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Temperature dependence of the superconductivity-induced collective mode in the c-axis infrared spectra of bilayer cuprate superconductors

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Temperature dependence of the superconductivity-induced collective mode in the c-axis infrared spectra of bilayer cuprate superconductors

D. Munzar

a,*

, J. Chaloupka

a

, C. Bernhard

b

, A. Dubroka

b

, J. Vašátko

a

aDepartment of Condensed Matter Physics, Faculty of Science, Masaryk University, Kotlárˇská 2, 611 37 Brno, Czech Republic

bDepartment of Physics and Fribourg Center for Nanomaterials, Chemin du Musee 3, CH-1700 Fribourg, Switzerland

The low-temperature spectra of thec-axis infrared conductivity of bilayer high-Tccuprate superconduc- tors (HTCS) exhibit two superconductivity-induced modes [Li Yu et al., Phys. Rev. Lett. 100 (2008) 177004; and references therein]. Both can be understood in terms of a microscopic theory developed recently [J. Chaloupka, C. Bernhard, D. Munzar, Phys. Rev. B 79 (2009) 184513]. Here we summarize the elements of the theory and report on the temperature dependence (TD) of the low-energy mode and of the total optical spectral weight (SW). The calculated TD of the mode is consistent with experiment but the trends of the SW are not.

The important issue of the origin of the superconductivity-in- duced modes in the spectra of thec-axis infrared response of bi- layer HTCS has been recently addressed using a microscopic theory[1]. Its elements are: (a) the local (intra-bilayer – ‘‘bl” and inter-bilayer – ‘‘int”) fields, current densities, conductivities, and an extension of the multilayer formula of Ref.[2]. (b) The conduc- tivities are calculated using a microscopic model and the linear re- sponse theory. This is the main difference with respect to previous phenomenological approaches[2–4]. (c) The microscopic model in- volves the bilayer-split (bonding and antibonding) bands. (d) The quasiparticles of the two bands are coupled to spin fluctuations, as in Ref.[5]. The coupling leads to superconductivity and is de- scribed at the level of generalized Eliashberg theory, as in Ref.

[6]. (e) The gauge invariance of the theory, required for a consis- tent, i.e., charge conserving description of the charging of the cop- per-oxygen planes induced by the applied field, has been achieved by including a class of vertex corrections (VC) ensuring that the renormalized current vertices satisfy the appropriate Ward identi- ties. The VC lead to dramatic and qualitative changes of the calcu- lated response as demonstrated below.Fig. 1shows the real part of the intra-bilayer conductivity calculated assuming insulating spac- ing layers between the bilayer units, considering a BCS-like (sepa- rable, nonretarded) interaction between the quasiparticles, for various values of the intrabilayer hopping amplitudet?(the values of other input parameters are the same as in Section III A of Ref.

[1]), with the VC neglected (a) and included (b). In the former case, the conductivity possesses also the delta function at the origin due to the condensate (not shown). Note the difference in the t?- dependence of the energy of the maximum: in (a), it begins at the superconducting gap 2D, in (b), the energy is proportional to t?. The maxima correspond to a pair-breaking (bonding-antibond- ing) peak and a collective mode (CM), respectively. As discussed in [1], the CM can be viewed as an analogue of the Bogoljubov–Ander- son mode occurring in the longitudinal response of homogeneous superconductors, seeFig. 1c and d. For small values of the bilayer splitting, its nature is similar to that of the transverse plasmon introduced in Ref.[2]. Thet?-dependence of its frequency is anal- ogous to the

v

F (Fermi velocity)-dependence of that of the Bogo- ljubov–Anderson mode,

x v

Fjqj, whereqis the wavevector. In the totalc-axis conductivity,

r

c, the CM is shifted towards higher energies due to the Coulomb interaction of the charged planes, an analogue of the Anderson–Higgs mechanism. The interpretation of the two modes in the data is the following: the well known peak around 400 cm1is attributed to the CM and the maximum around 1000 cm1[7]to a pair-breaking feature resulting from the coupling through the spacing layers. The theory can be further extended[8]

to account for the phonon anomalies discussed in Ref. [3]. The resulting formulas have the same form as those of Refs.[3,9].

