实验与计算对比的文字
This commit is contained in:
@@ -13,10 +13,11 @@ This approximation is based on the fact that
|
||||
the dispersion of these phonons is continuous and very close to the #sym.Gamma point,
|
||||
and has been widely adopted in the literature @_n-sic_2008.
|
||||
Symmetry analysis pointed out that
|
||||
these phonons correspond to twelve irreducible representations of the C#sub[6v] point group
|
||||
(2A#sub[1] + 4B#sub[1] + 2E#sub[1] + 4E#sub[2], see appendix for details).
|
||||
In which the B#sub[1] representation is Raman inactive,
|
||||
while other phonons are potentially observable in Raman experiments.
|
||||
these phonons correspond to twelve irreducible representations of the C#sub[6v] point group and were named accrodingly
|
||||
(A#sub[1]-1 to A#sub[1]-2, B#sub[1]-1 to B#sub[1]-4, E#sub[1]-1 to E#sub[1]-2, and E#sub[2]-1 to E#sub[2]-4,
|
||||
see appendix for details).
|
||||
Among which the B#sub[1] representation is Raman inactive,
|
||||
while other eight modes are potentially observable in Raman experiments.
|
||||
However, it should be noted that the intensity of Raman scattering from each mode
|
||||
cannot be inferred from symmetry considerations alone.
|
||||
|
||||
@@ -39,73 +40,50 @@ Furthermore, the absolute amplitude differences among atoms of the same type wit
|
||||
and only their vibrational directions were considered.
|
||||
This enables a preliminary estimation of the Raman tensor magnitudes prior to expensive first-principles calculations,
|
||||
with the results summarized in @table-nopol.
|
||||
Our analysis gave the result that the E#sub[2]-3 mode
|
||||
should possess a much higher Raman scattering intensity than the others,
|
||||
which is consistent with experimental and first-principles calculation results in the following text.
|
||||
Our analysis gave the result that the E#sub[2]-3 mode possess a much higher Raman intensity
|
||||
and should be clearly observable in Raman experiments,
|
||||
while the observability of other modes depends on their frequencies were well-separated or not
|
||||
and could only be confirmed by further first-principles calculations or experiments.
|
||||
Our result showed that
|
||||
the high Raman intensity of this mode arises from the constructive interference of contributions from all bonds,
|
||||
in contrast to other negligible-polar modes where contributions tend to cancel each other out.
|
||||
|
||||
#include "table-nopol.typ"
|
||||
|
||||
我们做了计算,估计哪些峰可以看到、哪些峰看不到。
|
||||
实验看到了7个峰,比别人多。
|
||||
|
||||
使用第一性原理计算得到了声子频率和拉曼张量的大小。
|
||||
我们的计算表明,E#sub[2]-1 E#sub[2]-2 E#sub[1]-1 A#sub[1]-1 E#sub[2]-3 模式的拉曼强度较高,并且被报道在绝大多数的拉曼实验中可以看到。
|
||||
A#sub[1]-2 被报道在一些实验中可以观测到而在另外一些实验中不可以观测到(cite)。
|
||||
我们的计算表明它在面内偏振下拉曼散射强度非常弱,但在 z 轴偏振下有可观测的强度;
|
||||
因此在正入射拉曼实验中可能难以看到,但在侧入射时通过选取合适的偏振配置应该可以观察到。
|
||||
E#sub[1]-2 和 E#sub[2]-4 模式位于最强模式 E#sub[2]-3 附近,且具有很弱的拉曼强度(分别为最强模式的0.1%和0.6%),在报道的实验中都不可见。
|
||||
E#sub[1]-2 与最强模式 E#sub[2]-3 表示不同,我们认为,通过选取合适的偏振配置,可能可以在实验中观察到。
|
||||
我们做了实验,看到了其中 7 个峰,比别人的实验要多。
|
||||
为了解释实验结果,我们进行了第一性原理计算。
|
||||
E#sub[2]-1 E#sub[2]-2 E#sub[1]-1 A#sub[1]-1 E#sub[2]-3 这几个模式在大多数实验中都可以看到,这是因为它们有较高的拉曼强度且位置比较分散。
|
||||
A#sub[1]-2 在一些实验中可以观察到而在另外一些实验中不可以观察到(cite),这是因为它在面内偏振下拉曼散射强度非常弱,但在 z 轴偏振下有可观测的强度;
|
||||
因此在我们的正入射拉曼实验中它很难被看到,但在侧入射时通过选取合适的偏振配置应该可以观察到。
|
||||
E#sub[1]-2 和 E#sub[2]-4 距离最强模式 E#sub[2]-3 很近,且具有很弱的拉曼强度,在报道的实验中都不可见。
|
||||
在我们的实验中,通过选取合适的偏振配置和延长积分时间,E#sub[2]-3 被压制后,E#sub[1]-2 也被观察到了。
|
||||
我们的实验第一次指出了 E#sub[1]-2 峰,并且与计算和理论吻合较好。
|
||||
|
||||
The Raman tensors and frequencies of the negligible-polar phonons were calculated using first-principles methods.
