Prerequisites & Notation

Before You Begin

This chapter develops the signal model that the rest of the book will optimize. If any prerequisite below is unfamiliar, a quick refresher will save time later — every optimization chapter assumes fluency with the cascaded-channel formulas derived here.

  • ULA / UPA steering vectors: a(θ)CN\mathbf{a}(\theta) \in \mathbb{C}^{N}(Review ch07)

    Self-check: Can you write the steering vector of an N1×N2N_1 \times N_2 UPA at AoA (θ,ϕ)(\theta, \phi) as the Kronecker product of two ULA vectors?

  • Rayleigh and Ricean fading: LoS component + i.i.d. Gaussian(Review ch06)

    Self-check: Given a K-factor KRiceK_{\text{Rice}}, can you decompose the channel into deterministic and random parts?

  • Kronecker correlation model: H=Rr1/2H~Rt1/2\mathbf{H} = \mathbf{R}_r^{1/2} \tilde{\mathbf{H}} \mathbf{R}_t^{1/2}(Review ch02)

    Self-check: What does the rank of Rt\mathbf{R}_t tell you about the number of significant transmit eigendirections?

  • Fraunhofer distance: dF=2D2/λd_F = 2D^2/\lambda where DD is the aperture dimension(Review ch05)

    Self-check: Compute dFd_F for a 1 m21\text{ m}^2 aperture at 28 GHz.

  • Rank and condition number of a matrix; keyhole channels(Review ch15)

    Self-check: Why does a rank-1 channel limit MIMO multiplexing to a single stream?

Notation for This Chapter

Channel-model symbols. We reuse Φ,H1,H2,N\boldsymbol{\Phi}, \mathbf{H}_1, \mathbf{H}_2, N from Chapters 1–2 and introduce steering vectors, correlation matrices, and near-field coordinates.

SymbolMeaningIntroduced
aBS(θ)\mathbf{a}_{\text{BS}}(\theta)BS array steering vector at AoD θ\theta, CNt\in \mathbb{C}^{N_t}s02
aRIS(θ,ϕ)\mathbf{a}_{\text{RIS}}(\theta, \phi)RIS array steering vector at AoA/AoD (θ,ϕ)(\theta, \phi), CN\in \mathbb{C}^{N}s02
aUE(ϕ)\mathbf{a}_{\text{UE}}(\phi)UE array steering vector, CNr\in \mathbb{C}^{N_r} (scalar 1 for single-antenna UE)s02
KRiceK_{\text{Rice}}Ricean K-factor of the cascaded paths03
RRISCN×N\mathbf{R}_{\text{RIS}} \in \mathbb{C}^{N \times N}Spatial correlation matrix of the RIS elements in a rich-scattering fields03
dF=2D2/λd_F = 2D^2/\lambdaFraunhofer (far-field) distance for an aperture of dimension DDs04
DDLargest dimension of the RIS apertures04
Pt,σ2P_t, \sigma^2Transmit power and noise variance (carried over)s01