Transcript Document

New roads opening in the field of
Superconducting Materials after the
discovery of MgB2
Sandro Massidda
Physics Department
University of Cagliari
[email protected]
http://www.dsf.unica.it/~sandro/
Outline
•Most superconductors have been discovered by chance!
•Can we do better?
•Basic elements can be found in many SC and can serve
as a guide in the search
•Ingredients of conventional superconductivity: electrons and
phonons.
•The electron-phonon interaction in real materials.
•Key concepts: Kohn anomaly, two-gap superconductivity, Fermi
surface nesting, covalently bonded metals.
•Applications to real materials: MgB2, CaSi2, intercalate graphite
CaC6 , alkali under pressure
Origin of “conventional” superconductivity: phonons
produce an attraction among electrons (Cooper pairs)
Lattice deformation
Overscreening of e-e
repulsion by the lattice
Classical view of how a lattice
deformation by a first electron
attracts the second one
First ingredient: Energy bands. Example of Cu
Symbols are from
experiments
s bands
nearly
parabolic:
free-electron
d bands
Narrow, filled
k
 k (r  l)   k (r)ei kl
Band dispersion from
Bloch theorem carries the
information on chemical
bonding
Similarity: bonding &
anti-bonding molecular
orbitals
An interesting material: MgB2
Tc=39.5 K
B planes
Mg planes
Isoelectronic to graphite, why so different?
Energy bands of MgB2
3D p bands (strongly dispersed along G-A (kz))
2D s bands (weakly dispersed along G-A)
s bonding
(px,py)
p bonding &
antibonding
(pz orbitals)
s
k=(kx;ky;)
(0,0,kz )
(kx;ky;p/c)
sp2
E l e c t r o n i c p r o p e r t i e s o f MgB2
s
Strong covalent
s bonds
p
B
B
B
2-D s-bonding bands
3-D p bands
Dispersion and bonding: p bands
Mg
-
Mg
+
+
+
B
B
G k 0
A
k   0,0,p / c 
s
Graphite
p
MgB2
•Different dispersion
along kz: 2D vs 3D
s
The presence of cations
is crucial to get s holes.
s holes are the origin
of superconductivity
Fermi surface of MgB2
B px and py ( s)
B pz ( p)
The FS is the iso-energy surface in k-space separating
filled and empty states
Second ingredient: Phonons
Lattice deformation:
Rls  R0ls  us (q)e
iqRl
3Nat phonon branches at each wave vector q
 '
ss '
C (q)
2
det
  (q)  0
M s M s'
Analogy with elementary
mechanics:
s atom
  cartesian
component
l  lattice point
k
2

M
Force constants contain the response of the electrons to
ionic displacement: fundamental ingredient
First-principles calculations vs experiments
Source of electron-electron attraction
k+q
k
Virtual phonon
 q
k’-q
k’
BCS theory: superconducting gap
 k  Vkk '
k'
k '
2 k '   k '
2
Ek  k 2   k 2
2
tanh
k ' 2   k ' 2
2kBT
excitation energies
  2h D e
 1
Exponential
dependence on
the coupling 
Tc  1.14  e
2
 3.52
kBTc
k ≈ 2p
Coherence
length
 1
ELIASHBERG theory (1960):
• attractive electron-phonon interaction:
Eliashberg Spectral Function 2F()
describes the coupling of phonons to
electrons on the Fermi Surface
  2  F ( )
2
d

Connection to normal state
electrical resistivity :
  trT
Pb and MgB2 Eliashberg functions
Pb
=1.62 Tc=7.2 K
Low phonon frequencies
MgB2
=0.87 Tc=39.5 K
Large phonon frequencies
Still, CaC6 has larger  and
similar  but Tc=11.5 K !!!
McMillan Equation
Tc 

1.2
1.04
e
1 
  * (10.62  )
 represents the Coulomb repulsion and
is normally fitted to experimental Tc
N(EF ) I

2
M  ph
2
N(EF) electronic density of states
I
e-ph interaction
M
nuclear mass
ph average ph. frequency
Exponential dependence
Results of theoretical calculations for elemental
superconductors: comparison with experiment
Tc
T=0 gap at EF 
M. Lüders et al. Phys. Rev. B 72, 24545 (2005)
M. Marques et al. Phys. Rev. B 72, 24546 (2005)
A. Floris et al, Phys. Rev. Lett. 94, 37004 (2005)
G. Profeta et al, Phys. Rev. Lett. 96, 46003 (2006)
Cagliari Berlin L’Aquila
collaboration
MgB2 superconductor, AlB2 no
Phonon density of states
Spectral function 2F()
Comparable phonon DOS, very different 2F()
 2 F( )
 2
d

B1g
Phonons in MgB2
E2g
Anomalously low frequency E2g branch
(B-B bond stretching)
Large coupling of the E2g phonon mode
with s hole pockets (band splitting)
E2g=0.075 eV
 ≈ 1-2 eV !!!
Electron doping destroys SC
Phonon life-time
MgB2 SC
AlB2 not SC
As soon as s holes disappear with e-doping, superconductivity disappears
The width of Raman lines are proportional to the phonon inverse life-time. The
difference between MgB2 and AlB2 indicates the different electron-phonon
coupling in these two materials
Kohn anomaly: LiBC, isoelettronic to MgB2 (Pickett)
phonon frequency
Stoichiometric compound
is a semiconductor
Strong renormalization
of phonon frequencies
Metallic upon doping
Kohn anomaly
High Tc predicted
Unfortunately not found
experimentally
Kohn anomaly
The electronic screening is discontinuous at 2kF
(log singularity in the derivative of the response )
d  q
dq q2 k
 
