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Physics-Guided Bayesian Optimization for High-Dimensional Mixed-Variable MIMO Base Station Design

Koki Kanzaki et al. · arxiv_cs
arXiv CS · Papers
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This paper proposes a physics-guided Bayesian optimization for high-dimensional mixed-variable multiple-input and multiple-output (MIMO) base station (BS) design. The considered problem jointly selects a subset of candidate sites for BS deployment and optimizes the azimuth angles, downtilt angles, a
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Physics-Guided Bayesian Optimization for High-Dimensional Mixed-Variable MIMO Base Station Design Koki Kanzaki and Koya Sato

arXiv:2610.00974v1 [eess.SP] 1 Oct 2026

Artificial Intelligence eXploration Research Center, The University of Electro-Communications, Chofu, Tokyo, Japan Email: k-kanzaki@uec.ac.jp, k sato@ieee.org Abstract—This paper proposes a physics-guided Bayesian optimization for high-dimensional mixed-variable multiple-input and multiple-output (MIMO) base station (BS) design. The considered problem jointly selects a subset of candidate sites for BS deployment and optimizes the azimuth angles, downtilt angles, and transmit power spectral densities of the BSs, while each configuration is evaluated using computationally expensive site-specific ray tracing. To efficiently optimize the system configuration, the proposed method constructs a low-cost physics-based proxy from precomputed propagation information. The proxy-estimated communication coverage is used as the Gaussian process (GP) prior mean, and a residual GP with threedimensional physical features learns the discrepancy between the proxy and full evaluations. Ray-tracing-based evaluations in two urban scenarios show that the proposed method achieves up to approximately 15 percentage points higher coverage than conventional and high-dimensional optimization baselines under the same evaluation budget. Index Terms—Bayesian optimization, Gaussian process, base station configuration, ray tracing, MIMO

I. I NTRODUCTION Wireless infrastructure is increasingly deployed and configured for specific environments, as exemplified by private 5G [1] and enterprise Wi-Fi networks [2]. In parallel, detailed open three-dimensional environment models are becoming widely available, including Project PLATEAU in Japan1 and Helsinki 3D2 . Together with site-specific propagation simulators such as Sionna RT [3], these resources have made it increasingly feasible to predict wireless channels before physical deployment. These developments create an opportunity to design base-station (BS) infrastructure directly against the communication performance expected in the actual deployment environment, rather than relying primarily on simplified propagation models or coverage heuristics. Such site-specific design must jointly account for BS locations, antenna orientations, and transmit powers, because blockage, reflection, and diffraction from surrounding structures strongly affect communication performance. This problem has become more This work was supported by JST PRESTO under Grant Number JPMJPR23P3, CRONOS under Grant Number JPMJCS24N1, BOOST under Grant Number JPMJBS2415, and JSPS KAKENHI under Grant Number 25K00138. 1 https://www.mlit.go.jp/plateau/en/ 2 https://www.hel.fi/en/decision-making/information-on-helsinki/ maps-and-geospatial-data/helsinki-3d

important as modern wireless systems increasingly rely on multi-antenna transmission with channel-adaptive precoding and beamforming. Even when BSs operate independently without coordinated transmission, the communication performance of a deployment is governed by location-dependent spatial multiple-input multiple-output (MIMO) channels and the resulting inter-BS interference. Therefore, received power or static antenna patterns alone are insufficient to characterize the quality of a BS configuration. High-fidelity channel simulation, such as ray tracing over a three-dimensional environment model, provides a natural means of evaluating such configurations. However, repeatedly performing site-specific ray tracing over many receiver locations inside a joint placement-andconfiguration search is computationally expensive [4]. An efficient optimization method is therefore needed to identify effective BS configurations with only a limited number of raytracing evaluations. Bayesian optimization (BO) [5] is well suited to this setting and has been applied to BS placement optimization [6]. However, many existing studies on BS placement optimization assume that BSs can be deployed at arbitrary locations within a prescribed area. In practice, deployment constraints, such as the availability of suitable installation space, often prevent BSs from being placed at arbitrary locations, restricting deployment to a finite set of feasible candidate sites. The resulting BS design problem is a conditional mixed-variable optimization problem that combines discrete variables for selecting candidate sites for BS deployment with continuous parameters, such as transmit power and antenna orientation, that are relevant only to the BSs deployment at the selected candidate sites. Moreover, the dimensionality of the design problem increases with the number of candidate sites, making it difficult to handle these variables directly using a naive BO implementation. Methods for discrete optimization include BO of combinatorial structures [7] and combinatorial Bayesian optimization using the graph Cartesian product [8]. Trust region BO (TuRBO) [9] and random embedding BO (REMBO) [10] have also been proposed for high-dimensional optimization. Nevertheless, BO methods that efficiently handle high-dimensional optimization problems with conditional mixed variables, such as BS design, remain insufficiently explored. Further, modern wireless systems commonly employ multi-

