Md Sherajul Islam1,2, Ashraful Hossain Howlader3, Rongkun Zheng3, Catherine Stampfl3, Jeongwon Park4,2, Akihiro Hashimoto5. 1. Department of Electrical and Electronic Engineering, Khulna University of Engineering and Technology, Khulna 9203, Bangladesh. 2. Department of Electrical and Biomedical Engineering, University of Nevada, Reno, Nevada 89557, United States. 3. School of Physics, The University of Sydney, Sydney, New South Wales 2006, Australia. 4. School of Electrical Engineering and Computer Science, University of Ottawa, Ottawa ON K1N 6N5, Canada. 5. Graduate School of Engineering, University of Fukui, Fukui 910-8507, Japan.
Abstract
We explored the mixing effect of 10B isotopes and boron (B) or nitrogen (N) vacancies on the atomic vibrational properties of (10,0) single-wall boron nitride nanotubes (BNNTs). The forced oscillation technique was employed to evaluate the phonon modes for the entire range (0-100%) of 10B isotopes and atomic vacancy densities ranging from 0 to 30%. With increasing isotope densities, we noticed a blue shift of the Raman-active A1 phonon peak, whereas an increased density of mixed or independent B and N vacancies resulted in the emergence of a new low-frequency peak and the annihilation of the A1 peak in the phonon density of states. High-energy optical phonons were localized as a result of both 10B isotopes and the presence of mixing defects. We found an asymmetrical nature of the localization length with increasing 10B isotope content, which corresponds well to the isotope-inherited localization length of carbon nanotubes and monolayer graphene. The localization length falls abruptly with the increase in concentration of both atomic vacancies (B or N) and mixing defects (10B isotope and vacancies). These findings are critical for understanding heat conduction and nanoscopic vibrational investigations such as tip-enhanced Raman spectra in BNNTs, which can map local phonon energies.
We explored the mixing effect of 10B isotopes and boron (B) or nitrogen (N) vacancies on the atomic vibrational properties of (10,0) single-wall boron nitride nanotubes (BNNTs). The forced oscillation technique was employed to evaluate the phonon modes for the entire range (0-100%) of 10B isotopes and atomic vacancy densities ranging from 0 to 30%. With increasing isotope densities, we noticed a blue shift of the Raman-active A1 phonon peak, whereas an increased density of mixed or independent B and N vacancies resulted in the emergence of a new low-frequency peak and the annihilation of the A1 peak in the phonon density of states. High-energy optical phonons were localized as a result of both 10B isotopes and the presence of mixing defects. We found an asymmetrical nature of the localization length with increasing 10B isotope content, which corresponds well to the isotope-inherited localization length of carbon nanotubes and monolayer graphene. The localization length falls abruptly with the increase in concentration of both atomic vacancies (B or N) and mixing defects (10B isotope and vacancies). These findings are critical for understanding heat conduction and nanoscopic vibrational investigations such as tip-enhanced Raman spectra in BNNTs, which can map local phonon energies.
Isotopes play an essential
role in manipulating the physical, chemical,
and biological phenomena of a material. Physical phenomena such as
nuclear fission or fusion, liquid or solid magnetic resonance, and
the superconducting transition temperature of metals[1,2] are due to the isotope effect. Chemical phenomena such as chemical
reactions change with isotopic contents when the substituted isotopes
participate directly in the chemical bonds that are broken or formed.
Biological phenomena such as complex biological reactions are traced
with unstable nuclei due to the isotope effect. As isotope content
changes the average mass of the material, it has the most significant
impact on the phonon (quanta of lattice vibrations) properties.[3] Especially in disordered nanotubes, the phonons
show some peculiar transport characteristics such as ballistic, diffusive,
and localized. The change in thermal conductivity in nanotubes due
to the isotope effect has also been demonstrated to have a substantial
impact.[4]The isotope effects are
even more pronounced in boron nitride nanotubes
(BNNTs) because natural boron (B) possesses a considerable isotopic
disorder. Natural BNNTs consist of 80.1% 11B and 19.9% 10B. Chang et al.[5] found a 50% enhancement
of thermal conductivity at room temperature with 99.5% 11B isotope in individual isolated multiwalled BNNTs using a microfabricated
test fixture with the facility of high-resolution transmission electron
microscopy. Savić et al.[6] found
dominant effects on the thermal conductivity reduction with isotope
disorder in BNNTs through ab initio calculations. They showed that
diffusive scattering was the main source of the decrease in thermal
conductivity, especially when the isotope concentration exceeded 10%.
