UNCORRECTED PROOF
YSPMI: 1213 pp. 1–6 (col. fig: NIL)
ARTICLE IN PRESS
Superlattices and Microstructures xx (xxxx) xxx–xxx
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Interband magneto-optics in single-walled carbon
nanotubes
S. Zaric
a
, G.N. Ostojic
a
, A.D. Engroff
a
, J. Kono
a,∗
, J. Shaver
b
,
V.C. Moore
b
, M.S. Strano
b
, R.H. Hauge
b
, R.E. Smalley
b
,
X. Wei
c
a
Department of Electrical and Computer Engineering, Rice University, Houston, TX 77005, USA
b
Department of Chemistry, Rice University, Houston, TX 77005, USA
c
National High Magnetic Field Laboratory, Tallahassee, FL 32310, USA
Abstract 1
We have carried out magneto-absorption and magneto-photoluminescence experiments on 2
micelle-suspended single-walled carbon nanotubes in magnetic fields up to 45 T. Chirality-assigned 3
spectral peaks exhibit significant changes with increasing magnetic field, which can be quantitatively 4
explained in terms of the theoretically predicted splittings and redshifts of the band edge due to the 5
Aharonov–Bohm effect combined with the magnetic-field-induced alignment of the nanotubes. 6
© 2003 Elsevier Ltd. All rights reserved. 7
The properties of a single-walled carbon nanotube (SWNT) sensitively depend on the 8
chirality vector C
h
= (n, m) [1]. When n - m = 3 M + ν( M: integer,ν =±1), 9
the nanotubes are direct-gap semiconductors with promising optical properties. However, 10
early optical experiments did not reveal any chirality-dependent features, presumably 11
due to their affinity to stick together to form bundles [2]. Recent success in preparing 12
unbundled SWNTs in aqueous solutions led to the observation of peaks in absorption 13
and photoluminescence (PL) spectra and to complete chirality assignments [3]. This has 14
opened ways to perform spectroscopy of SWNTs of specific chiralities. 15
One of the experimentally unexplored aspects is the influence of a magnetic field ( B ) on 16
a nanotube’s electronic structure through the Aharonov–Bohm effect [4]. In an interesting 17
interplay with a nanotube’s zero-field electronic structure, B parallel to the tube axis is 18
∗
Corresponding author. Tel.: +1-713-348-2209; fax: +1-713-348-5686.
E-mail address: kono@rice.edu (J. Kono).
0749-6036/$ - see front matter © 2003 Elsevier Ltd. All rights reserved.
doi:10.1016/j.spmi.2004.03.060