antenna transmission with channel-adaptive precoding and beamforming. Hence, the performance of a BS deployment depends not only on received power or static antenna patterns, but also on user-dependent spatial MIMO channels, the resulting precoders, and inter-cell interference. This aspect is particularly important for BS design because the effective transmission pattern varies dynamically with the user location and channel state. Nevertheless, existing BS placement formulations often rely on received-power metrics or single-stream directional transmission and do not explicitly account for channel-adaptive MIMO operation. Therefore, BS placement and configuration should be evaluated based on the communication performance achievable over the spatial MIMO channels after precoding and interference mitigation. To address these challenges, we propose a physics-guided BO for high-dimensional mixed-variable MIMO BS design. The proposed method jointly optimizes the BS placements and their parameters; the azimuth angles, downtilt angles, and transmission powers. The objective is to maximize coverage, defined as the fraction of target-area locations achieving a prescribed spectral efficiency, with each full evaluation based on MIMO channels obtained through site-specific ray tracing. To efficiently search the system configuration under a limited full-evaluation budget, we construct a low-cost physics-based proxy using propagation information precomputed for the candidate sites and a discrete set of antenna orientations. The proxy-estimated coverage is used as the prior mean of a Gaussian process (GP), while low-dimensional physical features derived from the proxy characterize the communication conditions of each configuration. A residual GP then learns the discrepancy between the proxy and full evaluations in this physical feature space, thereby guiding the selection of subsequent configurations for expensive full evaluation. II. S YSTEM M ODEL Fig. 1 summarizes the system model. We consider a wireless system where multiple MIMO BSs operating on a shared frequency band3 are deployed in an area A ⊂ R3 . Our goal is to optimize BS placements and their parameters to maximize communication area. Possible applications of our discussion include cellular systems, private 5G, and public Wi-Fi. A. Signal Model Let C = {1, . . . , N } denote the set of candidate-site indices and si ∈ R3 the location of candidate site i. We refer to the BS deployed at candidate site i as the i-th BS. A system configuration is specified by a set x ≜ {Cx , {ψ i }i∈Cx }, where Cx ⊆ C is the set of selected candidate-site indices and ψ i = [αi , βi , pi ]⊤ is the continuous parameter vector of the i-th BS. Here, αi [rad], βi [rad], and pi [W/Hz] denote the azimuth angle, the downtilt angle measured from the horizontal plane, and the total transmit power spectral density (PSD) across 3 Owing to the orthogonality among frequency channels, the proposed method can be extended to multi-channel systems by exploiting an additive decomposition of the objective function [11]. Since this extension is straightforward, this paper focuses on system design over a shared frequency band.

・ antennas ・Design variable:

Candidate for BS placement Evaluation point

Fig. 1. System model.

all transmit antennas, respectively. We evaluate the downlink spectral efficiency independently at Neval receiver locations eval {ru }N u=1 ⊂ A. These locations are evaluation points rather than simultaneously active users. All selected BSs are assumed active; the serving BS transmits the signal to the receiver under evaluation, while the others generate inter-BS interference. Resource sharing and inter-user scheduling are not modeled. For simplicity, quantities associated with the u-th receiver location are indexed by u. The channel matrix between the i-th BS and the u-th receiver location at fc is denoted by Hu,i (x) ∈ CNr ×Nt , where Nt and Nr are the numbers of transmit and receive antenna, respectively, including polarization ports. Each BS employs a digital MIMO architecture with an independent radio-frequency chain for each transmit antenna. BSs operate independently, without coordinated transmission or joint precoding. Perfect instantaneous channel state information (CSI) for the link between a receiver and its serving BS is assumed to be available at both ends and is used to precode the desired signal. For a receiver at the u-th location served by the i-th BS, the singular value decomposition (SVD) of the channel matrix is H Hu,i (x) = Uu,i (x)Σu,i (x)Vu,i (x).

