+ All Categories
Home > Documents > Coupling of the A1g As-phonon to magnetism in iron … of the A1g arsenide phonon to magnetism in...

Coupling of the A1g As-phonon to magnetism in iron … of the A1g arsenide phonon to magnetism in...

Date post: 18-May-2018
Category:
Upload: lamhuong
View: 217 times
Download: 3 times
Share this document with a friend
44
Coupling of the A1g As-phonon to magnetism in iron pnictides Belén Valenzuela Instituto de Ciencias Materiales de Madrid (ICMM-CSIC) BNL, New York 2013
Transcript

Coupling of the A1g As-phonon to magnetism in iron pnictides

Belén Valenzuela

Instituto de Ciencias Materiales de Madrid

(ICMM-CSIC)

BNL, New York 2013

In collaboration with:

BNL, New York 2013

Noel A. García-Martinez (ICMM-CSIC)

Sergio Ciuchi (Universitá dell’Aquila)

Emmanuele Cappelluti (CNR Roma)

Maria J. Calderón (ICMM-CSIC)

Elena Bascones (ICMM-CSIC)

Index

•  Introduction: Interplay of charge, spin and lattice dynamics in iron superconductors –  A1g As-phonon Raman response

•  Our work: – Electron-phonon Hamiltonian plus interactions. – Phonon Raman response using charge-phonon

theory. – Results: Raman intensities of the A1g As-phonon

in the A1g, B1g and B2g symmetries.Hardening/softening.

BNL, New York 2013

K0.8Fe2Se2

11

111

122 1111

BNL, New York 2013

Davis, et al. Science’10

The orthorhombic transition follows the magnetic transition with (π,0) ordering

Green&Paglione, Nat.Phys.’10

Both, chemical doping and pressure suppress the SDW and induce SC.

BNL, New York 2013

•  Experimentally several phononic signatures show unconventional behavior in the magnetic state: Choi et al. PRB’08, Le Tacon et al. PRB’08, PRB’09, Chauviere et al. PRB’09, PRB’11, Akrap et al. PRB’09, Zhang et al. JACS’10, Schafgans et al. PRB’11, Nakajima et al. PNAS’11, Kim et al Nat. Mat.’12, Liu et al. PRL’13…

Zbiri et al., Phys. Cond. Matt’10

•  Theoretically (Ab-initio calculations): •  iron-magnetism is present also above

TN? what about the estimations of the electron-phonon coupling?

•  The electron-phonon coupling has been shown to be enhanced by magnetism. (Yndurain et al PRB’09, Boeri et al. PRB’10)

•  Role for the mechanism of superconductivity?

A1g As-phonon

BNL, New York 2013

It has been claimed that the height of the As atom affects: •  the band structure at the Fermi level •  the magnetic moment, magnetic ordering •  the superconducting critical temperature, sc gap

Raman A1g As-phonon

BNL, New York 2013

A1g=LL B1g=x’y’ B2g=xy

Raman A1g As-phonon

BNL, New York 2013

Chauviere et al PRB’11 (BaFe2As2)

Below the Magneto-structural transition the A1g As-phonon Intensity increases a lot for B1g (x’y’)

A1g=LL B1g=x’y’ B2g=xy

Raman A1g As-phonon

BNL, New York 2013

Chauviere et al PRB’11 (BaFe2As2)

Below the Magneto-structural transition the A1g As-phonon Intensity increases a lot for B1g (x’y’)

A1g=LL B1g=x’y’ B2g=xy

A1g As-phonon intensity in B1g is 1.5 bigger than in A1g in the magnetic state of BaFe2As2

The structural transition cannot explain these features, Why then?