q > 2kF
F
For q>2kF it is not possible to create
excitations at the small phonon energy
q < 2kF
FS
For q<2kF the electronic screening
renormalizes the phonon frequency
A Kohn anomaly lowers the energy of E2g phonons in MgB2
2-dimensionality increases the effect
Two band model for the electron phonon coupling (EPC)
•  stronger in s bands due to the
coupling with E2g phonon mode
• Experiments show the existence
of two gaps: s and p.
s
p
Fermi surface
Two band model:
experimental
evidence
R. S. Gonnelli, PRL
89, 247004 (2002)
Specific heat: evidence of 2 gaps
Two-gap structure associated with s and p bands
Tunnelling
experiments
Two band superconductivity
Tc
depends on the largest
eigenvalue of the inter- and
intra- band coupling constants,
nm and not on the average 
Impurities in two-gap superconductors
have a pair-breaking effect as magnetic impurities in single-gap SC
Unfortunately, the experimental situation is not so clear
Parent structures to MgB2
CaGa2-xSix
CaGa2  CaSi2
CaSi2 becomes Superconductor
under pressure, Tc around 14 K
Tc
CaSi2: phase transitions and superconductivity
Frozen-in B1g phonon:
trigonal structure due to
instability of p bands
Trigonal
MgB2
  trT at high T
CaSi2: instability of p bands; sp2  sp3
Large splitting at EF upon distortion
DOS
KSi2
CaSi2
Amplitude of trigonal distortion
vs pressure and band filling
Lowered frequencies in
SC MgB2. CaBeSi?
CaBeSi
s bands
at EF
Intercalate graphite: CaC6 Tc=11.5 K
The highest Tc among
intercalated graphite
compounds
(normally Tc < 1 K)
N. Emery et al.
Phys. Rev Lett. 95, 087003 (2005)
CaC6
 Amount of Ca
contribution
Ca FS
FS
C p FS
Phonons in CaC6: 21 modes
Very high frequencies but also
low frequency branches
Orbital character
CaC6: gap and orbital character
k
Gap k over the Fermi surface
Superconductivity under pressure
29 elements superconducts under normal conditions
23 only under pressure: Lithium is the last discovered
Tc(P) is a strongly material-dependent function*
* C. Buzea and K. Robbie
Supercond. Sci. Technol. 18 (2005) R1–R8
Aluminium under pressure……
270 GPa
Bonds get stiffer, frequencies higer
…Al becomes a normal metal
N(EF ) I 2

M  2ph
Alkali metal under high pressure: many phase transitions
Lithium is a superconductor under pressure
CI16
42
hR1
…
…
39
…
fcc
7
0
9R
Electron states of Li and K under pressure
Charge on
d states
K
27 GPa
Li
30 GPa
Charge on
p states
Phonon dispersion in Li: softening and stiffening
26 GPa
26 GPa
0 GPa
0 GPa
Why?
Increasing the pressure a lattice instability driven by the
Fermi surface nesting increases the electron-phonon coupling
Pieces of Fermi surface connected
by the same wave-vector q
Phonon softening and
lattice instability
q
q
Imaginary frequency: instablility
Orbital character at EF and superconductivity
d character

K
Li
p character

Electron-Phonon Coupling
Pressure 

Stiffer bonds (higher ’s) but higher coupling at low 
Theoretical predictions
Summary
• I presented an essential description of the properties
and SC mechanisms in a few important materials
• Each real material has plenty of interesting physics
•SC needs material-adapted understanding where
similar mechanisms can act in very different ways
A15 Compounds
Nb3Sn Tc=18 K
it could be a Multigap SC
Guritanu et.al. PRB 70
184526 (2004)
Lattice distortions in Nb3Sn
Free-energy of cubic
and tetragonal
V3Si
c
  1
a
Nb3Sn
Softening of elastic
constant
Softening of optical
phonon mode
Lattice distortions in A15
Band structure of Nb3Sn
Large peak
at EF
Concepts in ELIASHBERG theory:
• repulsive Coulomb interaction (Morel Anderson):
  Vel el
 

FS

1   ln
EF
D
The difference between electron (h/EF) and nuclear (1/D) time
scales reduces the coulomb repulsion (retardation)
Superconductivity results from the competition
of opposite effects: 
Impurities in two-gap superconductors
Irradiation by neutrons (Putti et al)
Only in a C-doped sample the
merging has been observed at
20 K (Gonnelli et coworkers)
Electronic properties of Al-doped MgB2
Mg1-xAlxB2
x=0
x = 0.25
x = 0.33
x = 0.5
Electron-phonon
spectral function
2F()
Bands of CaSi2 in the ideal and distorted (full lines) structures
Spectral function of Nb3Sn from tunnelling
Many different results
with many different 
values, ranging from
 =1.08 to 2.74!
Non-magnetic impurities: Anderson theorem
In the presence of disordered impurities the wave-vector k is not
a conserved quantity: electrons cannot sneak anymore as
Bloch suggested, if the potential is not periodic
However, the impurity potential being static, V(r, t ), we
still have stationary states:
k  n
We can form Cooper pairs by
time-reversal degenerate states
k ,k  n ,
*
n
Important physical conclusion: Tc does not change in a
significant way due to the presence of impurities!
Impurities: experiments
Tc proportional to the low temperature
resistivity, related to impurities induced
by irradiation.
Magnetic impurities: Gorkov-Abrikosov theory
Magnetic impurities split the energy of states with spin  and 
pair breaking effect
Important physical conclusion: Tc is strongly
depressed by the presence of magnetic impurities!
d
d
Ni
The presence of a static
magnetic moment is
incompatible with conventional
superconductivity