They concluded that localization effects could not be extracted from
the thermal conductivity measurements. To demonstrate this dramatic
increase of thermal conductivity in almost isotopically pure BNNTs,
the same group developed an independent cascade scatter model of BNNTs.
They modeled thermal transport in BNNTs through the atomistic Green
function approach combined with first-principles phonon calculations.
They revealed that isotope-induced phonon scattering inhibited phonon
transport at high frequencies. In contrast, isotope enrichment enhances
thermal conductivity even in a totally diffusive environment in which
scatterers act independently.[7] From these
studies, it is evident that the impact of isotope disruption on nanotube
thermal conduction is still controversial and unclear.On the
other hand, the very first fabrication of BNNTs was described
by Chopra et al.,[8] which was based on an
arc discharge method. Besides the arc discharge method,[8,9] chemical vapor deposition[10,11] and laser ablation
methods[12,13] are also used for synthesizing BNNTs. During
these synthesis processes of BNNTs, there will be the introduction
of ubiquitous atomic vacancies, similar to their two-dimensional counterpart.[14] Moreover, intentional atomic vacancy creation
by irradiation was utilized to recognize the chirality of an independent
wall in multiwalled BNNTs by observing the direction or the growth
track of the vacancy defects.[15] Atomic
vacancies alter the continuity of the regular arrangement of the hexagonal
network and create dangling bonds. It has already been found that
atomic vacancies may change the electrical, optical, and magnetic
properties[16,17] of BNNTs. Thus, atomic vacancies
should have significant effects on the phonon properties of BNNTs.As BNNTs are structural analogues of carbon nanotubes (CNTs), it
is regarded that they should show the same effects on the phonon properties
due to alternation of the regular atomic arrangement, especially by
isotopes and vacancies.[18,19] Moreover, phonon scattering
by isotopes or vacancies significantly impact the electron–phonon
interaction in BNNTs,[20] leading to the
possible alteration of electron transport properties. Thus, an in-depth
analysis of individual isotopes and vacancies, as well as combinations
of these, in BNNTs, is indispensable. The phonon properties of pristine
BNNTs have been explored in the literature using a valence shell model,[21] Ab initio calculation,[22] the force constant model,[23,24] the continuum model,[25] Raman spectroscopy,[26−29] and infrared spectroscopy.[30] Even though the phonon properties in disordered
BNNTs have been discussed in several theoretical and experimental
studies, a comprehensive investigation of this problem in natural
systems with a large atomic scale is still absent. Moreover, to our
knowledge, there is no work on phonon properties of BNNTs with both
isotopes and vacancies.Here, a systematic, detailed study of
the effects of isotopes and
vacancies (individual B and N atoms), as well as mixed isotopes and
vacancy defects, on the phonon characteristics of BNNT is presented.
The forced oscillation technique (FOT), established by Williams and
Maris[31] for a disordered system with a
large number of atoms, was used to determine the phonon eigenmodes
of disordered BNNTs. It was found that in an isolated system having
a single electron and disordered potential, the eigenmodes were in
exponentially localized states, whereas the eigenmodes were in spatially
diffusive states with periodic potentials. This phenomenon is called
Anderson localization.[32] In a disordered
system, phonons should also be confined just like electrons. In most
cases, a substantial vibrational amplitude arises around defects and
decays exponentially into the system’s pristine area. It was
perceived that the phonon modes in a disordered system shifted to
the outside of the normal-frequency region.[33,34] Here, we step by step inspect the properties of vibrational modes
in disordered BNNTs addressing the questions of how the modes shift
and the mode patterns localize.
Methods
The translation vector (T)
and the chiral vector (C) of the nanotube
related to its length and width, respectively, were multiplied to
determine the unit cell[35] of single-walled
BNNTs (SWBNNTs). Figure shows the isotope and vacancy-defected ball–stick model and
the Brillouin zone (BZ) of (10,0) SWBNNTs. The unit cell of a (10,0)
SWBNNT consists of 20 B and 20 N atoms.
Figure 1
(a) Ball and stick model
of isotope and vacancy-defected SWBNNTs.
Copper-blue balls are N atoms, rosy-pink balls are 11B
atoms, and light-black balls are 10B atoms. (b) BZ of the
(10,0) zigzag SWBNNTs with high-symmetry points. The BZ consists of
N number of straight lines through the k space of
h-BN, each with a length of 2π/T, where T and N represent the BNNT unit cell length
and the number of h-BN unit cells in a single BNNT unit cell, respectively.