(1)

Here, Uu,i (x) ∈ CNr ×Nr and Vu,i (x) ∈ CNt ×Nt are unitary Nr ×Nt matrices, while Σu,i (x) ∈ R≥0 contains the singular values in nonincreasing order on its main diagonal. The superscript (·)H denotes the conjugate transpose. The number of spatial streams, Ns , is fixed and satisfies 1 ≤ Ns ≤ (N ) min(Nt , Nr ). We denote by Vu,is (x) ∈ CNt ×Ns the matrix formed by the first Ns columns of Vu,i (x), which correspond to the Ns largest singular values. The i-th BS allocates its total transmit PSD pi equally among the Ns streams. The transmit covariance density matrix of the desired signal is then  H pi (Ns ) (N ) Vu,i (x) Vu,is (x) . (2) Qsig u,i (x) = Ns The corresponding desired-signal covariance density matrix at the receiver is H Su,i (x) = Hu,i (x)Qsig u,i (x)Hu,i (x).

(3)

Next, we consider interference from non-serving BSs. For non-serving BSs, we assume isotropically distributed beam directions independent of the channel to the receiver under evaluation. Since E[Wj WjH ] = (Ns /Nt )INt , the interferenceplus-noise covariance for the u-th receiver served by BS i is X pj Ωu|i (x) = Hu,j (x)HH (4) u,j (x) + N0 INr . Nt j∈Cx j̸=i

Main Loop for Bayesian Optimization Candidate Selection

Residual GP Ray tracing and Proxy

RT and Proxy Fit

Ray tracing result Proxy

GPR mean GPR variance

Features

Selection:

Approximate Coverage Map

Assuming independent complex Gaussian signals for the desired streams and treating interference as Gaussian noise with the covariance density specified above, the spectral efficiency of the link from the i-th BS to the u-th receiver location in bps/Hz is   ηu,i (x) = log2 det INr + Ω−1 (5) u|i (x)Su,i (x) .

Proxy Estimate

Ray Tracing Evaluation

Feature Extraction Coverage

BS dominance

Spatial variation 50%

Median SE

Propagation database Precomputation of The Propagation Database

After T loops Optimization Result

Path Gain:

The receiver at the u-th location is associated with the BS at the selected candidate site that provides the highest reference received PSD. We define the reference received PSD metric for the link from the i-th BS to the u-th receiver location as  pi tr Hu,i (x)HH (6) ρu,i (x) ≜ u,i (x) , Nt where tr(·) denotes the matrix trace. The serving BS index i∗u (x) is then selected as i∗u (x) ∈ arg max ρu,i (x).

(7)

i∈Cx

The spectral efficiency at the u-th receiver location is therefore Ru (x) = ηu,i∗u (x) (x). B. Problem Setting We define coverage as the fraction of the Neval receiver locations satisfying the required spectral efficiency Rreq > 0. Specifically, the objective function is given by f (x) ≜

1

N eval X

Neval u=1

1 [Ru (x) ≥ Rreq ] ,

(8)

where 1[·] is the indicator function that outputs 1 if the condition in brackets holds and 0 otherwise. Finally, the optimization problem is formulated as maximize

f (x)

subject to

Cx ⊆ C,

x

|Cx | = M,

0 ≤ αi < 2π,

i ∈ Cx ,

βmin ≤ βi ≤ βmax ,

i ∈ Cx ,

pmin ≤ pi ≤ pmax ,

i ∈ Cx ,

(9)

where 1 ≤ M ≤ N . The constants βmin and βmax bound the downtilt angle, while constants pmin and pmax bound the transmit PSD. We denote the set of configurations satisfying these constraints by X . Because radio propagation is strongly affected by surrounding buildings, evaluating f (x) requires high-fidelity channel simulation for each configuration x. Moreover, since x contains both discrete and continuous variables, the problem in Eq. (9) is a conditional mixed-variable

Optimized parameters: • BS locations • Antenna orientations • Downtilt angles

Fig. 2. Overview of the proposed method.

