---
title: Quantum Radar Cross Section
url: https://www.emergentmind.com/topics/quantum-radar-cross-section-qrcs
type: topic
---

# Quantum Radar Cross Section

Searching arXiv for the specified papers and closely related QRCS work.
arXiv search: "Quantum Radar Cross Section"
Quantum radar cross section (QRCS) denotes a family of quantum formulations of electromagnetic target scattering rather than a single universally accepted object. In one line of work, QRCS is a **computational** problem: the classical frequency-domain finite-element (FD-FEM) radar cross section calculation is embedded into a quantum linear-systems pipeline, notably the Clader–Jacobs–Sprouse (CJS) algorithm, with the aim of obtaining an end-to-end exponential speedup in the problem dimension $N$ [2602.20553]. In another line of work, QRCS is a **quantum-optical scattering observable**: field amplitudes are promoted to operators, and cross sections are defined through one-photon or two-photon scattering amplitudes, coincidence channels, and second-order correlations [2205.14000], or through intensity-operator expectation values for single-photon and biphoton incident states [2606.05603]. A third strand of the literature argues that no physically distinct “quantum radar cross section” larger than the classical radar cross section $\sigma$ appears in a full quantum treatment of far-field scattering, so that quantum radar proposals still inherit the same $\sigma$ entering the classical radar equation [2403.00047].

## 1. Terminological scope and definitional landscape

In the literature considered here, QRCS is used in two distinct senses. The distinction is substantive because the corresponding mathematical objects, performance claims, and feasibility questions are different.

| Usage | Core object | Representative source |
|---|---|---|
| Quantum-computational QRCS | Quantum algorithm for solving $A x=b$ arising from FD-FEM Maxwell/Helmholtz discretization and extracting RCS | [2602.20553] |
| Quantum-optical QRCS | Cross section defined from operator expectation values, scattering amplitudes, or coincidence rates for one- or two-photon states | [2205.14000], [2606.05603] |

The classical benchmark is the usual radar cross section,
$$
\sigma(\Omega)=\lim_{r\to\infty}4\pi r^2\frac{|E_s(r,\Omega)|^2}{|E_i|^2},
$$
or, equivalently in the far field, Jackson’s formula
$$
\sigma(\hat k,\epsilon,k_0,\epsilon_0)=\lim_{r\to\infty}4\pi r^2\frac{|\epsilon^*\!\cdot E_s(r\hat k)|^2}{|\epsilon_0\!\cdot E_0|^2}.
$$
The computational QRCS program retains this classical scattering quantity but seeks to accelerate its evaluation by quantum means; the quantum-optical program instead reformulates the scattering observable itself in terms of states, operators, and correlations [2602.20553], [2205.14000].

A central controversy follows immediately. “On Target Detection by Quantum Radar (Preprint)” states that **no new, larger cross section appears** in a full quantum treatment and that all classical and quantum radar link-budget formulas hold with the identical $\sigma$ [2403.00047]. By contrast, “Quantum Radar Cross Section with two-photon entangled states” defines single-photon and biphoton QRCS formulas and reports enhancements relative to single-photon and separable two-photon QRCS in angular scattering patterns for signal–signal entangled probes [2606.05603]. This suggests that part of the disagreement is terminological: one literature addresses link-budget invariance of the far-field scattering strength, whereas another studies quantum-state-dependent angular distributions and detection observables.

