Electron effective mass in an ultra-high mobility GaAs/AlGaAs quantum well from MIRO and EPR experiment on DPPH Sergei Studenikin, Geof Aers, and Andy Sachrajda National Research Council of Canada, Ottawa, Canada Q. Shi, and M. A. Zudov School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota, USA L. N. Pfeiffer, and K. W. West Department of Electrical Engineering, Princeton University, Princeton, New Jersey, USA 1 Three first MIRO/ZRS papers: number of scitations per year Three first papers in the MIRO field: Number of scitations per year Number of citations Zudov PRL PRB 2001 Mani Nature 2002 Zudov PRL2003 Total 100 50 0 2002 2004 2006 2008 2010 2012 2014 Year 2 First time use of “MIRO” Joan Miró (1893-1983) 3 Niko Pirosmani (1862-1918) Electron effective mass in an ultra-high mobility GaAs/AlGaAs quantum well from MIRO and DPPH EPR experiment Outline 1) Introduction: methods for m*-measurements 2) Sample and Experimental setup 3) B calibration with DPPH in 5-70 mT range 4) m*MIRO measurement 5) Conclusions 5 Why it is interesting to precisely measure m*? m*0 is a band parameter m* (w, Ei, B, ….) is sensitive to details m* is sensitive to e-e interactions Can MIRO be used as a precise tool for m* ? What kind of m* is deduced from MIRO ? 6 Rxx=d Vxx/dIdi (arb.un.) Known methods to measure 2DEG m*: FIR cyclotron resonance 1.84 THz m*=0.06857m0 m*=0.06849m0 2.5227THz 3.1059 THz 400 2 200 Rxx () 300 100 =3/2 3 4 5 6 7 8 9 0 Magnetic field (T) Maan et al. APL 40, 609 (1982). S.S. et al. Phys. E 34, 73 (2006). In FIR experiments m* is affected by high B, SdH, plasmons Important comment: CR resonance is not effected by e-e interactions Kohn’s theorem - Phys. Rev. 123, 1242 (1961) 7 Remark: CR cannot be reliably measured in high-mobility 2DEG at MW (1) (2) (3) (1) Calculated reflection/absorbtion by ideal 2DEG (2) A cavity measurements of absorption in a 1mm 2DEG strip (3) CR on photo-excited electrons in bulk GaAs by B.Ashkinadze PRB 52, 17165 (1995) S.S., et al., Phys. Rev. B 76, 165321 (2007) 8 Known methods to measure m*: magneto-plasmon resonance n=2.3x1011 cm-2, m=1.2x106 cm2/Vs m*=0.070 m0 Vasiliadou, Miller, Heitmann, Weiss, von Klitzing, PRB 48, 17145 (1993) 9 Magneto-plasmon resonance experiment on high-mobility samples n=2.7x1011 cm-2 , m=1.3x107 cm2/Vs Hatke, Zudov, Watson, Manfra, Pfeiffer, West, PRB 87, 161307(R) (2013) 𝛼𝑐 =e/2π𝑚∗ 10 Magneto-plasmon resonance in MW absorption on a high-mobility sample m*=0.068 m0 w=0.8 mm n=1.8x1011 cm-2 m=3x106 cm2/Vs m* 0.068 m0 FEDORYCH, STUDENIKIN, MOREAU, POTEMSKI, SAKU, HIRAYAMA, Int. J. Mod. Phys. B 23, 2698 (2009). 