black-box optimization problem that combines discrete site selection with continuous parameters defined only for the BSs deployed at the selected candidate sites. III. P HYSICS -G UIDED BAYESIAN O PTIMIZATION Since evaluating f (x) requires costly site-specific ray tracing, we employ BO with a physics-guided surrogate. A GP directly defined over the variables in Eq. (9) is problematic because its dimension grows with the number of candidate sites and geometric proximity does not necessarily imply similar propagation conditions. We therefore construct a lowcost physics-based proxy and use its low-dimensional physical features as GP inputs, as summarized in Fig. 2. A. Construction of the Physics-Based Proxy To avoid ray tracing for every candidate configuration, we precompute propagation information for the candidate sites, representative antenna orientations, and a reduced set of proxy receiver points before optimization begins. We precompute propagation information for representative antenna orientations and Np < Neval proxy receiver points {rpu }u∈Up ⊂ A, where Up = {1, . . . , Np }. The antenna azimuth and downtilt angles are discretized into the sets Dα ≜ {α1 , α2 , · · · , αNα }, Dβ ≜ {β 1 , β 2 , · · · , β Nβ }, (10) where Nα and Nβ are the numbers of representative azimuth Nr ×Nt and downtilt angles, respectively. Let Hpre u,i,a,b ∈ C denote the MIMO channel at fc between proxy u-th receiver point and a BS at i-th candidate site with azimuth αa and downtilt β b . These channel matrices are computed once by ray tracing before optimization begins. For each channel matrix, we compute the normalized Gram matrix 1 pre  pre H Gpre ≜ H Hu,i,a,b . (11) u,i,a,b Nt u,i,a,b

We refer to the collection of these precomputed Gram matrices over all candidate sites, representative antenna orientations, and proxy receiver points as the propagation database. Because the angles αi and βi in a configuration x are continuous, the Gram matrix for an arbitrary antenna orientation is approximated by interpolating the neighboring matrices in the propagation database: we define this operation as n o  G̃u,i (x) ≜ I Gpre ; α , β (12) i i , u,i,a,b where I denotes bilinear interpolation over neighboring azimuth and downtilt grid points, with the azimuth treated as periodic at 0 and 2π. The interpolated matrix is a weighted sum of Gram matrices with nonnegative weights that sum to 1, preserving their Hermitian positive semidefinite property. We use the approximate Gram matrices to compute approximate spectral efficiency under the communication model in Sec. II. Let λ̃u,i,ℓ (x) denote the eigenvalues of G̃u,i (x) in descending order and ũu,i,ℓ (x) the corresponding unitnorm eigenvectors. Accounting for the normalization by 1/Nt in Eq. (11), the approximate desired-signal and interference covariance density matrices are, respectively, N

s pi Nt X λ̃u,i,ℓ (x)ũu,i,ℓ (x)ũH S̃u,i (x) = u,i,ℓ (x), Ns

(13)

ℓ=1

J̃u←j (x) = pj G̃u,j (x).

(14)

Using the approximated Gram matrix, the reference   received PSD metric is approximated as ρ̃u,i (x) = pi tr G̃u,i (x) . The BS with the largest value of this metric is selected as the serving BS. The above covariance density matrices are then used to compute the approximate spectral efficiency R̃u (x). The proxy estimate of the objective is defined as Np i 1 X h ˜ fphys (x) ≜ 1 R̃u (x) ≥ Rreq . Np u=1

(15)

The proxy requires no additional ray tracing for each configuration, but antenna-orientation interpolation and receiver-point subsampling introduce a discrepancy from the full objective f (x). We therefore use the proxy as a baseline and write the surrogate as g(x) ≜ f˜phys (x) + r(z(x)),

(16)

with f (x) ≈ g(x), where z(x) is defined in Sec. III-B and the residual function r(·) is learned by Gaussian process regression (GPR) [12] in Sec. III-C. B. Physical Feature The residual term in Eq. (16) should reflect similarity in communication conditions rather than in raw configuration parameters. A direct representation is 4N -dimensional, includes continuous parameters of unselected candidate sites, and may poorly reflect propagation similarity because of blockage and reflection. We therefore derive low-dimensional physical features from the proxy outputs. In addition to approximate coverage, the proxy provides spatial distributions of spectral

efficiency and reference received PSD. Their local variations are relevant to receiver-grid subsampling near the spectralefficiency threshold and BS-association changes caused by orientation interpolation when competing BSs have similar received PSDs. We characterize these variations together with a representative spectral-efficiency level. To quantify spatial variation, we construct an undirected graph Gp = (Vp , Ep ) over the proxy receiver grid, where Vp = Up and Ep connects horizontally or vertically adjacent receiver points, with Ep ̸= ∅. For scalar values q = [q1 , q2 , . . . , qNp ]⊤ defined on the receiver points, we define the graph energy as X 1 (qu − qv )2 . (17) EGp (q) = |Ep | (u,v)∈Ep

