Spectral Efficiency and Power Efficiency Trade-offs

The Fundamental Design Trade-off

Every modulation scheme sits at a specific point in the bandwidth efficiency vs power efficiency plane. A system designer must choose a modulation format that meets both the spectral efficiency requirement (bits/s/Hz) and the power budget (required Eb/N0E_b/N_0). This section maps the standard modulation formats onto this plane and compares them against the ultimate limit: the Shannon capacity bound.

Definition:

Bandwidth Efficiency

The bandwidth efficiency (or spectral efficiency) of a modulation scheme is

η=RbW=log⁑2M1+αbits/s/Hz\eta = \frac{R_b}{W} = \frac{\log_2 M}{1 + \alpha} \quad \text{bits/s/Hz}

where RbR_b is the bit rate, W=(1+Ξ±)Rs/2W = (1+\alpha)R_s/2 is the occupied bandwidth, and Ξ±\alpha is the roll-off factor.

Higher-order modulations (larger MM) increase Ξ·\eta but require higher Eb/N0E_b/N_0 for the same BER β€” the fundamental trade-off in modulation design.

Definition:

Power Efficiency

The power efficiency of a modulation scheme is characterised by the required Eb/N0E_b/N_0 (in dB) to achieve a target bit error rate, typically BER=10βˆ’5\text{BER} = 10^{-5} or 10βˆ’610^{-6}.

For MM-QAM in AWGN, the approximate BER is

Pbβ‰ˆ4log⁑2M(1βˆ’1M)Q ⁣(3log⁑2MMβˆ’1β‹…2EbN0)P_b \approx \frac{4}{\log_2 M}\left(1 - \frac{1}{\sqrt{M}}\right) Q\!\left(\sqrt{\frac{3\log_2 M}{M-1} \cdot \frac{2E_b}{N_0}}\right)

The required Eb/N0E_b/N_0 grows logarithmically with MM: doubling Ξ·\eta costs approximately 3 dB of additional Eb/N0E_b/N_0.

The Shannon limit on power efficiency for reliable communication at spectral efficiency Ξ·\eta is

EbN0∣Shannon=2Ξ·βˆ’1Ξ·\frac{E_b}{N_0}\bigg|_{\text{Shannon}} = \frac{2^\eta - 1}{\eta}

At the ultimate limit Ξ·β†’0\eta \to 0: Eb/N0β†’ln⁑2=βˆ’1.59E_b/N_0 \to \ln 2 = -1.59 dB.

,

Theorem: Shannon Limit on Bandwidth Efficiency

For an AWGN channel with bandwidth WW and received SNR SNR=Es/(N0W)\text{SNR} = E_s / (N_0 W), the channel capacity is

C=Wlog⁑2 ⁣(1+SNR)bits/sC = W \log_2\!\left(1 + \text{SNR}\right) \quad \text{bits/s}

Expressing in terms of spectral efficiency Ξ·=C/W\eta = C/W and Eb/N0=SNR/Ξ·E_b/N_0 = \text{SNR}/\eta:

Ξ·=log⁑2 ⁣(1+Ξ·β‹…EbN0)\eta = \log_2\!\left(1 + \eta \cdot \frac{E_b}{N_0}\right)

This implicit equation defines the Shannon boundary in the (Ξ·,Eb/N0)(\eta, E_b/N_0) plane. No modulation scheme can operate to the left of this boundary (higher Ξ·\eta for a given Eb/N0E_b/N_0) with arbitrarily low error probability.

Any practical modulation scheme operates at a Shannon gap Ξ“\Gamma (in dB) to the right of the boundary. The gap depends on the constellation and coding scheme.

Shannon's theorem says you can trade bandwidth for power (and vice versa) along the capacity curve, but you cannot escape the curve. The bandwidth efficiency plane is a convenient way to visualise where each modulation sits relative to this limit.

,

Bandwidth Efficiency Plane

The bandwidth efficiency plane plots spectral efficiency Ξ·\eta (bits/s/Hz) against required Eb/N0E_b/N_0 (dB) for a target BER. Standard modulation schemes appear as discrete points, and the Shannon limit defines the ultimate boundary. Observe how each modulation format trades power for bandwidth efficiency.