Raman A1g As-phonon

BNL, New York 2013

Rahlenbeck et al PRB’09 (BaFe2As2): Below the Magneto-structural transition softening and narrower scattering rate

Choi et al PRB’08 (CaFe2As2): Below the Magneto-structural transition hardening and narrower scattering rate

Our work: Coupling of the A1g arsenide phonon

to magnetism in iron pnictides

N. García-Martinez, B.V, M.J. Calderón, S. Chiuci, E. Cappelluti, E. Bascones, arXiv:1307.7065

BNL, New York 2013

Our model: Microscopic Hamiltonian

dxy dxz, dyz d3z2-r2

dx2-y2

Spin 2

Introducing on-site interactions: U -> intraorbital repulsion U’ -> interorbital repulsion J -> Hund’s coupling U’=U-2J

6 electrons in 5 d orbitals in a tetrahedral environment with crystal field 100-200meV:

!

H = HTB +Hph +H int

BNL, New York 2013

Tight-binding

ü  Focus on Fe-pnictogen planes, square lattice, Fe unit cell

ü  Five Fe d-orbitals; pnictogen included through hoppings;

direct (Fe-Fe) + indirect (Fe-pnictogen-Fe) hoppings

ü  Symmetry of the orbitals considered through Slater-Koster

parameters to describe the hoppings (pdσ, pdπ, ddσ1, ddπ1,ddδ1)

ü  Straightforward change of pnictogen position (angle α)

MJ Calderon, B.V, E Bascones PRB’09

BNL, New York 2013

Phonon Hamiltonian

BNL, New York 2013

We are just interested in Raman processes i.e q=0

The electron-phonon coupling is split in two contributions gα (geometrical) y gpd (through energy integrals pdσ and pdπ). Both have local and non-local contributions:

Geometrical phonon coupling:

Energy integral phonon coupling:

With: We assume: valid for p & d orbitals localized

(π,0) Magnetic phase diagram

We calculate the magnetic U-JH/U phase diagram applying mean field theory to the electronic Hamiltonian.

!

H = HTB +H int (U,J)

BNL, New York 2013

1 1.5 2 2.5 3U (eV)

0

0.1

0.2

J H/U

ITINERANT

STRONG ORBITALDIFFERENTIATION

E. Bascones, M.J. Calderón, B. V., PRL’10; PRB’12

xy and yz become half-filled gap states

We study this line J=0.25U

NM

LM

HM

Band structure for the non-magnetic and magnetic regime in the itinerant

region

BNL, New York 2013

Spectral weight reorganization at low energies due to magnetism in a multiorbital system

We have add a renormalization factor of 3 (in accordance with ARPES)

Raman response for the A1g As-phonon

BNL, New York 2013

Raman vertices:

BNL, New York 2013

In the PM state B1g and B2g Raman response are zero because they are orthogonal to the symmetry of the A1g As-phonon. Our proposal: Due to the electron-phonon coupling the B1g Raman response of the A1g As-phonon is large in the magnetic state since the tetragonal symmetry is broken by the (π,0) magnetic ordering: Anomalies in phonons driven by magnetism

(antisymmetric kx ky)

(antisymmetric kx -kx or ky -ky )

Charge-phonon theory I:

BNL, New York 2013

Raman vertex Electron phonon

Interaction

Ω0 and Γ0 are the phonon frequency and the phonon scattering rate

The Raman response is calculated using the Charge-phonon theory

This contribution has been calculated in B.V, Calderon, Leon, Bascones PRB’13

Our main calculation Mixed bubble

Phonon propagator

Charge-phonon theory II:

BNL, New York 2013

Charge-phonon theory II:

BNL, New York 2013

Charge phonon theory related to Fano theory. All the physics is encoded in the mixed bubble:

E. Cappelluti, et al, PRB’12

Results: A1g As-phonon Raman intensity

BNL, New York 2013

1 1.25 1.5 1.75 2U (eV)

0

0.003

0.006

0.009

0.012

I!