We define a smooth measure of spectral efficiency satisfaction, cu (x), and a measure of serving-base-station dominance, du (x), as ! R̃u (x) − Rreq , (18) cu (x) ≜ sigmoid τ du (x) ≜

ρ̃u,(1) (x) − ρ̃u,(2) (x) , ρ̃u,(1) (x) + Nr N0

(19)

where sigmoid(a) = (1 + e−a )−1 and τ > 0 is a smoothing parameter with the same units as spectral efficiency. Smaller values of τ yield a sharper transition in cu near the threshold. The quantities ρ̃u,(1) and ρ̃u,(2) are the largest and secondlargest reference received PSD metrics among the BSs deployed at the selected candidate sites. The term Nr N0 is the total noise PSD across all receive antenna. The metric du is small when the two strongest BSs provide similar received PSDs and large when the strongest BS dominates both the others and the noise. Defining c(x) = [cu (x)]u∈Up and d(x) = [du (x)]u∈Up , we construct the physical feature vector h(x) ∈ R3 as " !#⊤ R̃u (x) h(x) = EGp (c(x)), EGp (d(x)), median , u∈Up Rreq (20) where median(·) denotes the median. The first feature measures local variation in spectral efficiency satisfaction, and the second measures local variation in serving-base-station dominance. The third expresses the representative spectral efficiency in the target area relative to the required spectral efficiency. Because the features have different scales, we evaluate a set of feasible configurations using only the proxy and compute the mean and standard deviation of each feature component. These configurations are generated independently of the initial optimization samples. Using these statistics, we standardize the feature vector: this operation is defined as z(x) ≜ Standardize(h(x)). The standardized vector is used as the GPR input. The standardization statistics are fixed before BO begins and are computed without full objective evaluations. Because the features depend only on communication conditions produced by the BSs deployed at the

selected candidate sites, they are independent of the continuous parameters associated with unselected candidate sites. The GPR input dimension is always 3, regardless of the number of candidate sites or deployed BSs. C. Sequential Search Using a Residual GP Let Tt = {(xj , yj )}tj=1 denote the observations obtained from t full evaluations. The surrogate model assumes inde2 pendent observation noise ϵj ∼ N (0, σobs ), so that yj = f (xj ) + ϵj . Following the decomposition in Eq. (16), the GPR model is applied only to the discrepancy between the full evaluation and the physics-based proxy. For observation yj , the residual is defined as rj ≜ yj − f˜phys (xj ). We introduce a latent function r : R3 → R to model this residual in the physical feature space. Before each GP fit, we compute the empirical mean r̄t of the observed residuals and a positive scale st from their empirical standard deviation. Unlike the fixed input-feature normalization, these target statistics are updated whenever the GP is refit. We define the standardized latent residual as r̂t (z) = (r(z) − r̄t )/st and and model it as r̂t (z) ∼ GP(0, k(z, z′ )). The kernel hyperparameters 2 /s2t are and the standardized observation-noise variance σobs learned jointly whenever the GP is refit. In standardized residual units, the covariance between configurations x and x′ is k(z(x), z(x′ )). Let Ttr = {(z(xj ), rj )}tj=1 denote the residual observations. Conditioning the GP on the centered and scaled residual observations yields a posterior in standardized units. We restore its mean by multiplying by st and adding r̄t , and its variance by multiplying by s2t , obtaining the residual posterior mean µrt (z) and variance (σtr (z))2 on the original coverage scale. Since the proxy value is deterministic for a given configuration, the predictive mean and variance of the full latent objective are µphys (x) = f˜phys (x) + µrt (z(x)), t (σtphys (x))2 = (σtr (z(x)))2 .