Fig. 2shows the TD of the CM in Re

r

ccalculated assuming insu- lating spacing layers, quasiparticles coupled to spin fluctuations, VC included,t?max¼45 meV, the values of other input parameters are the same as in Section III B of Ref.[1]. AboveTc of 89 K, the spectra display a broad maximum centered around 600 cm1due

* Corresponding author. Tel.: +420 549495980; fax: +420 541211214.

E-mail address:[email protected](D. Munzar).

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Published in "Physica C: Superconductivity, 2010 doi: 10.1016/j.physc.2009.10.094"

which should be cited to refer to this work.

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to the interband transitions. Only belowTc, a sharp peak corre- sponding to the CM appears around 480 cm1, collecting SW both from lower and from higher energies. Its frequency is only weakly temperature dependent, in agreement with the experimental data on underdoped YBa2Cu3O7-d[10]. Its SW exhibits an order-param- eter like increase belowTc, in agreement with the data on slightly underdoped samples[10]. The total optical SW exhibits a decrease belowTc. This is consistent with the BCS theory and in contrast with the observed increase of the SW in the infrared[11,12,7]. A slightly different temperature dependence of the total SW would be obtained in case of a temperature dependent spin susceptibility

v

SF. The total SW decreases considerably with decreasing fre- quency of the low-energy component of

v

SF. The shift from

40 meV to 30 meV, e.g., leads to a decrease of the normal-state SW by about 5%.

In conclusion, the calculated frequency of the collective mode is only weakly temperature dependent and its SW exhibits an order-parameter like behaviour, consistent with experiment. The TD of the total optical SW, however, displays a decrease below Tc, in contrast with experiment. The discrepancy is probably re- lated to the inadequacy of the present approach to describe the c-axis electrodynamics in the normal state. Alternatively, it may be due to a strong TD of the pairing ‘‘glue”. This work was sup- ported by the Ministry of Education of Czech Republic (Grant No.

MSM0021622410) and the Schweizerische Nationalfonds (SNF) (Grant No. 200020-119784).

0 10 20 30 40 50 60 70 80

0 200 400 600 800 1000 1200 1400 1600

Reσc-1cm-1]

ν [cm-1] T=20K

T=60K T=80K T=100K T=120K

1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5

0 20 40 60 80 100 120 140 160 spectral weight [103Ω cm-2]

T [K]

SW in 400-550cm-1 total× 1/4 total× 1/4 (NS)

Fig. 2.Temperature dependence of the real part of the totalc-axis conductivity. Inset: that of the spectral weight in the frequency interval marked by the arrow and of the total optical spectral weight. The dashed line represents a straightforward extrapolation of the normal state dependence.

j

j

j

Δθ

− +

+ +Δθ

−Δθ

−Δθ +Δθ

j

int

bl

int 0 5 10 15 20 25

0 50 100 150 200

t1 maxReσbl/bl [meV-1Ω-1cm-1]

photon energy [meV]

(b)

VC

0 1 2 3 4 5 6 7 8 9

t3 maxReσbl/bl [10-3 meV-3 Ω-1 cm-1 ]

(a)

NV t⊥ max=10meV

15meV 30meV 45meV 60meV 90meV

(c) (d)

Fig. 1.Real part of the intra-bilayer conductivityrbl=blcalculated with the VC neglected (a) and included (b). Schematic representation of the density-, current density-, and phase-pattern associated with the Bogoljubov–Anderson mode of a single layer superconductor (c) and the same for the collective mode of the bilayer system (d).

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References

[1] J. Chaloupka, C. Bernhard, D. Munzar, Phys. Rev. B 79 (2009) 184513.

[2] D. van der Marel, A. Tsvetkov, Czech J. Phys. 46 (1996) 3165.

[3] D. Munzar et al., Solid State Commun. 112 (1999) 365.

[4] M. Grüninger et al., Phys. Rev. Lett. 84 (2000) 1575.

[5] M. Eschrig, M.R. Norman, Phys. Rev. Lett. 89 (2002) 277005.

[6] J. Chaloupka, D. Munzar, Phys. Rev. B 76 (2007) 214502.

[7] Li Yu et al., Phys. Rev. Lett. 100 (2008) 177004.

[8] J. Vašatko et al., unpublished data.

[9] A. Dubroka, D. Munzar, Physica C 405 (2004) 133.

[10] C. Bernhard et al., Phys. Rev. B 61 (2000) 618.

[11] D.N. Basov et al., Science 283 (1999) 49.

[12] A.V. Boris et al., Phys. Rev. Lett. 89 (2002) 277001.

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