" (a

rbitr

ary

units

)

!=A1g!=B1g

(a)

1 1.25 1.5 1.75 2U (eV)

0

0.2

0.4

0.6

0.8

I!

pd (a

rbitr

ary

units

)

1 1.25 1.5 1.75 2U (eV)

0

1

2

3

M (

µ B) (b)

There is a critical value of U where IB1g > IA1g as in BaFe2As2

IA1g increases a lot in the magnetic state as in 122 compounds

But the resulting intensity cannot be calculated due to uncertainties in the values of the phonon couplings gα and gpd

NM NM AFM AFM

Phonon hardening/softening and life-time

BNL, New York 2013

1 1.25 1.5 1.75 2U (eV)

-3

-2

-1

0

1

2

!"

M (c

m-1

)

M=#M=pd

(a)

1 1.25 1.5 1.75 2U (eV)

-0.2

-0.1

0

0.1

0.2

0.3

0.4

0.5

!"

M (c

m-1

)

(b)

Softening of the phonon frequency in the magnetic state.

Narrowing or broadening appear depending on parameters

Hardening just for large values of U when e-ph coupling goes via gpd

Phonon hardening/softening and life-time

BNL, New York 2013

1 1.25 1.5 1.75 2U (eV)

-3

-2

-1

0

1

2

!"

M (c

m-1

)

M=#M=pd

(a)

1 1.25 1.5 1.75 2U (eV)

-0.2

-0.1

0

0.1

0.2

0.3

0.4

0.5

!"

M (c

m-1

)

(b)

Softening of the phonon frequency in the magnetic state.

Narrowing or broadening appear depending on parameters

Hardening just for large values of U when e-ph coupling goes via gpd

The softening is related to the spectral weight redistribution in a multiorbital system from higher energies (Ω > Ω0) to lower energies (Ω < Ω0) when entering into the magnetic state.  

Summary of our work •  The electron-phonon coupling is via the dependence of the Slater-Koster

parameters (α, pdσ, pdπ) on the As position. •  Magnetism is included at the mean-field Hartree-Fock level. •  The Raman response is evaluated in the paramagnetic and in the (π, 0)

magnetic states using the proper generalization of the charge-phonon theory.

•  A finite Raman intensity can be observed in the magnetic state in the B1g but not in the B2g polarization and it is a consequence of the coupling of the phonons to the anisotropic (π,0) magnetic state.

•  Softening and hardening are possible. •  For a quantitative comparison more work is needed. Outlook •  It is possible that in the nematic state there is a signal in B1g. •  In the double stripe magnetic state of FeTe, the out-of-plane Te-phonon will

be different from zero in the B2g polarization geometry, instead B1g symmetry.

It would be interesting to explore these possibilities experimentally.  

Thank you!

Going beyond…. •  The interplay between magnetism and As-heigh should be treated self-consistently •  The electron-phonon coupling could be go through the interactions •  Magnetism beyound mean-field.

1 1.25 1.5 1.75 2U (eV)

-0.004

-0.002

0

0.002

0.004

0.006

0.008

-!'B 1g

pdno

n-lo

c (a

rbitr

ary

units

) (d)

1 1.25 1.5 1.75 2U (eV)

-0.04

-0.03

-0.02

-0.01

0

0.01-!

'A1g

pdno

n-lo

c (ar

bitra

ry u

nits

)(b)

1 1.25 1.5 1.75 2U (eV)

-0.003

-0.002

-0.001

0

-!'B 1g

"no

n-lo

c (a

rbitr

ary

units

)

1st neighbors2nd neighborsTotal

(c)

1 1.25 1.5 1.75 2U (eV)

-0.002

0

0.002

0.004

0.006

0.008

-!'A

1g"

non-

loc (a

rbitr

ary

units

) (a)

Anisotropy in transport:

- Anisotropy in transport (Chu et al. PRB’10; Science’10, Tanatar et al. PRB’11) and in optical conductivity (Dusza et al, EPL’11, Review: I.R. Fisher et al. Rep. Prog. Phys.’11, Nakakima et al. ‘11), etc

Chu et al. Science’10

Fe More metallic

Less

met

allic

BNL, New York 2013

Unexpected because: •  FM bond is shorter than AF one •  AF is naively associated with gaps

and FM with metallicity •  Scattering rate is larger in the AF

direction

Magnetism: (π,0) mean field phase diagram: metallic region

BNL, New York 2013

We also calculate the Drude ratio with the Kubo formula and

get the same result.