Here, T and N are 0.435 nm and 20,
respectively. k and kθ are the wave vectors along the tube
axis and perpendicular to it, respectively.
(a) Ball and stick model
of isotope and vacancy-defected SWBNNTs.
Copper-blue balls are N atoms, rosy-pink balls are 11B
atoms, and light-black balls are 10B atoms. (b) BZ of the
(10,0) zigzag SWBNNTs with high-symmetry points. The BZ consists of
N number of straight lines through the k space of
h-BN, each with a length of 2π/T, where T and N represent the BNNT unit cell length
and the number of h-BN unit cells in a single BNNT unit cell, respectively.
Here, T and N are 0.435 nm and 20,
respectively. k and kθ are the wave vectors along the tube
axis and perpendicular to it, respectively.In this analysis, we used 125-unit cells with a
total of 5000 atoms
and a length of 54.37 nm. Ballistic transport of charge carriers will
be possible with such a length since it is smaller than 100 nm.[36] Site percolation theory was employed to introduce 10B isotope and atomic vacancies into the structure. The maximum
bond probability of ∼70% can be achieved for the honeycomb
site percolation structure. Thus, we investigate a wide range of vacancy
densities up to 30% and isotope levels up to 100%. The fourth-nearest
neighbor atomic interactions are considered using the force constants
derived by Xiao et al. for the planar h-BN sheet.[37] Because of the curvature effect, the force constants of
SWBNNTs and the h-BN planar sheet are not the same. We have corrected
the force constants of the SWBNNT by calculating the changes in the
bond angles of the cylindrical tube relative to the planar h-BN sheet.
The approach to achieve the curvature effect is depicted in Figure a,b. Considering
a force constant K, between two atoms A (B atom)
and B (N atom), the projection of B on the xy-plane
and its force constant tensor are denoted as B′
(unfilled circle) and K′, respectively, as
shown in Figure a. K and K′ rotate around the y-axis at an angle of ϕ/2, where ϕ denotes the
central angle between A and B. The projection of B′ on the zx-plane and its force constant
tensor are represented as B″ (unfilled circle) K″, where K″ is parallel
to the x-axis. Using the new bond angles in the cylindrical
SWBNNTs compared to the planar h-BN sheet, the force constants of
the SWBNNTs are calculated. Table shows the modified force constants.
Figure 2
(a) View of SWBNNTs from
the top. The projection of the B atom
(filled circle) on the xy-plane is denoted as (unfilled
circle). (b) Side view of the SWBNNT. The projection of B′ (unfilled circle) on the zx-plane is denoted
as B″ (unfilled circle).
Table 1
Corrected Force Constant Parameters
for (10,0) SWBNNTs in Units of 104 dyn/cm by Adding the
Bending Effecta
force constant
parameters
ref.[37]
corrected
force constants for (10,0) SWBNNT
φr(1)
31.00
30.61557
φr(2B–B)
7.00
6.737185
φr(2N–N)
8.00
7.69964
φr(3)
1.00
0.949699
φr(4)
–1.90
–1.72893
φti(1)
18.50
18.27058
φti(2B–B)
–3.23
–3.10873
φti(2N–N)
–0.73
–0.702592
φti(3)
–3.25
–3.08652
φti(4)
1.29
1.17385
φto(1)
5.60
5.530554
φto(2B–B)
–0.70
–0.673719
φto(2N–N)
–0.55
–0.52935
φto(3)
0.65
0.6173044
φto(4)
–0.30
–0.272988
Here, r, ti, and to represent the
radial, transverse in-plane, and transverse out-of-plane, respectively.
