeeman energy distribution (55Mn) Inuclear = 5/2 Three NMR lines corresponding to the three non-equivalent Mn sites Finite width of lines due to interaction with all electronic spins f(E) Hˆ i Ei Siz Interaction of nuclear spins Magnetic dipole moments Vij mi m j 3n n 3 ij R ~ 10 K Ei , j 6 1 ˆ H tot Ei si Vij si s j 2 i , j , , i Outline 1. Crystals of magnetic molecules; frozen electronic spins 2. Nuclear spins in distributed static field 3. Spectral diffusion and self-diffusion 4. What next? 5. Acknowledgement Scenario for spin self-diffusion Assume the presence of irreversible dynamics in ensemble of nuclear spin. Transitions of spins stimulates transitions of other spins due to spin-spin interactions Can this process result in self-consistent irreversible dynamics? Mechanism of spin diffusion Single spin evolution (H) Sz=-1/2 B 40T ~ 10-6 K ~ 0.01K Sz=1/2 Single spin flip is not possible because the energy fluctuation ~10-6K due to “dynamic” nuclear spin interaction is much smaller than the static hyperfine energy splitting ~10-1K Two spin “flip-flop” transition Transition can take place if Zeeman energies are in “resonance” |1-2| < m1m2 u0 V~ 3 ~ 3 R12 R12 Transition probability is given by (Landau Zener) 1 2 2V 2T 1 1 exp T1 is the spectral diffusion period Transition rate induced by spectral diffusion W (t ) t ndR f ( E )dE f ( E )u0 n T1 2u 2T1 1 exp 6 R u n 0 u t u0 n T1 E E dR t 8 21/ 4 3 2 1/ 4 W (t ) T1 9 u0 nT1 2 f ( E )dEu0 n 2 3 Self-diffusion rate Overall relaxation rate is determined by the external rate plus the stimulated rate 1 1 1 8 2 ~ ~ T1 T1 T1 1/ 4 3 9 2 1/ 4 ~ u0 nT1 2 f ( E )dEu0 n Solution: 1 1 64 21/ 2 4 1/ 2 u0 n , k ~ k 1 T1k 27 T1 1 T1 yields ~ k T1 f 2 ( E )dEu0 n 2 Nuclear spin relaxation and decoherence rates d=3, agrees with Morello, et al, Phys. Rev. Lett. 93, 197202 (2004) 1 T1diff 64 21/ 2 4 1/ 2 u0 n 27 f 2 2 ( E )dEu0 n 100s 1 1 dE 2 u0 n 8 2 u0 n 2 1 f ( E ) dE u n 1000 s 0 T2 dt 3 T1 9 3 d=2 u0 n 3 / 2 1 1000 T1 u0 n 3 / 2 1 100 T2 f f 2 2 ( E )dEu0 n ( E )dEu0 n 3/ 2 3/ 2 10 6 8 10 3 2 s 1 s 1 Outline 1. Crystals of magnetic molecules; frozen electronic spins 2. Nuclear spins in distributed static field 3. Spectral diffusion and self-diffusion 4. What next? 5. Acknowledgement What next? Spin tunneling is suppressed in 2-d: subject for experimental verification? Isotope effect in T2 can be predicted, subject to test Effect of polarization on the nuclear spin relaxation: 1/T2~1/<M2>, 1/T1diff~1/<M2>2 to be tested Outline 1. Crystals of magnetic molecules; frozen electronic spins 2. Nuclear spins in distributed static field 3. Spectral diffusion and self-diffusion 4. What next? 5. Acknowledgement Acknowledgement To coworkers: Igor Tupitsyn & Philip Stamp To Tulane Chemistry Department Secretary Ginette Toth for help in organizing this meeting Funding by Louisiana Board of Regents, Tulane Research and Enhancement Fund and PITP 2 2 u 3T1 2 u0 n f ( E )dEf ( E ) t ndR 1 exp 6 R u n 2 3 T1 0 u u0 n 2 1 f ( E )dEf ( E ) t n dR 1 4u02 