## 2. Operator-based and scattering-amplitude formulations

In the quantum-optical treatment, the one-photon scattering operator $\hat S$ and two-photon operator $T$ act on an input state $|\psi_{\rm in}\rangle$, and the outgoing-state detection probability defines the QRCS. For a two-photon entangled probe, the differential QRCS in the coincidence channel $(\Omega_1,\Omega_2)$ is written as
$$
\sigma_Q(\Omega_1,\Omega_2)\equiv
\frac{\langle\psi_{\rm in}|\,\hat S^\dagger(\Omega_1,\Omega_2)\,\hat S(\Omega_1,\Omega_2)\,|\psi_{\rm in}\rangle}{\Phi_{\rm in}},
$$
where $\Phi_{\rm in}$ is the two-photon incident flux. Under the Born approximation, this reduces to
$$
\sigma_Q(\Omega_1,\Omega_2)=\frac{|\langle \Omega_1,\Omega_2|T|\psi_{\rm in}\rangle|^2}{\Phi_{\rm in}},
$$
with two-photon scattering amplitude
$$
f_Q(\Omega_1,\Omega_2)=\langle \Omega_1,\Omega_2|\,\hat T\,|\,\psi_{\rm in}\rangle.
$$
The second-order correlation function is
$$
G^{(2)}(\Omega_1,\Omega_2)
=\langle E^{(-)}(\Omega_1)\,E^{(-)}(\Omega_2)\,E^{(+)}(\Omega_2)\,E^{(+)}(\Omega_1)\rangle
\propto |f_Q(\Omega_1,\Omega_2)|^2,
$$
and the integrated monostatic QRCS is obtained by integrating over one solid angle [2205.14000].

The same source states that in the single-photon limit the quantum definition reduces to the classical RCS:
$$
\sigma_{\rm cl}(\Omega)
=\frac{|\langle \Omega|\hat T|1_{\rm in}\rangle|^2}{\Phi_{\rm single}}
=\lim_{\psi_{\rm in}\to\text{one-photon plane wave}}\sigma_Q(\Omega).
$$
The assumptions are explicit: Born (first-order) scattering, far-field (Fraunhofer) regime, stationary target, traveling-wave signal and idler modes, and narrowband (quasi-monochromatic) envelopes. The biphoton source is modeled as
$$
|\psi_{\rm in}\rangle = \int d\omega_s\, d\omega_i\, \phi(\omega_s,\omega_i)\, a_s^\dagger(\omega_s)\, a_i^\dagger(\omega_i)\,|0\rangle.
$$

A different but related quantum-optical formulation defines single-photon QRCS by analogy with classical RCS through intensity operators:
$$
\sigma_Q
=\lim_{R\to\infty}4\pi R^2\frac{\langle \hat I_s(r,t)\rangle}{\langle \hat I_i(r,t)\rangle}.
$$
Under the Weisskopf–Wigner scattering model for $N$ identical, randomly oriented point-scatterers at positions $\{x_n\}$, the scattered intensity satisfies
$$
\langle \hat I_s\rangle\propto \left|\sum_{n=1}^N e^{i(\mathbf{k}_i-\mathbf{k}_s)\cdot x_n}\right|^2,
$$
leading to
$$
\sigma_Q^{(1)}
=
\frac{4\pi\,A_\perp(\theta_i,\phi_i)\,
\left|\sum_{n=1}^N e^{i(\mathbf{k}_i-\mathbf{k}_s)\cdot x_n}\right|^2}
{\int_0^{2\pi}\!\!\int_0^{\pi/2}
\left|\sum_{n=1}^N e^{i(\mathbf{k}_i-\mathbf{k}_s)\cdot x_n}\right|^2
\sin\theta_s\,d\theta_s\,d\phi_s},
$$
where $A_\perp(\theta_i,\phi_i)$ is the projected area of the target for illumination direction $(\theta_i,\phi_i)$ [2606.05603].

## 3. Multiphoton extensions and the role of entanglement

For a product state of $M$ identical single-photon wavepackets, each photon scatters independently, and the separable extension is
$$
\sigma_Q^{(M,\text{sep})}
=
\frac{4\pi\,A_\perp\,
\left|\sum_n e^{i\Delta k\cdot x_n}\right|^{2M}}
{\int_0^{2\pi}\!\!\int_0^{\pi/2}
\left|\sum_n e^{i\Delta k\cdot x_n}\right|^{2M}
\sin\theta_s\,d\theta_s\,d\phi_s},
\qquad
\Delta k=\mathbf{k}_i-\mathbf{k}_s.
$$
The stated conclusion is that there is **no quantum-entanglement-induced enhancement beyond the classical scaling** $\propto |F(\Delta k)|^{2M}$ for this separable case [2606.05603].