(a) View of SWBNNTs from
the top. The projection of the B atom
(filled circle) on the xy-plane is denoted as (unfilled
circle). (b) Side view of the SWBNNT. The projection of B′ (unfilled circle) on the zx-plane is denoted
as B″ (unfilled circle).Here, r, ti, and to represent the
radial, transverse in-plane, and transverse out-of-plane, respectively.The FOT was used to estimate the eigenstate and localization
phenomena
of phonons for defective SWBNNTs. Usually, a large system is required
to quantify the defect effects precisely. However, the dynamical matrix
technique or first-principles calculations are limited by a small-scale
system. Moreover, it is also challenging to extract the low-frequency
modes by these techniques. The main advantage of the FOT is that if
we know only the force constants and atomic mass of the system, we
can determine the phonon characteristics of any disordered, complex,
and large system over the whole frequency range by calculating the
total energy of the system without knowing the phonon lifetime.The principal idea of the FOT comes from the resonance of a mechanical
system upon application of excitation. A resonant state with frequency
Ω can be acquired in a lattice dynamical system if an uninterrupted
excitation having an exterior continuous periodic force of frequency
Ω is imparted to the system for a long time. If M and u, respectively, are the mass and displacement of
the lth atom of a lattice dynamical system consisting
of N atoms, the equation of motion of the system can be described
aswhere the spring constant among the lth atom and l′th atom is φ and F is the continuous periodic exterior
force. The mathematical expression of F is . Here, F0 is
a time-independent constant and ϕ is an arbitrary number between 0 to 2π. We can write the displacement u of the system aswhere Qλ corresponds to a normal mode and Qλ (t) and e (λ) are the magnitude and displacement values of λ,
respectively. The average value of E can be obtained
by averaging all possible ϕ values
asThe modes whose frequencies fall within
the range about ∓(2π/t) of Ω contribute
to the sum in eq . t is chosen in such a way
that Ωt ≫ 1, which means that the sum
in eq is contributed
by only a small range of frequency modes in the Ω scale. The
number of such modes are greater than unity. Thus, the sum in eq can be represented as
a delta (δ) function, which provides the average energy aswhere g(Ω) signifies
the partial density of states (PDOS). Hence, the task is reduced to
obtaining the time evolution of the equations of motion upon application
of an external force. If time t is discretized with
a step τ, the equations of motion can be expressed aswhere n is the number of
time steps defined as t = nτ.
The step size τ should be small enough to get a fine resolution.
Here, τ is chosen as 0.01 × 10–13. Usually,
typical atomic vibrational frequencies lie within the range of approximately
1012 to 1014 Hz. Thus, the frequency of the
external applied force is chosen as 1013 Hz to extract
each frequency mode of the system. The system reaches the resonant
condition after a long period of external excitation. Under the resonant
condition, the average total energy of the system is calculated from
which the PDOS is calculated asThe eigenvector of the disordered SWBNNT
is also calculated. After
driving the system for a certain reasonable time period T, u(1) becomes the new displacement of an
atom l. Following that time period, a new force with
a new value is assigned to atom l and is written
as F(1) = u(1)M. The eventual displacement after p iterations can be represented ashere, C stands for a constant.
Therefore, the spatial eigenvector for the mode λ1 can be attained.
Results and Discussion
Figure shows the
estimated PDOS of 10B isotope-containing (0–100%)
SWBNNTs. As expected, Van Hove singularities appear in the estimated
PDOS caused by the confinement effect of the reduced dimensionality
of SWBNNTs. The PDOS successfully generates all the distinctive peaks
associated with the sp2 bonded B–N compound. The
estimated PDOS is quite similar to that of the 2D h-BN sheet, except
for tiny peaks induced by one-dimensional singularities. The high-energy
in-plane tangential G-band phonon modes [longitudinal optical (iLO)
and transverse optical (iTO)] are of primary attention in this study.
Generally, the E2g peak in PDOS is Raman-active in armchair-edged
BNNTs, similar to 2D h-BN; however, the A1 peak is Raman-active
in zigzag-edged BNNTs.[21,22,24,27,29] We observe
the A1 peak at 1376 cm–1 in our simulations
to be smaller than the value (E2g) obtained for 2D h-BN[38] due to the curvature effect.[18] The curvature effect of BNNTs softens this Raman-active
mode frequency to the lower value, which is consistent with the earlier
results.[39]
Figure 3
PDOS of BNNTs with various 10B and 11B isotope
concentrations.
PDOS of BNNTs with various 10B and 11B isotope
concentrations.A general trend of moving all vibrational modes
toward the higher-energy
region is found when the 10B isotope level increases. The
A1 peak has a considerable upward shift due to the isotope
interaction. The previous studies found that adding a lighter (heavier)
isotope atom generates a large upward or downward move in the high-frequency
phonon mode.[40,41] However, the effect was negligible
in the low-frequency regime.[19,39] Usually, the phonon
lifetime for the low-frequency phonon modes for carbon-based and similar
BN structures shows power law behavior. Moreover, in-plane and out-of-plane
phonon modes have vastly different lifetime scales because of their
vastly different stiffness. Consequently, isotope impurities affect
the high-frequency phonon modes sensitively but not the low-frequency
modes for these types of structures. Prior studies also revealed that
the incorporation of heavier isotope atoms causes a significant downward
shift of the high-frequency phonon mode, whereas the impact is weaker
in the low-frequency regime.[42,43] Isotopic substitution
decreases the average atomic mass of BNNTs, and even a minor amount
of isotope in BNNTs can drastically alter the phonon characteristics.
