TY - JOUR
T1 - Topological Transitions and Fractional Charges Induced by Strain and a Magnetic Field in Carbon Nanotubes
AU - Efroni, Yonathan
AU - Ilani, Shahal
AU - Berg, Erez
N1 - Publisher Copyright: © 2017 American Physical Society.
PY - 2017/10/5
Y1 - 2017/10/5
N2 - We show that carbon nanotubes (CNT) can be driven through a topological phase transition using either strain or a magnetic field. This can naturally lead to Jackiw-Rebbi soliton states carrying fractionalized charges, similar to those found in a domain wall in the Su-Schrieffer-Heeger model, in a setup with a spatially inhomogeneous strain and an axial field. Two types of fractionalized states can be formed at the interface between regions with different strain: a spin-charge separated state with integer charge and spin zero (or zero charge and spin ±/2), and a state with charge ±e/2 and spin ±/4. The latter state requires spin-orbit coupling in the CNT. We show that in our setup, the precise quantization of the fractionalized interface charges is a consequence of the symmetry of the CNT under a combination of a spatial rotation by π and time reversal.
AB - We show that carbon nanotubes (CNT) can be driven through a topological phase transition using either strain or a magnetic field. This can naturally lead to Jackiw-Rebbi soliton states carrying fractionalized charges, similar to those found in a domain wall in the Su-Schrieffer-Heeger model, in a setup with a spatially inhomogeneous strain and an axial field. Two types of fractionalized states can be formed at the interface between regions with different strain: a spin-charge separated state with integer charge and spin zero (or zero charge and spin ±/2), and a state with charge ±e/2 and spin ±/4. The latter state requires spin-orbit coupling in the CNT. We show that in our setup, the precise quantization of the fractionalized interface charges is a consequence of the symmetry of the CNT under a combination of a spatial rotation by π and time reversal.
UR - http://www.scopus.com/inward/record.url?scp=85030775259&partnerID=8YFLogxK
U2 - 10.1103/PhysRevLett.119.147704
DO - 10.1103/PhysRevLett.119.147704
M3 - مقالة
C2 - 29053312
SN - 0031-9007
VL - 119
JO - Physical review letters
JF - Physical review letters
IS - 14
M1 - 147704
ER -