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PHYS07200604007 Manas Kumar Dala - Homi Bhabha National ...

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Electronic Structure of Pr 0.67 Ca 0.33 MnO 3 64<br />

300 K<br />

77 K<br />

5 X Difference<br />

(a)<br />

300 K<br />

110 K<br />

5 X Difference<br />

(b)<br />

Intensity (arb. units)<br />

-1 -0.5 0 0.5 1 1.5<br />

300 K<br />

220 K<br />

5 X Difference<br />

(d)<br />

-1 -0.5 0 0.5 1 1.5<br />

300 K<br />

150 K<br />

5 X Difference<br />

(c)<br />

-1 -0.5 0 0.5 1 1.5<br />

Binding Energy (eV)<br />

-1 -0.5 0 0.5 1 1.5<br />

Figure 3.2: High-resolution photoemission spectra of the near-E F region of the valence<br />

band of Pr 0.67 Ca 0.33 MnO 3 . In (a) the spectrum taken below T c (red) is compared with<br />

the normal state (300 K) spectrum (blue). The difference spectrum (green) obtained<br />

by subtracting the spectra at 300 K from 77 K and multiplied by 5 is also shown in<br />

the panel. Similarly, in (b), (c), and (d) the near-E F spectra taken at 110, 150, and<br />

220 K are compared with that taken at 300 K. The feature in the difference spectra<br />

corresponds to the tail feature A (e g↑ ) in Fig. 3.1.<br />

is quite small compared to B and C and is a signature of the insulating nature<br />

of this material. Earlier photoemission experiments on La 1−x Sr x MnO 3 also have<br />

shown that the intensity of this tail feature A is quite small [8, 20, 21, 22, 23].<br />

The presence of the feature A is clear from Fig. 3.2, where we have shown the<br />

near-E F region of the valence band spectra taken with a higher resolution. Here,<br />

the spectra taken at different temperatures have been compared with those at room<br />

temperature. The figure also shows the difference spectra obtained by subtracting<br />

the room-temperature spectra from spectra taken at low temperatures. The feature<br />

in the difference spectra corresponds to A, which originates from the e g↑ states [22].<br />

In order to estimate the relative changes in all the three features (A, B, and C)<br />

due to temperature, we have carefully fitted the whole valence band spectrum with

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