An upward shift of the Raman-active phonon modes was also detected
in 10B isotope-containing BNNTs in the earlier study.[44] The frequency of vibrational mode ω is
related to the atomic mass M as ω ∝ M–1/2, showing that lowering the mass
can raise the frequency.Using the standard harmonic oscillator
theory, the linear upward
shift of frequencies due to isotope defects can be described asHere, ω11 and x signify the frequency of original BNNTs and the 10B isotope contents, respectively. The upward shift of the A1 peak as a function of 10B isotope concentration is depicted
in Figure . A comparison
of the values obtained from eq with the results of our computation is also shown. The solid
line represents the computed values of the prior relation, whereas
circles reflect our computational results. We discover that our computational
results and theoretical values are perfectly consistent. From 0 to
100% 10B isotope contents, the A1 mode shifts
upward by about 42 cm–1. The system contains the
same mass for both 0 and 100% 10B isotope concentrations.
However, the harmonic arrangement is disrupted beyond these two extreme
situations, and the mass of the nanotube should be the inverse of
the square root of both 11B and 10B atoms. With
the increase of 10B atoms in the system, the average atomic
mass decreases, resulting in a phonon frequency shift to the high-energy
regime.
Figure 4
10B isotope concentration vs Raman-active A1 mode frequency. The solid line is extracted from the simple harmonic
oscillator model described in eq .
10B isotope concentration vs Raman-active A1 mode frequency. The solid line is extracted from the simple harmonic
oscillator model described in eq .Next, we concentrate our investigation on the impacts
of vacancies
on BNNT phonon behavior. Vacancy defects have been demonstrated to
induce considerable deviations in phonon and heat conduction characteristics
of CNTs in previous studies. The bond length and energy can be altered
by vacancies, and the vibrational frequency is highly reliant on these
parameters.[45] Because of significant changes
in the phonon structure,[46−48] the effect of vacancy defects
on thermal conductivity is more noticeable than that of isotopes.
An earlier study[49] showed that the thermal
conductivity of a graphene nanoribbon (GNR) was reduced by 81% even
at a relatively low concentration of vacancies (0.1%). Different studies
on CNTs[50−52] manifested that 1–2% vacancy concentration
resulted in about a 50% reduction in the thermal conductivity.Again, some studies on silicene nanoribbons[53] and silicon nanotubes[54] found
around a 50% reduction in thermal conductivity with 1–2% atomic
vacancy concentration. Thus, the effects of vacancies on the phonon
characteristics of BNNTs are exciting. The impact of various concentrations
of B and N vacancies on the PDOS of BNNTs is presented in Figure a,b. Although the 10B isotope disorder causes an upward swing in vibrational
frequencies, the PDOS peaks show a widening and downward shift as
the vacancy concentration rises. For both types of vacancies, the
A1 peak has totally vanished at 10% and higher densities.
Using the bond-order theory, Xie et al.[55] demonstrated that phonons in 2D materials are dispersed greatly
by atomic vacancies. Vacancy disorders can also change the periodicity
of the sp2-hybridized BNNT structure. The momentum conservation
of the crystal is broken due to the disruption of the periodic order
by the significant density of vacancies. Consequently, the high-energy
phonon peaks no longer appear.
Figure 5
PDOS values of SWBNNTs with (a) 11B vacancies and (b)
N vacancies.
PDOS values of SWBNNTs with (a) 11B vacancies and (b)
N vacancies.The emergence of several abrupt peaks at low frequency
with increasing
vacancy concentration is another key feature of the phonon mode, as
seen in Figure . The
concentrations of unsaturated bonds of B and N atoms increase with
increasing vacancy concentration, which may cause a decrease in the
high-frequency phonon density. As a result, phonon modes migrate toward
the low-energy region. Phonon scattering in the low-frequency region
due to the defects was notable in CNTs, as demonstrated by Mingo et
al.[56] In addition to generating a substantial
peak, increasing defect density also lowers the average PDOS in the
low-frequency zone. Mahan et al.[57] discovered
the low-frequency flexural phonon modes with a quadratic dispersion
in the PDOS of CNTs. On the other hand, Mariani et al.[58] and Ochoa et al.[59] showed that the average PDOS of graphene reduces due to the stiffening
of the flexural phonon modes caused by the disorder-induced strain.