(21) (22)

Thus, f˜phys (x) acts as the physics-based prior mean, while the residual GP provides the correction and its uncertainty. As the acquisition function,  we use expected improvement  (EI) defined as EIt (x) = E max(g(x) − ft+ , 0) | Tt , where ft+ = maxj≤t yj is the best observation value. The expectation is taken under the Gaussian predictive distribution with the mean and variance given in Eqs. (21) and (22), respectively. This formulation compares configurations with high proxypredicted coverage and configurations that are promising after accounting for residual corrections and uncertainty on the same objective scale. To maximize the acquisition function, we generate a finite candidate set Pt of unevaluated configurations in the original feasible set X . In addition to random configurations drawn from the full search space, we generate candidates from configurations with high observed objective values in two ways: replacing one selected selected candidate site with another candidate site, or keeping the selected candidate sites

(a)

(b)

(c)

(d)

Fig. 3. Best observed coverage in Munich and Etoile versus (a), (c) elapsed time and (b), (d) number of ray tracing evaluations.

fixed and modifying the continuous parameters of the BSs deployed at those sites. All candidates satisfy the prescribed BS count and parameter bounds; duplicate and previously evaluated configurations are removed. We compute the proxy values, physical features, and EI for this candidate set and select the next configuration as xt+1 ∈ arg max EIt (x).

(23)

x∈Pt

Dimension reduction is applied only to the GPR input through z(x); candidate configurations are generated and selected in the original feasible set X . After evaluating Ninit randomly selected initial configurations, we alternate GP updates and configuration selection until the evaluation budget is exhausted. The budget T counts full configuration evaluations, including the initial observations, with 1 ≤ Ninit ≤ T . Proxy and acquisition-function evaluations, as well as propagationdatabase precomputation, are excluded from this count. IV. P ERFORMANCE E VALUATION We consider the Munich and Etoile urban scenes provided by Sionna RT [3]. We randomly place N = 100 candidate sites 5 m above the rooftops and select M = 5 of these sites for BS deployment. The search ranges are [0, 2π) for azimuth, [0, π/3] for downtilt, and [−80, −60] dBm/Hz for total transmit PSD. Each transmitter uses an 8 × 4 array, and each receiver uses a 1 × 2 array. Both arrays use crossed polarization, half-wavelength element spacing, and directional elements following 3GPP TR 38.901 [13], giving Nt = 64 and Nr = 4 antenna. The number of spatial streams is fixed at Ns = 2. The carrier center frequency is fc = 3.5 GHz. Further, we set N0 = 4.00 × 10−21 W/Hz (290 K, 0-dB noise figure). For each full evaluation, we use a 100 × 100 receiver

(a)

(b)

(c)

(d)

(e)

(f)

Fig. 4. Optimization example in Munich: (a) Proposed (fine), (b) Random, (c) GA, (d) GP BO, (e) TuRBO, and (f) REMBO.

grid (Neval = 104 ) with 5 m spacing over a 500 × 500 m2 area. Both the full-evaluation and proxy receiver grids are at a height of 1.5 m. We set the required spectral efficiency to Rreq = 1 bps/Hz, the initial sample size to Ninit = 5, and the evaluation budget to T = 100, including the initial evaluations. We compare three discretization levels for the proxy propagation database. The fine setting uses azimuth and downtilt steps of 45◦ and 5◦ , respectively, and 25 m receiver spacing (Nα = 8, Nβ = 13, Np = 400). The medium setting uses 90◦ and 10◦ angular steps and 50 m receiver spacing (Nα = 4, Nβ = 7, Np = 100). The coarse setting uses 180◦ and 20◦ angular steps and 100 m receiver spacing (Nα = 2, Nβ = 4, Np = 25). The azimuth grids start at 0 and exclude 2π, while the downtilt grids include both 0 and π/3. All three settings share the same ray-tracing propagation settings and full-evaluation grid. For the physical features, we set τ = 0.1 bps/Hz and fix the input standardization statistics using 2048 independently generated feasible configurations evaluated only by the proxy. The baselines are random search (Random), a genetic algorithm (GA) [14], a naive GP-based BO implementation (GP BO) using a 4N = 400-dimensional configuration representation, and the high-dimensional BO methods TuRBO [9] and REMBO [10]. We also include Physics BO, which uses the same three-dimensional physical features, GP, and search procedure as the proposed method but sets the prior mean to zero and learns the objective directly. Physics BO uses the medium discretization in the figures, allowing comparison with Proposed (medium) to isolate the effect of the physical prior mean. The proposed method and Physics BO use a Matérn 3/2 kernel with automatic relevance determination (ARD). The GP targets are residuals for the proposed method and objective values for Physics BO; both are centered and scaled anew at each refit. On the standardized target scale, the observation-noise variance is initialized to 10−3 and learned within [10−4 , 10−1 ]. Fig. 3 shows convergence performances in Munich ((a)(b)) and Etoile ((c)(d)). Af-