11 Effective mass m* from T-dependence of Shubnikov – de Haas oscillations BUT: SdH m* measurements can be affected by side effects… M. Zudov (not published) 12 Effective mass m* from SdH oscillations: side effects Tan, Zhu, Stormer, Pfeiffer, Baldwin, PRL 94, 016405 (2005) : Possible technical issues: o o o o SdH sensitive to n-gradients and fluctuations Possible extra heating Reliable Te- control in B-field SdH amplitude may be affected e.g. by spin splitting o SdH may be non-sinusoidal: higher harmonics 13 Effective mass m* from SdH oscillations: side effects Tan, Zhu, Stormer, Pfeiffer, Baldwin, PRL 94, 016405 (2005) Physical reasons for m* variations: o o o o Assumes Lifshitz-Kosevich formula is correct for 2DEG Depends on LL index i Non-parabolicity Different models o SdH m* depends on e-e interaction 14 MIRO is a beautiful phenomenon: access to new physics? Dmitriev, Mirlin, Polyakov, Zudov, Rev. Mod. Phys. 84, 1709 (2012): 𝛿𝜌 = −𝐴 sin 2𝜋𝜖 ϵ= 𝜔 , 𝜔𝑐 𝜔𝑐 = 𝑒𝐵 is the cyclotron frequency 𝑚∗ 𝜆 = exp(− 𝜋 ) 𝜔𝑐 𝜏𝑞 𝒜(𝑇) = 2𝜋𝜌0 (𝜏/(2𝜏∗ ) + 2𝜏𝑖𝑛 /𝜏) Amplitude vs. B tq quantum scattering time, e.g. Amplitude vs. B vs. B|| - tq in B|| Amplitude vs. T scattering mechanism Amplitude vs. T scattering mechanisms Waveform access to LL shape Shi, Zudov, Studenikin, Baldwin, Pfeiffer, West (2015) Precise MIRO positions m* (B 10mT, precise B - calibration needed) 15 Example of MIRO T-dependence at 1K<T<4K, m=1.3107 cm2/Vs Hatke, Zudov, Pfeiffer, West, PRL 102, 066804 (2009) No signature of the inelastic contribution 16 Example of MIRO T-dependence at 0.35K<T<1.7K, m>3107 cm2/Vs Shi, Zudov, Studenikin, Baldwin, Pfeiffer, West (2015) 𝒜(𝑇) = 2𝜋𝜌0 (𝜏/(2𝜏∗ ) + 2𝜏𝑖𝑛 /𝜏) 17 Can MIRO be used for precise measurements of m* at large LL? What kind of m* : Hatke, MZ, Watson, Manfra, Pfeiffer, West, PRB 87, 161307(R) (2013) Band parameter (CR) Modified by e-e exchange interaction Else? m*MPR = 0.066 m*MIRO= 0.059 18 Example of MIROs on m~3x107 sample Rxx () 0.30 0.25 0.20 0.15 4 8 12 16 20 Magnetic field (mT) Many MIRO harmonics observed, but very small field => limited by magnet precision… 19 Sample: n=3.2 x 1011 cm2, m3107 cm2/Vs, tq=46 ps, mq=1.2106 cm2/Vs AlxGa1-xAs/GaAs/AlGaAs QW Width 30 nm, x=0.24 Symmetrically doped on both sides Spacers - 80 nm, Distance to the surface - 195 nm Cooling process (~2h) under illumination by a red LED (i=50 mA), illumination stopped at 25K n=3.2x1011 (EF=11.4meV) m*(E1+Ef)=0.06793 20 Self-consistent calculations of m* Following: Vurgaftman et al., JAP 89, 5815 (2001) Quantum Codes: GaAs/AlxGa1-xAs QW, EF=11.3 meV, x=0.24 0.074 calculated m*(E1+Ef) m* 0.072 0.070 m*=0.06793 0.068 QW band edge m*= 0.067016 0.066 0 100 200 300 400 QW Width (Å) 21 Self-consistent calculations of m* vs. E GaAs/AlxGa1-xAs QW, w=30 nm, EF=11.3 meV, x=0.24 0.074 Emax-en/e0e calculated m*(E1+Ef) m* 0.072 0.070 0.068 QW band edge