Jeon et al.[24] found flexure phonon modes
in BNNTs even though the constituting atoms (B and N) are polar in
nature. We believe that vacancies stiffen the flexural phonons, resulting
in a drop in the average PDOS in the low-frequency region.The
effect of isotope mixing with B or N vacancies on the BNNT
PDOS is depicted in Figure . Although the isotope disorder causes an upward change in
phonon modes, the combination of the isotope and vacancies appears
to have a downward shift. The vacancy disorder in BNNTs, however,
induces a more significant downward shift than the mixing defects.
As shown in Figure , the softening of the A1 peak is highly influenced by
defect density, with the descending shift being greater for B vacancies
than for other defects. Simon et al.[60] also
found similar results. They created a double-walled CNT in which the
inner wall was 13C enriched and the exterior wall was natural
carbon (i.e., 1.1% 13C and 98.9% 12C) enriched
along with inevitable vacancies. The 13C-enhanced inner
wall of the CNT caused a nonuniform expansion and descending shift
of the tangential G mode. The inevitable point defects present in
a system have a considerable impact on the phonon scattering owing
to the extreme sensitivity of phonon to mass disorder. The scattering
generated by point defects may cause the phonon to traverse through
new states, causing the PDOS to broaden. Furthermore, in a system
having a breakdown in its lattice symmetry by defects, the atomic
vibrations in that system can be identified outside of the ideal system’s
normal frequency range.[33,34] In a defect-free environment,
phonons are unrestricted to move; however, in the presence of isotopes
or vacancies, phonons become confined. In disordered systems, the
phonon mean free path changes according to the square of the localization
length. As a result, the phonon energy may collect at its defective
area, similar to the Anderson localization of electrons.[32] The static localized phonons lose their heat-carrying
properties. As a result, the standard transmission of thermal energy
through the sample material is hampered by these localized phonons.
However, phonon localization in low- dimensional materials can be
beneficial in a variety of applications, including thermoelectric
energy conversion and microelectronic heat management.[61−63] The normal linewidth of the Raman spectra is also caused by localized
phonons.[27] To explain the experimental
findings, a better understanding of isotope phonon localization and
vacancy-induced BNNTs is required.
Figure 6
PDOS values of BNNTs with a (a) mixture
of 10B isotope
and B vacancies and a (b) mixture of 10B isotope and N
vacancies.
Figure 7
Impurity concentration vs A1 mode frequency.
PDOS values of BNNTs with a (a) mixture
of 10B isotope
and B vacancies and a (b) mixture of 10B isotope and N
vacancies.Impurity concentration vs A1 mode frequency.The atomic-scale localization behavior of phonon
modes in SWBNNTs
has also been investigated in the presence of isotope and vacancy
defects. In a perfect system, the wave of a phonon is disturbed. However,
phonons can go through ballistic, diffusive, or confined regions in
a disordered structure. Defects cause the disruption of the momentum
conservation of the system. As a result of the interruption of momentum
conservation of the regular atomic arrangement, the wave vectors of
phonons cannot occupy regular quantum numbers. The phonons disperse
into various phonon states and become spatially confined. There have
been numerous attempts to estimate and display the phonon localization
events in isotope-defected nanostructures. Savić et al.[6] performed a first-principles analysis to investigate
phonon transmission in 14C isotope-enriched CNTs and 10B isotope-disordered BNNTs, claiming that the thermal conductivity
decrease in isotope-disordered CNTs and BNNTs is due to diffusive
scattering, whereas localization of phonons was not considered. Because
heat transport happens with ballistic and diffusive phonons, they
reasoned that phonon localization could not be seen. They projected
that localization effects would arise in optical modes with short
wavelengths. As a result, to see any localization effects, separate
experimental techniques competent for exploring these high-energy
modes are necessary. Using molecular dynamics modeling, Li et al.[64] examined the heat transport of isotope-disordered
GNRs and CNTs. They discovered that the loss in thermal conductivity
in CNTs is more significant than in GNR owing to strong optical phonon
localization. They calculated the phonon dispersion relation in an
attempt to depict the localized phonon modes but were unable to obtain
the actual image of the localization effect. The mixing effect of 10B isotopes and vacancies, as well as their independent effect
on the phonon localization in unfolded SWBNNTs, has been explored
here. We are particularly interested in high-frequency tangential
phonon modes.Figure depicts
the atomic vibrational patterns for the A1 phonon mode
at 1376 cm–1. The vibrational patterns displayed
here are based on 460 sites only. A sufficiently localized mode can
be retained in this site area, which reduces the need for a significant
number of atoms. The circle in Figure specifies an atom; larger circles denote 11B atoms, smaller circles indicate 10B atoms, and different
hues represent the strength of the displacement. The mode pattern
for pure BNNTs is shown in Figure a.