|
||||
The results showed that
|
||||
the E#sub[2]-1, E#sub[2]-2, E#sub[1]-1, A#sub[1]-1, and E#sub[2]-3 modes possess relatively high Raman intensities
|
||||
The calculated phonon frequencies were in good agreement with experimental values,
|
||||
with a slight underestimation of 2-5%,
|
||||
which might be attributed to the known tendency of the PBE functional underestimating interatomic forces (cite).
|
||||
The calculated Raman tensors were also consistent with both experimental and theoretical results.
|
||||
Among negligible-polar modes, the E#sub[2]-3 mode showed the highest Raman intensity,
|
||||
followed by four modes with lower intensities that were also visible in normal incidence Raman experiments,
|
||||
including the E#sub[2]-1 mode, the E#sub[2]-2 mode, the E#sub[1]-1 mode, and the A#sub[1]-1 mode.
|
||||
The E#sub[1]-2 mode and E#sub[2]-4 mode were not visible in our Raman experiments,
|
||||
as they were located close to the most intense E#sub[2]-3 mode (only about 10 cm#super[-1] away)
|
||||
with very weak Raman intensities (only 0.1% and 0.6% of the E#sub[2]-3 mode, respectively).
|
||||
Additionally,
|
||||
the A#sub[1]-2 mode had only a very weak Raman intensity under the incident light with in-plane polarization
|
||||
(only 0.01),
|
||||
but showed an observable intensity when the polarization is along the z-axis (1.78).
|
||||
Thus, it was not typically observed in normal incidence Raman experiments (cite),
|
||||
but could be clearly detected in edge incidence configurations in our experiments.
|
||||
|
||||
|
||||
我们做了实验,比别人多看到了几个峰;和计算结果比对良好。
|
||||
|
||||
拉曼散射实验在衬底上进行,并与第一性原理计算结果进行了比较。
|
||||
在我们的实验中,除了 E#sub[2]-4 以外的弱极性模式对应的拉曼散射峰都被观察到,多于其它实验;
|
||||
这包括 A#sub[1]-2 在 xzzx 下可以观察到,
|
||||
以及 E#sub[1]-2 在 xzyx 下通过额外延长积分时间而观察到。
|
||||
计算的声子频率与实验数据有很好的吻合,误差在 2-5% 之间,这个误差可能是由于 PBE 泛函对原子间力的低估(cite)。
|
||||
计算的拉曼张量也与实验和理论结果基本一致。
|
||||
|
||||
The Raman tensors and frequencies of the negligible-polar phonons were calculated using first-principles methods,
|
||||
and the results were compared with both experimental data and theoretical predictions (@table-nopol).
|
||||
The calculated phonon frequencies were in good agreement with experimental values,
|
||||
with a slight underestimation of 2-5%,
|
||||
which might be attributed to the known tendency of the PBE functional underestimating interatomic forces (cite).