3T1 3 T1 1 6 R u0 n 2 u n 1 2 0 f ( E )dEt n dx1 1 T1 0 1 2 x 4 2 2 9 4u02 3T1 u0 n 2 4 2 2 9 4u0 n3T1 2 u0 n 1 2 f ( E )dEt dx1 1 T1 0 1 2 x t 8 21/ 4 3 2 1/ 4 W (t ) T1 9 u0 nT1 2 f ( E )dEu0 n 1 64 21/ 2 4 1/ 2 u0 n T1 27 f 2 ( E )dEu0 n 2 Non-adiabatic “Floquet” Regime Level crossing when E1-E2-n =0, n=0,1,-1,2,-2, …a/ Transition amplitudes: V12,n= (a/)1/2U0/R3 E E1 Level crossing neighbors TPU0 E Spectral diffusion covers level splitting: <TPU0 inevitable E1 level crossing when |E1-E2|<a, otherwise (>TPU0) a special consideration is needed Non-adiabatic Transitions between Floquet States Number of level crossings during the spectral diffusion cycle (1): Ncr~TPU0/ Transition probability per single crossing Ptr ~ Vtr2/(TPU0/1) ~ ~ (U0Pa)2(/a)1/(TPU0)=a(PU0)21/(TPU0) Self-consistent transition rate 1/1=a(PU0)21/(TPU0)1Ncr ~ a(PU0)2 coincides with the non-adiabatic Landau-Zener expression Current Status Frequency 1/1 1/2 Mechanism <T2(PU0)4/a T(PU0)3 T(PU0)2 Quasistatic field, Linear Regime T2(PU0)4/a<<a(PU0)2 (a)1/2(PU0) (T2a)1/4(PU0) a(PU0)2<<T(PU0) TPU0< Adiabatic field control a(PU0)2 (aT)1/2(PU0)3/2 Non-adiabatic “Landau-Zener” or “Floquet” regimes ? ? ? Non-Linear Self-Consistent Regime TPU0 < TPU0 E E1 Level crossing is permitted with the only one of n=a/ Floquet states, transition amplitude goes down by n-1/2: RENORMALIZATION: PPa/, U0U0(/a)1/2 Relaxation rate Rate of the energy change v = Amplitude/Quasi-period = TPU0/1, Transition amplitude 0p ~ U0(/a)1/2 PTPU0a/ Non-adiabatic case: a/(T(PU0)2)2 < v = TPU0/1 Transition probability per one crossing: aT ( PU0 ) 1 Wtr . v TPU0 2 0p 1 Transition rate: 1,sd (Remember many-body theory) 1 1 2 Wtr (a / )T ( PU0 ) 4 3 Summary Frequency 1/1 1/2 Mechanism <T2(PU0)4/a T(PU0)3 T(PU0)2 Quasistatic field linear regime T2(PU0)4/a<<a(PU0)2 a(PU0)2<<T(PU0) (a)1/2(PU0) (T2a)1/4(PU0) Adiabatic field control a(PU0)2 (aT)1/2(PU0)3/2 Non-adiabatic regime TPU0<<a (a/)T(PU0)3 (a/)1/2T(PU0)2 Non-linear selfconsistent regime a<<T T(PU0)3 T(PU0)2 Fast field linear regime Conclusion (1) Interaction induced relaxation is very complicated under the realistic conditions, non-linearity takes place at a>TPU0 ~10-5K (10mK). For an elastic field a==104K. One needs ~10-9 – 10-8 for the true linear regime. For an electric field a=el, assuming ~1D wanted el ~ 40V/m. Looks almost impossible (see, however, Pohl and coworkers, 2000). (2) Theory predicts both linear temperature dependence and/or the absence of any temperature dependence. A careful treatment of existing measurements is needed (backgrounds, etc.) (3) It is not clear whether the thermal equilibrium of phonons and TLS is fully established. This can change the way of the treatment of experimental data Acknowledgement (1) Yuri Moiseevich Kagan (2) Leonid Aleksandrovich Maksimov (3) Il’ya Polishchuk (4) Fund TAMS GL 211043 through the Tulane University Dedication To Professor Siegfried Hunklinger with the best wishes of Happy 65th birthday and the further great successes in all his activities