We assume the scattering rate is isotropic

Da / Db =va2 (k,n )g (k,n )!("n (k)! EF )

k ,n"

vb2 (k,n )g (k,n )!("n (k)! EF )

k ,n"

Drude weight ratio

BNL, New York 2013

Da/Db>1 consistent with experimental ra/rb<1 Is given in regions with low magnetic moment

Drude weight ratio: Da/Db

Drude weight anisotropy:

BNL, New York 2013

nyz<nzx

Experimental signs of anisotropy and orbital ordering are anticorrelated, B. Valenzuela, E. Bascones, M.J. Calderón, PRL 105, 207202 (2010)

nyz-nzx

Da/Db>1 consistent with experimental ra/rb<1

Drude weight ratio: Da/Db

Is orbital order responsible of resistivity anisotropy?

BNL, New York 2013

Magnetic reconstruction as origin of the conductivity anisotropy

                                       Dx/Dy

J H/U

Anisotropy linked to topology and morphology of the Fermi Surface. Experimental anisotropy in general for low moment.

B. Valenzuela, EB, M.J. Calderón, PRL 105, 207202 (2010)

Dx/Dy=  0.72  Dx/Dy=  1.34  

Dx/Dy=  0.52  Dx/Dy=  1.09  

Sensitivity of the anisotropy to the angle α

BNL, New York 2013

                                       Dx/Dy

Regular  tetrahedron    Squashed  tetrahedron  

 In  the  squashed  tetrahedron  the  region  with  Dx/Dy>1  has  reduced  very  much  and  it  is  increased  for  the  elongated  tetrahedron.  

U(eV)

J/U

1 1.5 2 2.50

0.05

0.1

0.15

0.2

0.25

0.2

0.4

0.6

0.8

1

1.2

1.4

1.6

U(eV)

J/U

1 1.5 2 2.50

0.05

0.1

0.15

0.2

0.25

0.5

1

1.5

2

2.5

3

3.5

4

4.5

5

Elongated  tetrahedron  

The effect of magnetism is not just at the Fermi surface but it is seen at all energies in the band

Bands

U=2.2, J=0.07U

BNL, New York 2013

Orbital reorganization in the Hartree-Fock phase diagram

x2-y2

3z2-r2

(π,0) in x2-y2 configuration (π,π) in 3z2-r2 configuration

Resembles the orbital reorganization found in the strong coupling limit

M.J. Calderón, G. León , B. Valenzuela, EB, arXiv: 1107.2279 (2011)

Tight-binding for five orbitals: angle dependence of the hoppings

BNL, New York 2013 MJ Calderon, B.V, E Bascones PRB’09

Hoppings related by symmetry and calculated with four fitting parameters

Experimental range

Hartree-Fock phase diagram. Sentivity to Crystal field

100 50 mev

Correlated metal

3z2-r2 /x2-y2 CF 100 meV larger

Nesting driven (π,0)

Γ M X Y Γ-4

-3

-2

-1

0

1

2

3

Reasoning from the strong coupling point of view to understand the LM

The low moment phase is stabilized because crossed hoppings are as big as direct hoppings and also very anisotropic: Release frustration

Q=(π,0)

t yyz,x2!y2

= 0

t xxy,yz = 0

Orbital ordering in the band structure for U=2.2 eV and J=0.07U

Phase separation

5 5.5 6 6.52

3

4

5

( , )

PS ( ,0)

PSDS

PS (

JH/U=0.22

U

n

Magnetism: Mean field phase diagram

BNL, New York 2013

In the mean field description there is a DS phase charge modulated instead of FM. But strong coupling analysis also points to DS instability at high JH

7 electrons 5 electrons

M.J. Calderón, G. León , B. V., E. Bascones, arXiv: 1107.2279 (2011)


Recommended