Active RIS vs. AF Relay
Active RIS vs. the Classical AF Relay
Active RIS and AF relays both amplify reflected signals. What's the difference? An AF relay is a single amplifier+antenna combo that receives on one antenna (or array) and retransmits on another. An active RIS is a distributed array of small amplifiers, each coupled to a sub-wavelength reflecting element. The distributed architecture enables coherent combining across elements — the same scaling that passive RIS enjoys, now with amplification. Active RIS is morally a "distributed amplify-and-forward relay" with phase control, and it inherits advantages of both.
Definition: AF Relay Reference Model
AF Relay Reference Model
A half-duplex AF relay has a single -antenna aperture and an amplifier of gain . In the receive phase, signal at the relay: ( is relay noise). In the transmit phase, the relay re-emits through its transmit antenna. Signal at the UE: .
Under half-duplex operation, the relay spends 1/2 the time receiving and 1/2 transmitting → rate loss factor of 2 (3 dB in rate). Active RIS is full-duplex (no receive phase needed), avoiding this penalty.
Theorem: Active RIS Beats AF Relay by (Full-Duplex Factor)
Compare active RIS (with elements, per-element amplifier gain , total amplifier power ) with an AF relay (single amplifier, gain , same total power ) under:
- Symmetric BS-RIS and RIS-UE channels.
- Matched-phase active RIS (coherent alignment).
- Same per-element amplifier noise figure.
Active RIS SNR = AF relay SNR (factor of 2 from full- duplex, factor of from coherent combining across elements vs. 1 relay).
At : active RIS beats the equivalent-power AF relay by . This is the decisive advantage.
Per-element amplifier gain is similar ( dB) in both active RIS and AF relays. The active RIS has elements combining coherently, giving an extra signal factor minus noise sharing (since noise adds independently per element), for net SNR boost over a single amplifier. Plus the half-duplex factor of 2: active RIS wins by in SNR compared to an AF relay with similar total amplifier power.
Signal
Active RIS coherent signal: where . AF relay signal: . Ratio: assuming .
Noise
Active RIS amplified noise: (noise per element × elements, incoherent sum). AF relay amplified noise: . Ratio: .
SNR ratio
Signal / noise ratio = (signal gain) / 1 (noise gain) = . Plus half-duplex factor of 2 in favor of active RIS (no receive phase). Total: .
The Relay Has Its Own Advantages
Despite the SNR gap, AF relays still have their niche:
- Physical form factor: a small box with a pair of antennas, vs. a planar array. Relay is easier to mount on a pole.
- Decode-and-forward (DF) relays can be noise-free by regenerating the signal. Beats active RIS in noise-dominated scenarios (adding baseband processing and latency).
- Backhaul integration: relays can be edge compute nodes with wired backhaul; active RIS is signal-only.
- Mature hardware: AF relays are off-the-shelf (WiFi range extenders, cellular repeaters); active RIS is research.
For modern deployments focused on link-budget closure, active RIS is the cleaner architectural win. For edge compute and multi-hop networking, relays remain relevant.
Active RIS vs. AF Relay vs. Passive RIS
Plot SNR vs. distance for three architectures: active RIS, AF relay, passive RIS. Active RIS dominates at moderate ; AF relay is better for very small ; passive is best when the link budget allows. Change amplifier power to see each regime.
Parameters
Practical Active RIS with Limited Amplifier Budget
Caire et al. (2023) address a practical gap in active-RIS theory: real RIS panels have total-power constraints (set by the DC supply and amplifier efficiency), not just per-element gains. They show that the optimal gain allocation is non-uniform: elements with stronger channels should receive more amplifier power. For -user scenarios, this becomes a joint resource allocation over elements and users. The algorithm (hybrid manifold + waterfilling) achieves improvement over uniform-gain active RIS at the same total DC power — a substantial win for constrained deployments. This is the CommIT contribution for the active-RIS chapter.
Active RIS Deployment Checklist
A pragmatic deployment guide:
- Identify the regime. Compute the passive-active crossover distance (Section 9.3). If typical UE distances exceed , go active.
- Size the panel. Active RIS is effective at smaller (256-512) than passive (1024+). Use this to reduce hardware cost.
- Budget DC power. Each element needs - mW. For : - W total. Ensure wired DC supply at the deployment site.
- Control cooling. Amplifier heat over a panel needs passive cooling. Thermal management is a first-order design consideration.
- Noise-figure optimization. Amplifier NF directly impacts the crossover. Invest in low-NF amplifiers () if the deployment is marginal.
- Fallback to passive. If amplifier noise dominates, the active RIS can operate at low gain (near-passive) and still work. Plan for degraded-mode operation.
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Typical active-RIS panel size: cm (sub-6 GHz), cm (mmWave).
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Total DC: W typical, W at aggressive gain.
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Amplifier MTBF: hours at moderate bias — longer than typical deployment.
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Heat dissipation: -.
Quick Check
At mmWave (28 GHz) with RIS elements and amplifier noise figure 5 dB, the active-passive crossover distance is:
m
cm
m
km
m. The crossover is extremely short at mmWave — active RIS is essentially always needed.
Common Mistake: Don't Push Amplifier Gain Past Saturation
Mistake:
"Higher means more SNR. Let's crank each amplifier to its max spec."
Correction:
Real amplifiers have a 1-dB compression point: above it, nonlinear distortion creates intermodulation products that look like interference to other users. Running close to compression creates spurious emissions, degrading system-level performance rather than improving it. Back off by - from compression to stay in the linear regime. The SNR gain is marginal above the linearity boundary; stability and cleanliness matter more than an extra dB.