1. Introduction
Recently, high-order modulation formats with coherent detection have attracted extensive attention, since they can greatly improve the spectral efficiency (SE) of optical systems. One major issue in a coherent optical communication system is to recover carrier phase, which is perturbed by phase noise generated from the laser linewidths of both the transmitter and local oscillator (LO) [
1K. P. Ho, Phase-Modulated Optical Communication Systems (Springer, 2005).
]. Since the phase estimation (PE) is imperfect, the residual phase estimation error degrades the system performance. The bit-error rate (BER) performance of various modulation formats with phase estimation error has been considered in [
2K. Kikuchi, T. Okoshi, M. Nagamatsu, and N. Henmi, “Degradation of bit error rate in coherent optical communications due to spectral spread of the transmitter and the local oscillator,” J. Lightwave Technol. LT-2, 103–112 (1984).
–
7C. Yu, S. Zhang, P. Y. Kam, and J. Chen, “Bit-error rate performance of coherent optical M-ary PSK/QAM using decision-aided maximum likelihood phase estimation,” Opt. Express 18(12), 12088–12103 (2010). [CrossRef] [PubMed]
].
From previous experience, it is important to optimize the signal constellations in the two-dimensional space [
8Y. Li, S. Xu, and H. Yang, “Design of signal constellations in the presence of phase noise,” in Proc. VTC’08-Fall, (Sept. 21–24, 2008, Calgary, Canada), pp. 1–5.
,
9L. Xiao and X. Dong, “The exact transition probability and bit error probability of two-dimensional signaling,” IEEE Trans. Wireless Commun. 4(5), 2600–2609 (2005). [CrossRef]
]. In the presence of phase noise, large angular distance between adjacent symbols gives a robust protection over the phase estimation error. Since the angular distance between adjacent symbols in 8-star quadrature amplitude modulation (QAM) is
which is larger than the other possible 8-ary constellations and 16QAM, it makes 8-star QAM more noise-tolerant. Moreover, compared with the 8-star QAM with 45 degrees phase offset in the inner ring, simulation results show that our 8-star QAM has a larger laser linewidth tolerance, and also 8-star QAM is easier to be implemented in experiments. Thus, 8-star QAM is a promising modulation format in coherent optical communication systems. Therefore, in this paper, we evaluate the BER performance of 8-star QAM in the presence of a phase estimation error and additive white Gaussian noise (AWGN). We also obtain a simple and accurate approximate BER, which allows quick estimations of the BER performance and laser linewidth tolerance. Finally, the ring ratio optimization algorithm is derived to optimize the placement of points in 8-star QAM, thus giving the minimum BER. This approach illustrates the procedure in detail how to carry out the analysis for 8-star QAM, and can also be extended to other duo-ring modulation formats to optimize the performance.
2. Exact BER of 8-star QAM
In coherent optical detection, digital-signal-processing (DSP) based PE algorithms, such as M-th power [
6G. Goldfarb and G. Li, “BER estimation of QPSK homodyne detection with carrier phase estimation using digital signal processing,” Opt. Express 14(18), 8043–8053 (2006). [CrossRef] [PubMed]
] and Decision-aided (DA) maximum likelihood (ML) [
10S. Zhang, P. Y. Kam, C. Yu, and J. Chen, “Decision-aided carrier phase estimation for coherent optical communications,” J. Lightwave Technol. 28(11), 1597–1607 (2010). [CrossRef]
], are preferred at the receiver for carrier phase recovery. The PE algorithm has a residual phase estimation error
which degrades the system performance.
In the presence of a random phase error, the BER
of a modulation format can be calculated as
where
represents the BER conditioned on a phase error value
and
is the probability density function (PDF) of the phase error, which can be assumed as a Gaussian PDF with mean zero and variance
[
6G. Goldfarb and G. Li, “BER estimation of QPSK homodyne detection with carrier phase estimation using digital signal processing,” Opt. Express 14(18), 8043–8053 (2006). [CrossRef] [PubMed]
,
10S. Zhang, P. Y. Kam, C. Yu, and J. Chen, “Decision-aided carrier phase estimation for coherent optical communications,” J. Lightwave Technol. 28(11), 1597–1607 (2010). [CrossRef]
,
11W. C. Lindsey and M. K. Simon, Telecommunication Systems Engineering (Prentice-Hall, 1973).
]. Besides laser phase noise, additive white Gaussian noise (AWGN) also exists in the system. The PDF of the additive noise is also Gaussian with mean zero and variance
and the variance
is assumed to be 1 in our simulations.
