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 NN small amplifiers, each coupled to a sub-wavelength reflecting element. The distributed architecture enables coherent combining across elements — the same N2N^2 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

A half-duplex AF relay has a single NRN_R-antenna aperture and an amplifier of gain gg. In the receive phase, signal at the relay: yR=h1s+wR\mathbf{y}_R = \mathbf{h}_1 s + \mathbf{w}_R (wR\mathbf{w}_R is relay noise). In the transmit phase, the relay re-emits gyRg\mathbf{y}_R through its transmit antenna. Signal at the UE: y=g(h2Hh1s+h2HwR)+wy = g(\mathbf{h}_2^H \mathbf{h}_1 s + \mathbf{h}_2^H \mathbf{w}_R) + w.

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 N/2N/2 (Full-Duplex Factor)

Compare active RIS (with NN elements, per-element amplifier gain gn2=PRIS/Ng_n^2 = P_{\text{RIS}}/N, total amplifier power PRISP_{\text{RIS}}) with an AF relay (single amplifier, gain g2=Prelayg^2 = P_{\text{relay}}, same total power Prelay=PRISP_{\text{relay}} = P_{\text{RIS}}) under:

  • Symmetric BS-RIS and RIS-UE channels.
  • Matched-phase active RIS (coherent alignment).
  • Same per-element amplifier noise figure.

Active RIS SNR = 2N2N \cdot AF relay SNR (factor of 2 from full- duplex, factor of NN from coherent combining across NN elements vs. 1 relay).

At N=256N = 256: active RIS beats the equivalent-power AF relay by 27 dB27\text{ dB}. This is the decisive advantage.

Per-element amplifier gain is similar (20\sim 20 dB) in both active RIS and AF relays. The active RIS has NN elements combining coherently, giving an extra N2N^2 signal factor minus noise sharing N\sqrt{N} (since noise adds independently per element), for net N2=N\sqrt{N}^2 = N SNR boost over a single amplifier. Plus the half-duplex factor of 2: active RIS wins by 2N2N in SNR compared to an AF relay with similar total amplifier power.

The Relay Has Its Own Advantages

Despite the SNR gap, AF relays still have their niche:

  1. Physical form factor: a small box with a pair of antennas, vs. a planar array. Relay is easier to mount on a pole.
  2. 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).
  3. Backhaul integration: relays can be edge compute nodes with wired backhaul; active RIS is signal-only.
  4. 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 NN; AF relay is better for very small NN; passive is best when the link budget allows. Change amplifier power to see each regime.

Parameters
256
20
100
5
🎓CommIT Contribution(2023)

Practical Active RIS with Limited Amplifier Budget

G. Caire, I. AtzeniIEEE Trans. Wireless Commun. (preprint)

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 KK-user scenarios, this becomes a joint resource allocation over NN elements and KK users. The algorithm (hybrid manifold + waterfilling) achieves 2-3 dB\sim 2\text{-3 dB} 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-rispower-allocationcaire-2023
⚠️Engineering Note

Active RIS Deployment Checklist

A pragmatic deployment guide:

  1. Identify the regime. Compute the passive-active crossover distance dd^\star (Section 9.3). If typical UE distances exceed dd^\star, go active.
  2. Size the panel. Active RIS is effective at smaller NN (256-512) than passive (1024+). Use this to reduce hardware cost.
  3. Budget DC power. Each element needs 5\sim 5-2020 mW. For N=256N = 256: 1\sim 1-55 W total. Ensure wired DC supply at the deployment site.
  4. Control cooling. Amplifier heat over a 0.5-m2\sim 0.5\text{-m}^2 panel needs passive cooling. Thermal management is a first-order design consideration.
  5. Noise-figure optimization. Amplifier NF directly impacts the crossover. Invest in low-NF amplifiers (<3 dB< 3\text{ dB}) if the deployment is marginal.
  6. 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.
Practical Constraints
  • Typical active-RIS panel size: 20×2020 \times 20 cm (sub-6 GHz), 10×1010 \times 10 cm (mmWave).

  • Total DC: 5\sim 5 W typical, 20\sim 20 W at aggressive gain.

  • Amplifier MTBF: 105\sim 10^5 hours at moderate bias — longer than typical deployment.

  • Heat dissipation: 3\sim 3-10W/dm210\,\text{W/dm}^2.

Quick Check

At mmWave (28 GHz) with N=256N = 256 RIS elements and amplifier noise figure 5 dB, the active-passive crossover distance dd^\star is:

1\sim 1 m

10\sim 10 cm

100\sim 100 m

1\sim 1 km

Common Mistake: Don't Push Amplifier Gain Past Saturation

Mistake:

"Higher gmaxg_{\max} 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 33-6 dB6\text{ dB} 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.