Parameters

Modulation Formats β€” Efficiency Summary

FormatΞ·\eta (bits/s/Hz)Eb/N0E_b/N_0 (dB)Constant envelope?
BPSK19.6Yes
QPSK29.6Yes
8-PSK313.0Yes
16-QAM413.5No
64-QAM617.8No
256-QAM821.5No
MSK19.6Yes
GMSK (BT=0.3BT=0.3)1.3510.0Yes
16-APSK413.2Quasi

Why This Matters: Modulation in MIMO Systems

In a MIMO system with nTn_T transmit antennas, the modulation problem extends from choosing a point in a one- or two-dimensional signal space to choosing a vector in a 2nT2n_T-dimensional space (I and Q per antenna). The signal-space geometry of this chapter generalises directly:

  • Spatial multiplexing: transmit independent QAM symbols on each antenna, using the MIMO channel's spatial dimensions to multiply throughput
  • Space-time codes: design constellations in the nTΓ—Tn_T \times T matrix space to achieve both diversity and multiplexing gain

The bandwidth efficiency plane extends to MIMO: with nTn_T antennas and rank-rr channel, the spectral efficiency scales as Ξ·β‰ˆrlog⁑2M\eta \approx r \log_2 M bits/s/Hz. The MIMO book develops these extensions in full detail.

Information-Theoretic Foundations

The Shannon limit on bandwidth efficiency invoked in this section is a consequence of the AWGN channel coding theorem, which establishes that rates up to C=Wlog⁑2(1+SNR)C = W\log_2(1 + \text{SNR}) are achievable with vanishing error probability using sufficiently long codes. The converse β€” that rates above CC are not achievable β€” is equally important. Both are developed with full proofs in the Information Theory and Applications (ITA) book and summarised in Chapter 11 of this book.

Key Takeaway

The Shannon gap is the additional Eb/N0E_b/N_0 (in dB) required by a practical modulation/coding scheme compared to the Shannon limit at the same spectral efficiency. Uncoded modulation typically has a gap of 8-10 dB. Modern LDPC and turbo codes reduce this gap to 1-2 dB. Closing the Shannon gap is the central goal of coded modulation design (Chapter 12).

Why This Matters: Adaptive Modulation and Coding in 5G

Modern wireless systems do not use a fixed modulation scheme. Instead, they adapt the modulation order and code rate to the instantaneous channel conditions:

  • When the channel is strong (high SNR): use 256-QAM with high code rate for maximum spectral efficiency
  • When the channel is weak (low SNR): fall back to QPSK with low code rate for reliability

In 5G NR, this is implemented through the MCS table (Modulation and Coding Scheme), which maps a Channel Quality Indicator (CQI) to a specific combination of modulation order and code rate. The MCS index ranges from 0 (QPSK, rate 0.12) to 27 (256-QAM, rate 0.93), covering spectral efficiencies from 0.23 to 7.41 bits/s/Hz.

This adaptive approach moves along the bandwidth efficiency plane in real time, tracking the Shannon boundary as closely as the finite MCS table allows.

See full treatment in Adaptive Modulation and Coding in OFDM

Quick Check

The Shannon limit at Ξ·=0\eta = 0 is Eb/N0=βˆ’1.59E_b/N_0 = -1.59 dB. What does this fundamental limit represent?

The minimum SNR for any reliable communication

The minimum energy per bit for reliable communication at vanishing rate

The noise figure of an ideal receiver

The coding gain of turbo codes

Spectral Efficiency

The data rate achievable per unit bandwidth, measured in bits/s/Hz. For MM-ary modulation with roll-off α\alpha: η=log⁑2M/(1+α)\eta = \log_2 M / (1 + \alpha).

Related: Bandwidth Efficiency, Shannon Limit, Modulation Order

Shannon Gap

The excess Eb/N0E_b/N_0 (in dB) required by a practical modulation and coding scheme relative to the Shannon capacity limit at the same spectral efficiency. Modern codes achieve gaps of 1-2 dB.

Related: Shannon Limit, Multiple Antennas and Capacity, Low-Density Parity-Check (LDPC) Code