|
||||
The calculated Raman tensors were also consistent with both experimental and theoretical results.
|
||||
Among negligible-polar modes, the E#sub[2]-3 mode showed the highest Raman intensity,
|
||||
followed by four modes with lower intensities that were also visible in normal incidence Raman experiments,
|
||||
including the E#sub[2]-1 mode, the E#sub[2]-2 mode, the E#sub[1]-1 mode, and the A#sub[1]-1 mode.
|
||||
The E#sub[1]-2 mode and E#sub[2]-4 mode were not visible in our Raman experiments,
|
||||
as they were located close to the most intense E#sub[2]-3 mode (only about 10 cm#super[-1] away)
|
||||
with very weak Raman intensities (only 0.1% and 0.6% of the E#sub[2]-3 mode, respectively).
|
||||
Additionally,
|
||||
the A#sub[1]-2 mode had only a very weak Raman intensity under the incident light with in-plane polarization
|
||||
(only 0.01),
|
||||
but showed an observable intensity when the polarization is along the z-axis (1.78).
|
||||
Thus, it was not typically observed in normal incidence Raman experiments (cite),
|
||||
but could be clearly detected in edge incidence configurations in our experiments.
|
||||
Raman experiments were established and seven negligible-polar phonon peaks were observed,
|
||||
which is more than all previous experiments (where only five or six peaks were typically reported).
|
||||
To further understand our experimental results,
|
||||
first-principles calculations were performed,
|
||||
and the result was compared with experimental data.
|
||||
Our calculation showed that the mode of E#sub[2]-1, E#sub[2]-2, E#sub[1]-1, A#sub[1]-1 and E#sub[2]-3
|
||||
had relatively high Raman intensities and well-separated frequencies,
|
||||
making them observed in our experiments as well as most previous experiments.
|
||||
The A#sub[1]-2 mode had only a very weak Raman intensity with in-plane polarization (e.g., zyy#overline[z]),
|
||||
while showed an observable intensity when the polarization is along the z-axis (e.g., xzzx).
|
||||
Thus, it could be observed clearly in our edge incidence experiments (xzzx),
|
||||
but hardly seen in normal incidence configurations.
|
||||
This peek was reported to be observable in some experiments (cite) but not in others (cite),
|
||||
our calculation provided an explanation for this discrepancy.
|
||||
The E#sub[1]-2 and E#sub[2]-4 modes are calculated
|
||||
to be located close to the most intense E#sub[2]-3 mode (< 10 cm#super[-1] away)
|
||||
and exhibit very weak Raman intensities (only 0.1% and 0.6% of the E#sub[2]-3 mode, respectively),
|
||||
making them hard to observe in reported experiments.
|
||||
However, in our experiments,
|
||||
with edge incidence configuration (zxy#overline[z]) and extended integration time,
|
||||
the E#sub[2]-3 peek was suppressed and the E#sub[1]-2 mode was also observed.
|
||||
Our experiments reported the E#sub[1]-2 peak for the first time,
|
||||
and the experimental results were in good agreement with both calculations and theoretical analysis.
|
||||
|
||||
#include "figure-raman.typ"
|
||||
|
||||
|
||||
@@ -48,6 +48,10 @@
|
||||
// E2 E2 A1 E2
|
||||
[0.228 #pm 0.051], [-0.260 #pm 0.025], m2[-0.279 #pm 0.016], [0 #linebreak() (used for calibration)],
|
||||
)},
|
||||
caption: [Negaligible-polarized Phonons at $Gamma$ Point.],
|
||||
caption: [
|
||||
Negaligible-polarized Phonons at $Gamma$ Point.
|
||||
The calculated phonon frequencies had a slight underestimation of 2-5% comparing to experimental values,
|
||||
which might be attributed to the known tendency of the PBE functional underestimating interatomic forces (cite).
|
||||
],
|
||||
)<table-nopol>]
|
||||
|
||||
|
||||
Reference in New Issue
Block a user