Figure 8
Typical mode patterns at ω = 1376 cm–1 for
unfolded SWBNNTs with (a) pristine, (b) 20% B vacancy, (c) 20% N vacancy,
(d) 20% 10B isotope, 20% combined (e) 10% 10B isotope and 10% B vacancies, and (f) 10% 10B isotope
and 10% N vacancy-defected structures. Each circle denotes an atom
(smaller circles are 10B atoms and larger circles are 11B atoms), and the colors denote the displacement, which is
linearly normalized by the maximum value. The intensity of the displacement
of each atom is presented by the color bar.
Typical mode patterns at ω = 1376 cm–1 for
unfolded SWBNNTs with (a) pristine, (b) 20% B vacancy, (c) 20% N vacancy,
(d) 20% 10B isotope, 20% combined (e) 10% 10B isotope and 10% B vacancies, and (f) 10% 10B isotope
and 10% N vacancy-defected structures. Each circle denotes an atom
(smaller circles are 10B atoms and larger circles are 11B atoms), and the colors denote the displacement, which is
linearly normalized by the maximum value. The intensity of the displacement
of each atom is presented by the color bar.The modes present an unequal distribution across
the entire sample
area. The mode patterns are determined by imposing a random force
proportionate to the displacement of atoms at each time step iteratively.
As a result, the eigenmode positions are expected to change over time.
The randomness of the eigenmodes could be due to other factors. Usually,
optical phonons experience more frequent scattering due to their high
density compared to the acoustic phonon in the PDOS. The range of
possible scattering outcomes is increased since scattering activities
are generally inelastic.[65] Consequently,
the coherent backscattering strength decreases owing to the reduced
possibility of a specific mode reversing its scattering order. However,
to achieve a high coherent backscattering effect, scattering events
should be entirely elastic.[66] As a result,
eigenmodes in the sample may appear at random.The presence
of the 10B isotope or vacancies in the
SWBNNT structure induces a spatially localized eigenmode in the displacement
pattern. Figure b–d
shows the mode patterns with a 20% randomly oriented 10B isotope and B or N vacancy-defected sample. Few modes are observed
to be confined and scattered irregularly across the sample area. The
displacement pattern for isotope (10%) mixing with vacancies (10%)
is shown in Figure e,f. The vibrational modes are not adequately diffused in this example,
and some vibrational modes are severely confined. Only a few atoms
vibrating with the highest amplitude are discovered concentrated near
the vacancy defects, indicating a significant localization. The location
of localized atoms remains unevenly distributed near the vacancies,
and it evolves through time. With increasing defect concentrations,
the localization impact becomes more substantial. Prior investigation
revealed that the thermal conductivity of nanotube structures reduces
with cumulative defect concentrations. The localization of phonons
due to the defects provides important evidence for earlier findings
because phonons are the primary heat carrier in semiconducting nanostructures.To further illustrate the degree of localization, the inverse participation
ratio (IPR) of the system is derived. It is possible to express the
IPR in the following waywhere u represents the eigenmode’s displacement of
the lth atom. In the localized state, a limited number
of atoms oscillate with the largest displacement. Considering the
normalization of the eigenvector among the n number
of atoms, the amplitude the localized atom is u =
1/√n. IPR = 1/n can now be
used to represent the inverse participation ratio. It is worth noting
that the strong localization can be achieved when n = 1 (i.e., IPR = 1), and only one atom oscillates in that mode.
With n = N and IPR = 1/N, a dispersed oscillation pattern with all atoms vibrating at the
same amplitude of u = 1/√N should be noticed. We calculated the localization length Lλ from the value of IPR, which is correlated
with the IPR as Lλ ∝ IPR–1/2,[67] and the Lλ of the state λ can be described aswhere L0 is the
unfolded SWBNNT size, that is, the 2D h-BN sheet, and IPR0 is the average value of IPRλ.Figure shows the
fluctuation of Lλ with the variation
of isotope concentration. The simulation was run with 5000 atoms at
= 1376 cm–1 for the A1 mode phonon. The
filled circles in Figure denote the average of 10 eigenmodes. Lλ is associated with IPRλ as Lλ ∞ IPRλ–1/2. It is projected that strong
localization will be obtained with the shortest localization length
and vice versa. According to the calculations, the localization length
decreases dramatically when isotope contents elevate from 0 to 60%
and then rise again from 60 to 100%. At a 60% isotope content, the
minimum localization length was discovered.