ter 100 evaluations, Proposed (fine/medium/coarse) achieves 87.6/86.2/83.0% coverage in Munich and 96.0/95.2/93.2% in Etoile. Physics BO achieves 85.5% and 93.9%, while TuRBO, the strongest remaining baseline, achieves 72.4% and 89.6%, respectively. Thus, Proposed (fine) improves over TuRBO by 15.2 and 6.4 percentage points, while using the physical prior mean improves the medium setting over Physics BO by 0.8 and 1.3 points. At 300 s, medium reaches 78.4% coverage in Munich and 93.1% in Etoile. fine provides the best performance for a fixed evaluation budget but incurs a larger precomputation cost, whereas medium provides a favorable balance between the two. These results show the tradeoff between evaluation efficiency and precomputation cost when choosing the proxy discretization. V. C ONCLUSION This paper proposed an efficient BO framework for MIMO BS design problem. The method uses a physics-based proxy to provide both the prior mean and a three-dimensional feature representation. A residual GP corrects the propagation-based approximation, improving the fraction of receiver locations that meet the spectral efficiency requirement within a limited budget of full evaluations. R EFERENCES [1] M. Wen et al., “Private 5G Networks: Concepts, Architectures, and Research Landscape,” IEEE J. Sel. Topics Signal Process., vol. 16, no. 1, pp. 7–25, Jan. 2022. [2] G. Geraci et al., “Wi-Fi: 25 Years and Counting,” Proc. IEEE, vol. 113, no. 11, pp. 1290–1336, Jan. 2025. [3] J. Hoydis et al., “Sionna,” 2022. [4] M. Vasudevan and M. Yuksel, “Machine Learning for Radio Propagation Modeling: A Comprehensive Survey,” IEEE Open J. Commun. Soc., vol. 5, pp. 5123–5153, 2024. [5] J. Snoek et al., “Practical Bayesian Optimization of Machine Learning Algorithms,” in Adv. Neural Inf. Process. Syst., vol. 25. Curran Associates, Inc., 2012. [6] K. Sato and K. Suto, “Bayesian Optimization Framework for Channel Simulation-Based Base Station Placement and Transmission Power Design,” IEEE Netw. Lett., vol. 6, no. 4, pp. 217–221, Feb. 2024. [7] R. Baptista and M. Poloczek, “Bayesian Optimization of Combinatorial Structures,” in Proc. 35th Int. Conf. Mach. Learn. PMLR, Jul. 2018, pp. 462–471. [8] C. Oh et al., “Combinatorial Bayesian Optimization using the Graph Cartesian Product,” in Adv. Neural Inf. Process. Syst., vol. 32. Curran Associates, Inc., 2019. [9] D. Eriksson et al., “Scalable Global Optimization via Local Bayesian Optimization,” in Adv. Neural Inf. Process. Syst., vol. 32. Curran Associates, Inc., 2019. [10] Z. Wang et al., “Bayesian Optimization in a Billion Dimensions via Random Embeddings,” J. Artif. Intell. Res., vol. 55, pp. 361–387, Feb. 2016. [11] M. Binois and N. Wycoff, “A survey on high-dimensional Gaussian process modeling with application to Bayesian optimization,” ACM Trans. Evol. Learn. Optim., vol. 2, no. 2, pp. 8:1–8:26, Aug. 2022. [12] C. E. Rasmussen and C. K. I. Williams, Gaussian Processes for Machine Learning. Cambridge, Mass.: The MIT Press, 2008. [13] 3rd Generation Partnership Project (3GPP), “Study on channel model for frequencies from 0.5 to 100 GHz,” 3rd Generation Partnership Project (3GPP), Technical Report TR 38.901, Sep. 2026. [14] D. E. Goldberg, Genetic Algorithms in Search, Optimization and Machine Learning, 1st ed. USA: Addison-Wesley Longman Publishing Co., Inc., 1989.

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