The constellation map with Gray coding and decision boundaries is shown in
Fig. 1
. Here, in the figure, the dot lines are the decision boundaries.
denote the decision regions. The two hollow points represent the points when the two original signal points “000” and “100” are rotated by a phase error
Observe that there are two rings in the 8-star QAM constellation. The inner ring radius is defined to be
and the outer ring radius is
so the ring ratio
is equal to
We define
to be the average energy per symbol, and
is the average energy per bit, since there are 3 bits per symbol. Then
can be written as
where
is the coefficient of the inner ring.
can be expressed as
Since the mean of energies of the inner ring and outer ring should be equal to the average symbol energy
therefore,
So we have the relation
Fig. 1 Constellation map, decision boundaries and Gray code mapping of 8-star QAM with a phase error
Due to the symmetry (assuming that the symbols “000” and “100” are transmitted) and equal probability of transmitting each symbol, the average BER conditioned on a phase error
can be written as
Supposing that an inner ring symbol “000” is sent, the conditional BER
is defined as the expected number of bit errors made per bit detected [
12A. J. Viterbi and J. K. Omura, Principles of Digital Communication and Coding (McGraw-Hill, 1979).
], and is given by
where
is the probability of the received signal point falling in the decision region
when the symbol “000” is sent. Observe that
and
are half-planes, and thus
Eq. (5) can be represented as
It is easy to show that
Similarly, supposing that signal “100” is transmitted, the conditional BER is given by
where
and
are half-planes. We get
Combining
Eq. (4) through
Eq. (9c), the conditional BER in the presence of a random phase estimation error
in 8-star QAM can be obtained. The final expression is omitted for lack of space.
3. Distribution of phase estimation error in DA ML PE
With the conditional BER
of 8-star QAM obtained, we consider the PDF of the phase estimation error
It is shown in [
6G. Goldfarb and G. Li, “BER estimation of QPSK homodyne detection with carrier phase estimation using digital signal processing,” Opt. Express 14(18), 8043–8053 (2006). [CrossRef] [PubMed]
,
10S. Zhang, P. Y. Kam, C. Yu, and J. Chen, “Decision-aided carrier phase estimation for coherent optical communications,” J. Lightwave Technol. 28(11), 1597–1607 (2010). [CrossRef]
,
11W. C. Lindsey and M. K. Simon, Telecommunication Systems Engineering (Prentice-Hall, 1973).
] that the distribution of the phase error
is Gaussian
The relations between phase error variance
and linewidth per laser symbol duration product (
) are also given under different PE methods in [
6G. Goldfarb and G. Li, “BER estimation of QPSK homodyne detection with carrier phase estimation using digital signal processing,” Opt. Express 14(18), 8043–8053 (2006). [CrossRef] [PubMed]
] and [
10S. Zhang, P. Y. Kam, C. Yu, and J. Chen, “Decision-aided carrier phase estimation for coherent optical communications,” J. Lightwave Technol. 28(11), 1597–1607 (2010). [CrossRef]
]. Here, we only consider the DA ML PE algorithm to recover the carrier phase as an illustration. The laser phase noise is a random-walk process [
2K. Kikuchi, T. Okoshi, M. Nagamatsu, and N. Henmi, “Degradation of bit error rate in coherent optical communications due to spectral spread of the transmitter and the local oscillator,” J. Lightwave Technol. LT-2, 103–112 (1984).
] characterized by a white Gaussian frequency noise with mean zero and variance
where
and
are the beat linewidth of the transmitter and LO and symbol duration, respectively. The phase estimation error variance
of DA ML can be expressed, as described in [
10S. Zhang, P. Y. Kam, C. Yu, and J. Chen, “Decision-aided carrier phase estimation for coherent optical communications,” J. Lightwave Technol. 28(11), 1597–1607 (2010). [CrossRef]
], as
where
and L is the memory length (number of past symbols used to estimate the carrier phase). The accuracy of this expression is verified by using Monte Carlo (MC) simulations in [
10S. Zhang, P. Y. Kam, C. Yu, and J. Chen, “Decision-aided carrier phase estimation for coherent optical communications,” J. Lightwave Technol. 28(11), 1597–1607 (2010). [CrossRef]
]. It shows that the analysis of the phase estimation error variance agrees well with the MC results. The optimal L is also given in [
10S. Zhang, P. Y. Kam, C. Yu, and J. Chen, “Decision-aided carrier phase estimation for coherent optical communications,” J. Lightwave Technol. 28(11), 1597–1607 (2010). [CrossRef]
] as
where
represents the largest integer less than or equal to
Therefore, the analytical BER of 8-star QAM can be obtained by numerically integrating
Eq. (1) for the BER conditioned on a phase estimation error value against the PDF of the phase error.
Figure 2
illustrates that the analytical BER expression of 8-star QAM is verified by using MC simulations for different values of phase error variance
The perfectly coherent curve in
Fig. 2 is obtained by setting
in
Eq. (7) and
Eq. (9). As can be seen in
Fig. 2, the analytical BERs agree quite well with the MC simulations.
Fig. 2 The BERs of 8-star QAM from analysis and MC simulations with different phase error variance.
4. Approximate BER in 8-star QAM
For analytical purposes, it is desirable to have a simple and accurate approximate BER with respect to SNR and phase error variance instead of doing numerical integration of the conditional BER. This approximation can be used to quickly estimate the BER performance and laser linewidth tolerance of a system.