Figure 9
Localization length as
a function of 10B isotope concentration.
Localization length as
a function of 10B isotope concentration.Despite the asymmetrical behavior, this finding
is consistent with
the earlier work on single-layer graphene by Rodriguez-Nieva et al.[43] A variety of reasons could cause this erratic
character. The influence of decreasing the mass of a system (by adding 10B isotopes to a 11B lattice) differs from that
of increasing the system’s mass (by adding 11B isotopes
to a 10B lattice). Lλ is calculated from the IPR, which is derived from the eigenstate
amplitudes of atoms. The total mass of the system decreases as 10B atoms are added to the 11B lattice. This eigenstate
amplitude of the atoms with reduced mass will be larger than the pristine
structures’ eigenstate amplitude. The same thing happens when 11B impurities are introduced into a 10B lattice.
In both circumstances, the eigenstates of the pristine structure are
smaller than the IPR, causing a lower Lλ. In the reduced mass case, the effect of isotope addition is stimulatingly
abrupt. As a result, the localization length may have an asymmetrical
characteristic. There could be additional explanations for the asymmetry.The localization of phonons in the flat zones of dispersion relation
can readily happen as described by Savić et al.[6] Besides, they[6] also revealed
that optical phonons in the high-frequency region are predominantly
localized.[6] The defect-related backscattering
is considerable in the optical phonons in the high-frequency region,
as observed in CNTs.[68] An island with a
different frequency is developed for the localized eigenstate compared
to the rest of the atoms, which may be the physical origin of localization.The Lλ value for different combinations
of defects has also been extracted, as shown in Figure . The values of Lλ decay noticeably with the rise of mixing defects
or separate B or N point vacancies, as shown in Figure . For the same defect density,
the combined defects demonstrate a sudden decrease in behavior in
comparison to isotope disorder. This is because the bond length and
energy change when vacancies form in the lattice structure, which
modifies the force constant parameters. The force constants for the 10B isotope-containing sample, on the other hand, stay unchanged
since the bonding chemistry is unaffected by the additional neutron
in each nucleus. However, because of the mass change of the ion, the
isotope defect affects the dynamics. Because the frequency f is related to the system mass m as the
inverse of the square root (i.e., f ∝ m–1/2), changes in 10B isotope
mass can significantly modify the PDOS. The isotope mixing with vacancies,
however, changes the PDOS more suddenly. Thus, the comparison of the Lλ for different impurity concentrations
and different types of defects is not straightforward. As a result,
there may be a sharp drop in Lλ.
Figure 10
Impurity
concentration vs localization length of BNNTs with a mixture
of 10B isotope and (a) B and (b) N vacancies.
Impurity
concentration vs localization length of BNNTs with a mixture
of 10B isotope and (a) B and (b) N vacancies.
Conclusions
In summary, the FOT was
used to investigate the effects of 10B isotope mixing with
B or N point vacancies on SWBNNT phonon
modes. The PDOS analysis revealed that the Raman- active A1 phonon peak is highly prone to both 10B isotope and vacancy
disorders. With increasing isotope levels, the A1 mode
exhibited a fairly linear downshift to the low-frequency region. A
stronger downshift in the A1 mode was observed for vacancy
defects than for the isotope, and it vanished when defect concentrations
reached a certain level. In the low-energy regime, the mixing defects
generated a new sharp peak. We created typical mode patterns for different
types of disordered structures to demonstrate the phonon localization
processes caused by the defects. Both 10B isotope and mixing
defects caused high-energy optical phonons to be localized. With increasing 10B isotope levels, we discovered an asymmetrical character
of the localization length, which corresponds well to the isotope-inherited
localization length of CNTs and monolayer graphene. With the inclusion
of separate B or N point vacancies as well as mixing defects, the
localization length reduced abruptly. This paper gives a theoretical
framework for isotope- and vacancy-induced phonon properties, which
is crucial for understanding SWBNNT thermal conductivity and Raman
spectra.
Authors: F Simon; Ch Kramberger; R Pfeiffer; H Kuzmany; V Zólyomi; J Kürti; P M Singer; H Alloul Journal: Phys Rev Lett Date: 2005-06-27 Impact factor: 9.161
Authors: C W Chang; A M Fennimore; A Afanasiev; D Okawa; T Ikuno; H Garcia; Deyu Li; A Majumdar; A Zettl Journal: Phys Rev Lett Date: 2006-08-24 Impact factor: 9.161