Incommensurate correlations & mesoscopic spin resonance in YbRh 2 Si 2 * *Supported by U.S. DoE Basic Energy Sciences, Materials Sciences & Engineering.

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Presentation transcript:

Incommensurate correlations & mesoscopic spin resonance in YbRh 2 Si 2 * *Supported by U.S. DoE Basic Energy Sciences, Materials Sciences & Engineering DE-FG02-08ER46544 C. Broholm Johns Hopkins University

Overview  Introduction  SDW Quantum Criticality in metals  The case of YbRh 2 Si 2  Results & Discussion  Incommensurate spin correlations  Quasi-FM Quantum Critical Scaling  Unconventional spin resonance  Conclusions

Field Driven QCP in YbRh 2 Si 2 Yb Rh Si 11 × Gegenwart et al PRL (2002)

Kondo Lattice quantum criticality Schroeder et al Nature (2003) Steglich et al J. Phys. Cond. Matter (2012)

Fermi-surface reconstruction at T N ? Friedemann et al PNAS (2010)

YbRh 2 Si 2 : neutrons come lately  200 x 5×5 mm 2 crystals  Mounted with H-free oil  Total mass 3 g  Mosaic FWHM 2 o  Penetration depth ≈2 mm

Field Driven QCP in YbRh 2 Si 2 Yb Rh Si 11 × Gegenwart et al PRL (2002) No neutron yet

Collaborators Chris Stock & F. Demmel ISIS Facility, Rutherford Appleton Lab C. Petrovic & R. Hu Brookhaven National Laboratory H. J. Kang & Y. Qiu NIST Center for Neutron Research SPINSDCSOSIRIS

Four CF Kramer’s Doublets in YbRh 2 Si 2 Kutuzov et al (2008)

Incommensurate critical fluctuations

Incommensurate correlations

Spin Fluctuations & Neutrons Scattering V 2-y O 3 Bao et al. PRL (1993)

Spin fluctuations near MIT in V 2 O 3 P I

Spin Density Wave Order Bao et al. PRL (1993) Wolenski et al., PRB (1998) Experimental Q c

Incommensurate correlations

SDW from nesting instability? (002) (111) (110) (1-(a/c) 2, 0,2) Norman PRB (2005) (1-(a/c) 2, 1-(a/c) 2,2) Friedemann et al (2010)

Apparent FM correlations upon heating 0.3 K

Quantum critical scaling for Q≈0

Critical Exponent Trovarelli et al PRL (2010)

Magnetization SQUID & neutrons C. Stock et. al., (2009)Gegenwart et al., NJP (2006)

From SDW to FM correlations with field (hh2) [r.l.u.] Effects of field:  Upward shift of spectral weight  Sharp peak at FM position  Field induced resonance Effects of field:  Upward shift of spectral weight  Sharp peak at FM position  Field induced resonance

Field Induced Resonance C. Stock et. al., PRL (2012)

MnSi: Field induced “ferromagnons” Tarvin et al., Phys. Rev. (1978).

YbRh 2 Si 2 : A spot in Q-space C. Stock et. al., PRL (2012) 1.25 Tesla

Form factor for chain-end spin Kenzelmann et al. PRL (2003)

Interpretation of the spin resonance Coincident g-factors indicate this is Electron Spin Resonance Coherent precession of spin density Similar to a Kondo length scale Kondo Screened spins for B>B c

Conclusions Effective FM critical regime for T>1 K Lower T: Incommensurate critical fluctuations SDW instability may arise from nesting of hole fermi- surfaces B suppresses SDW favoring FM polarized metal Meso-scopic spin precession indicates Kondo screened 4f spin degree of freedom SDW correlations persist at lower energies in magnetized kondo lattice state Stock et al PRL (2012)

Outlook SDW phase –Can band-theory account for incommensurate Q c –Q c may help to clarify nature of low field state and field driven transition –Detect SDW Bragg peak and measure critical exponents –Pressure or doping driven changes in Q c QCP –Inelastic scattering at lower T and ħ  –Identify field driven QC metal with higher critical temperatures and/or less neutron absorption