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Periodic table

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Periodic table Transition-metal elements Why manganites? : Colossal Magnetoresistance (CMR) Drastic reduction of resistivity with small magnetic fields. – PowerPoint PPT presentation

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Title: Periodic table


1
Periodic table
Transition-metal elements
2
Why manganites? Colossal Magnetoresistance (CMR)
  • Drastic reduction of resistivity with small
    magnetic fields.

FM metal
3
Why materials with large MR are important?
  • Using magnetic technology, the most significant
    market is recording.
  • Projected aerial density for 2005 is 10Gbits/in2
    (rapidly growing). 1 bit size 1000 Angstroms.

4
Basic-science motivation
  • Understand the complex phase diagram that
    experiments are unveiling.

T
Fraction of holes
5
Structure of the Manganites
6
Models for Manganites
7
Main couplings in models for manganites and
Double-Exchange mechanism for ferromagnetism
Mn 3
Mn 4

WARNING SOME COUPLINGS ARE LARGE!
8
Computational Techniques
  • Partition Function
  • Monte Carlo simulation over classical spins.
    Quantum itinerant electrons treated exactly.
  • All temperatures and densities are accessible.
  • Dynamical properties can be calculated
    straightforwardly.

9
Typical results
As observed experimentally (see later)
  • FM, AF , Phase Separation and Spin
    Incommensuration observed.

T0
10
Monte Carlo and DMFT evidence of phase separation
in 1-orbital model
Phase separation manifests as a discontinuity in
density vs. chemical potential. It appears in all
dimensions investigated .
11
Influence of 1/r Coulomb interaction
  • Droplets, stripes or other nanometer size
    patterns may form.

12
Pseudogap in simulations
At intermediate temperatures dynamical clusters
are found near the phase-separation critical
temperature. The clusters are metallic
or insulating, inducing a Pseudogap. ?
similarities with cuprates!
No disorder
With disorder
A.Moreo et al., PRL 83, 2773 (1999)
First reported by Dessau et al. ARPES,
bilayers PG observed..
13
Two Orbitals plus Jahn-Teller phonons
g electron-phonon coupling
k phonon stiffness
14
Orbital and Spin order at x0
Hotta et al. PRB 60, R15009 (1999)
Spin and orbital order at x0
Many states close in energy gt JAF is much
relevant.
15
2 Orbitals and J-T Phonons
  • All the stable phases observed experimentally are
    obtained.
  • PS very prominent as in 1 orbital model.

T 0
Yunoki et al., PRL 81, 5612 (1998)
16
Stripes exist as the ground state at large e-JT
coupling
Hotta et al. PRL86, 4922 (2001)
Pi-shift in orbital order. 1/r not needed.
Ferromagnetic phase.
17
Nanoscale phase coexistence in manganites
Renner et al., Nature 02 BiCaMnO STM
18
Polarons or Larger Clusters?
FM Polaron
Lattice polaron
One carrier surrounded by a distortion.
Mn oxide experiments reveal far larger
clusters, with many carriers inside. Polaron
picture not suitable.
19

Quenched disorder plays an important role
20
Phase Competition in the Presence of Quenched
Disorder
Double Exchange
n1
nlt1
(phase separation)
21
Global Phase Diagram
T
FM
W
SG
T
quenched disorder
quenched disorder
FM
CO
W
SG
T
FM
CO
bandwidth W
W
Courtesy Prof. Yoshi Tokura, Tokyo.
22
Disorder effects are very important near a
first-order transition
Disorder due to chemical doping gt random hopping
and Coulomb centers.
large clusters equal density disorder-induced phas
e separation
Imry-Ma Wortis
Warning Cluster size is disorder strength
dependent!
23
Random Resistor Network
24
CMR effect in inhomogeneous states
Field is small, but effective spin is large!
T
Tc
25
Evidence of T
Thermal expansion
LCMO
From De Teresa, Ibarra et al.
26
State of the art simulations Sen et al., PRL
2007
Resistance vs. temperature via transmission
(Landauer).
Large magneto-resistance observed.
Summary CMR appears in a tiny cluster! Now we
can ask questions to the computer, as in an
experiment.
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