The entanglement structure matters. “Quantum Radar Cross Section with two-photon entangled states” reports that signal-idler entanglement does not improve the unconditional QRCS and therefore focuses on signal–signal entanglement, where both photons scatter from the target [2606.05603]. For the maximally entangled case, the incident joint amplitude is
$$
\mathcal{A}_i(\hat k_1,\hat k_2)=\delta(\hat k_1-\hat k_2).
$$
The scattered two-photon amplitude is
$$
\mathcal{A}_s(\hat k,\hat k')
=
\int d\hat k_1\,d\hat k_2\;
\langle k|T|k_1\rangle\,
\langle k'|T|k_2\rangle\,
\mathcal{A}_i(\hat k_1,\hat k_2),
$$
with single-photon $T$-matrix
$$
\langle k|T|k_1\rangle
=
\sum_{a,b} t_{ab}(k)\,e^{\,i(\mathbf{k}\cdot r_a-\mathbf{k}_1\cdot r_b)}.
$$
Evaluating the integrals yields
$$
\mathcal{A}_s(\hat k,\hat k')
=
4\pi
\sum_{a,b,a',b'}
t_{ab}(k)\,t_{a'b'}(k')
e^{\,i\bigl(k\hat k\cdot r_a+k'\hat k'\cdot r_{a'}\bigr)}
\,\mathrm{sinc}\bigl(|kr_b+k'r_{b'}|\bigr),
$$
and the corresponding biphoton QRCS is
$$
\sigma_Q^{(2,\max)}
=
\frac{4\pi\,A_\perp\;
\bigl|\sum_{a,b,a',b'}t_{ab}t_{a'b'}
e^{i(k\hat k\cdot r_a+k'\hat k'\cdot r_{a'})}
\mathrm{sinc}(|kr_b+k'r_{b'}|)\bigr|^2}
{\int_0^{2\pi}\!\!\int_0^{\pi/2}\bigl|\dots\bigr|^2\sin\theta_s\,d\theta_s\,d\phi_s}.
$$

To interpolate between separable and strongly entangled states, the same work uses the double-Gaussian approximation
$$
\mathcal{A}_i(\hat k_1,\hat k_2)
=
N_s\,
\exp\!\Bigl[-\frac{(\hat k_{1\perp}+\hat k_{2\perp})^2}{\sigma^2}\Bigr]\,
\exp\!\Bigl[-\frac{(\hat k_{1\perp}-\hat k_{2\perp})^2}{\mu^2}\Bigr],
$$
with Schmidt number
$$
K=\frac{\sigma^2+\mu^2}{2\,\sigma\,\mu},
$$
where $K=1$ is separable and $K\gg 1$ is strongly entangled. The resulting QRCS contains an entanglement-dependent overlap integral $I(k,k';r_b,r_{b'})$ expressed through angular integrals and Bessel functions $J_m$ and $I_m$ [2606.05603].

The same paper reports concrete pattern-level effects. For square, circular, and triangular 2D atom arrays of side or diameter $L=4\lambda$ (and also $L=1\,\mathrm m$), sampled by $961$, $709$, and $462$ atoms respectively, the monostatic entangled two-photon QRCS shows **enhanced side-lobes** around $\theta\approx\pm0.5\,\mathrm{rad}$ and a **suppressed main-lobe** at $\theta=0$; the side-lobe enhancement is strongest for smaller targets such as the circle and triangle. In bistatic plots at $\theta_i=85^\circ$, the single-photon and separable two-photon lobes follow the illumination direction, whereas the maximally entangled QRCS remains anchored. For partially entangled states, truncating the infinite $m$-sum at $m=20$, the paper states that states with $K\sim 2$–$5$ can outperform the maximal case by up to $\sim 14.7\%$ in the side-lobe region [2606.05603].