It can be observed that in order to get the approximate BER, we need to simplify the four error-functions (erfc) multiplication in
Eq. (7c) and
Eq. (9c) to a single erfc. Since
and
are the most dominant terms in
Eq. (7c) and
Eq. (9c), respectively, therefore, the final conditional BER expression can be approximated as
It can be seen that only some single erfc terms are left in
Eq. (12). Putting the 1st erfc term of
Eq. (12) into
Eq. (1), we obtain
The approximation
and
are used in the derivation, so
Eq. (13) can be further approximated to
since
The details of derivation of the other terms are left to the reader. Finally, the approximate BER in 8-star QAM can be expressed as
The approximation in
Eq. (15) is plotted in
Fig. 3
for
and
respectively, which correspond to linewidth per laser
of 100 kHz and 1 MHz in a 10Gsymbol/s system. Exact numerical results and MC simulations are also presented to show that the approximation is accurate. Here, optimum memory length
Eq. (11) is used to calculate the phase estimation error variance in
Eq. (10). Furthermore, it is also found that the derived approximate BER can quickly estimate the laser linewidth tolerance of 8-star QAM in DA ML PE. The laser linewidth tolerance is examined and plotted in
Fig. 4
based on our numerical integration and approximate results. The SNR reference is the SNR/bit (
) at BER = 10
−4 in the perfectly coherent case, which is 11.7dB. As shown in
Fig. 4, by using the approximate BER, the estimated value of
leading to a 1-dB SNR/bit (
) penalty at BER = 10
−4 is
for 8-star QAM. The estimated value of laser linewidth tolerance is smaller than the one using exact numerical BER, which is
This is because the approximate BER is an upper bound of the exact numerical BER. Therefore, it provides a more rigid laser linewidth requirement than the exact BER.
Fig. 3 Comparison between numerical BER, MC simulations, and approximate BER under different laser linewidth with optimum memory length.
Fig. 4 The SNR/bit penalty as a function of linewidth per laser symbol duration product () when BER = 10−4 from numerical integration and approximation.
5. Ring ratio optimization
Generally, varying the radii of the two rings in 8-star QAM would severely affect its performance. Therefore, we need to determine the optimal ring ratio. Based on
Eq. (15), an optimal ring ratio
can be obtained to give the minimum BER
From
Eq. (15), the term
can be dropped for simplicity because it is much smaller than
since the terms in the parentheses are both negative and
And also the terms
and
can be dropped since they are much less than 1. The dominant terms are left as
We substitute the relation
into
Eq. (16), use the approximation
differentiate it by
and make it equal to 0, drop
in the
term since
and arrive at the result
By solving
Eq. (17), we get the solution
From
Eq. (18a) to
(18d), it can be seen that optimal ring ratio
is a function of SNR/symbol
and phase error variance
The term
as a function of
is plotted in
Fig. 5
. We also scan the numerical BER of
Eq. (1) as a function of the ring ratio
given a fixed average
= 15dB and
and the result is shown in
Fig. 6
. It is shown that given the above condition the optimal ring ratio of 8-star QAM from numerical integration is 2.4. Then we substitute the same parameters into
Eq. (18a) to
(18d), and obtain the value of 2.45 for the optimal ring ratio from the approximation. The ring ratio shift is only 0.05, which corresponds to an SNR per bit penalty of 0.015dB at BER = 10
−4. We also examine the SNR penalty due to the ring ratio shift under this condition as depicted in
Fig. 7
. This figure illustrates that 8-star QAM can tolerate a large ring ratio fluctuation around the optimal ring ratio value. Although numerical integration can be used to determine the optimal ring ratio, it is time consuming. As can be seen in
Fig. 6, a large range of values of the ring ratio has to be scanned to locate the optimal value. The ring ratio optimization algorithm gives us an explicit way to see that the optimal ring ratio is not a constant, but depends on the product of SNR/symbol and phase estimation error variance. It also allows engineers to make a quick estimation of the optimal ring ratio under different parameters.
Fig. 5 Optimal ring ratio as a function of SNR/symbol phase error variance product.
Fig. 6 BER as a function of ring ratio from numerical integration given and
Fig. 7 SNR penalty due to ring ratio shift
6. Conclusion
In this paper, the conditional BER expression of 8-star QAM in the presence of a phase estimation error and AWGN is derived. The numerical results can be obtained by numerically integrating
Eq. (1) for the BER conditioned on a phase error value against the PDF of the phase error. An approximate BER is also presented analytically through a series of approximations. The approximate BER can be used in any PE algorithms given the PDF of the phase estimation error. It is found that this approximation can quickly estimate the BER performance under different parameters, such as SNR/bit, laser linewidth and symbol rate, and also can predict the lower bound on the laser linewidth requirement. The accuracy of the approximation is confirmed via numerical integration and MC simulation.
To optimize the BER performance, the approximate BER is minimized with respect to the ring ratio. This leads to a new ring ratio optimization algorithm. It is found that the optimal ring ratio is not a constant, but depends on two parameters, namely, SNR/symbol and phase error variance. This algorithm can provide us a quick estimation of the optimal ring ratio for different parameters, instead of using time-consuming numerical integration and scanning over a large range of values of ring ratio. Therefore, our work shows how to place the signal points to optimize the performance in 8-star QAM, and can also be applied for other duo-ring modulation formats.