m*= 0.06702 0.066 0 20 40 Electric Field (kV/cm) 22 Chip holder for DPPH+MIRO experiment DPPH C18H12N5O6 (1,1-Diphenyl-2-picrylhydrazyl, Free Radical) g*=2.0036 J. Krzystek, A. Sienkiewicz, L. Pardi, and L. C. Brunel, "DPPH as a Standard for High-Field EPR," Journal of Magnetic Resonance, vol. 125, pp. 207211, 1997. RuO2 Thermo-resistor: LakeShore RX-102A-BR 23 Chip and MW antenna arrangement for MIRO experiment 24 MIRO Frequency dependence excited by an antenna 49.62GHz, +5dBm Nov02050_colflip_s_x10, +3 dBm 0.04 0.10 0.08-5dBm Nov02200serMIRO_s_colFlip, 0.02 70 0.05 0.10 0.20 50 0.15 Magnetic field (T) B (mT) 0.00 0.00 B (T) 60 0.06 0.04 40 Nov03200_colflip_s, P=-10 dBm 35 30 25 0.02 20 B (mT) Rxx () 0.06 15 10 10 -5 2 4 6 8 10 15 20 25 40 35 30 5 30 45 50 f (GHz) f (GHz) 12 f (GHz) 0.0 0.0 0.2 0.4 0.6 0.8 Nov03200_colflip_s 0.2 0.4 0.6 0.8 1.0 Nov02050_colflip_s_x10 1.0 25 DPPH resonance from 5 to 70 mT, T=300mK ddyNov03050DPPH_s g*=2.0036 d2dyNov050DPPH_s d2R/dB2 dR/dB 70 70 60 60 50 50 DPPH resonance B (mT) RRuO2 (k) 3.40 3.36 3.32 0.15 0.20 0.25 0.30 Magnetic field (T) B (mT) f=6.0 GHz 40 40 30 30 20 20 10 10 1.5 1.0 0.5 1.6 gmBB=1.16 meV=13 mK 0.8 0.4 f (GHz) f (GHz) At B=10 mT 1.2 -0.0015 -0.0010 -0.0005 0.0000 0.0005 0.0010 0.0015 d2dyNov03050DPPH_s T=300mK => ( n↑ −𝑛 ↓)/n=1-exp(-g*mBB/kBT) 4% 26 B-field calibration using DPPH resonance from 5 to 70 mT Sweep down rate 0.01T/min 70 Sweep down callibration: BDPPH=(0.9804+/-0.0009)Bset+(1.15+/-0.04) mT BDPPH (mT) 60 BDPPH (mT) 50 40 30 20 10 0 0 10 20 30 40 50 60 70 BIPS120(mT) 90° Angle was optimized by maximizing VHall to the fifth digit. 27 MIRO vs 1/BIPS and 1/BDPPH B corrected using DPPH BIPS Rxx () 0.4 0.2 0.0 40 80 120 160 -1 1/BIPS, 1/Bcorrected (T ) 28 m* from MIRO and DPPH 140 0.6 (Xmin+Xmax)/2 120 47.8GHz, -5 dBm Peak Centers of C f=47.800GHz m*/m0=0.0649 +/- 0.0002 0.4 80 Rxx () -1 1/BN (T ) 100 Band theory: m*=0.0679 60 40 Equation y = a + b*x Weight No Weighting Adj. R-Square 0.99995 Value (Xmin+Xmax)/2 Intercept (Xmin+Xmax)/2 Slope 20 0.2 Standard Error 1.16167 0.12699 9.01734 0.01437 0.0 0 0 5 10 15 N Measured m*=0.0649, 40 80 120 BIPS, Bcorrected (mT) Theory: m*(E1+Ef)=0.06793 29 Measured m*=0.0649, band theory m*=0.06793 Quantum Codes: GaAs/AlxGa1-xAs QW, EF=11.3 meV, x=0.24 0.074 m*(E1+Ef) band theory measured m* m* 0.072 0.070 m*=0.06793 0.068 QW band edge m*= 0.06702 0.066 m*MIRO=0.0649 0.064 0 100 200 300 400 QW Width (Å) cos−1 (0.0649/0.0679)=17° 30 Electron effective mass in an ultra-high mobility GaAs/AlGaAs quantum well from MIROs and EPR experiment on DPPH Conclusion 1) Measured m*MIRO= 0.0649 is smaller than theoretically calculated m*theory=0.0679 Question 1) is m*MIRO sensitive to e-e interactions? Or else? 31