## 4. Shape form factors, monostatic and bistatic geometry, and correlation-based advantages

In the far field, the discrete sum over scatterers may be replaced by the surface integral
$$
F(\Delta k)=\int_S e^{\,i\Delta k\cdot r}\,dS(r),
$$
so that the single-photon QRCS becomes
$$
\sigma_Q^{(1)}
=\frac{4\pi\,A_\perp\,|F(\Delta k)|^2}
{\int |F(\Delta k)|^2\sin\theta_s\,d\theta_s\,d\phi_s}.
$$
Closed-form monostatic form factors are given for several target classes:
- rectangular plate of sides $L_x,L_y$:
  $$
  F(\Delta k)=L_xL_y\,\mathrm{sinc}\!\left(\frac{\Delta k_xL_x}{2}\right)\,
  \mathrm{sinc}\!\left(\frac{\Delta k_yL_y}{2}\right),
  $$
- circular disk of radius $a$:
  $$
  F(\Delta k)=\pi a^2\,\frac{2J_1(|\Delta k|a)}{|\Delta k|a},
  $$
- spherical shell of radius $a$:
  $$
  F(\Delta k)=4\pi a^2\,\frac{\sin(|\Delta k|a)}{|\Delta k|a},
  $$
- triangular plate, expressible via Dirichlet kernels or decomposition into parallelogram form factors [2606.05603].

For monostatic backscatter, the paper writes
$$
\sigma_{\rm mono}^{(1)}
=
\frac{4\pi\,A_\perp\,|F(0)|^2}
{\int |F(\Delta k(\theta_s,\phi_s))|^2\sin\theta_s\,d\theta_s\,d\phi_s},
$$
and for bistatic operation one studies $\sigma_Q(\theta_s,\phi_s)$ at fixed $(\theta_i,\phi_i)$ [2606.05603].

A different quantum-optical literature emphasizes measurement-theoretic gains rather than target-form-factor reshaping. It states that entanglement enhances QRCS in two principal ways: **signal-to-noise ratio (SNR) improvement** and **resolution (phase-sensitivity) gain**. The stated scaling comparison is classical Poisson-limited SNR $\sim \sqrt N$ versus entangled-pair coincidence detection approaching the Heisenberg limit $\sim N$, because the joint detection $G^{(2)}$ suppresses uncorrelated background. Likewise, classical interferometric phase resolution $\Delta\phi_{\rm cl}\simeq 1/\sqrt N$ is contrasted with entangled $N$-photon NOON-like scaling $\Delta\phi_Q\simeq 1/N$. In the biphoton case, the interferometric phase term in $f_Q$ is said to acquire doubled sensitivity,
$$
f_Q(\Omega_1,\Omega_2)\propto
e^{\,i[k_s\,r(\Omega_1)+k_i\,r(\Omega_2)]}\,
\Phi\bigl(r(\Omega_1)-r(\Omega_2)\bigr),
$$
so that small range differences $\delta r$ produce a phase shift $\sim 2k\,\delta r$, halving the range-resolution limit [2205.14000].

## 5. Quantum computation of radar cross sections

The computational QRCS program begins from a conventional electromagnetic scattering setup. An incident plane wave
$$
E_i(r)=E_0 e^{i k_0\cdot r},
\qquad
k_0\cdot E_0=0,
\qquad
\omega=|k_0|c,
$$
generates a steady-state scattered field $E_s(r,\theta,\phi)$ satisfying the vector Helmholtz equation
$$
(\nabla^2+k^2)E_s=0
$$
with boundary conditions on the target surface $S$. After FEM discretization of a $d$-dimensional volume into $N$ finite elements, one obtains the sparse linear system
$$
A x=b,
$$
where $A\in\mathbb{C}^{N\times N}$, $b$ encodes boundary excitation, and $x$ encodes unknown edge-field amplitudes. If $R\in\mathbb{C}^N$ is the observation vector for direction $\hat k$ and polarization $\epsilon$, then the far-field amplitude is $R\cdot x$ and
$$
\sigma(\hat k,\epsilon,k_0,\epsilon_0)=4\pi |R\cdot x|^2/|E_0|^2.
$$
The CJS algorithm builds efficient oracles for $|b\rangle$ and for a rescaled Hermitian operator $\hat H\approx A$ using a sparse-approximate-inverse preconditioner $M$, then applies an HHL variant plus amplitude estimation to compute $|x\rangle$ and estimate $R\cdot x$ in $O(\mathrm{polylog}\,N)$ time [2602.20553].

The preconditioned Hermitian embedding is
$$
\hat H=
\begin{pmatrix}
0 & MA\\
(MA)^\dagger & 0
\end{pmatrix},
$$
acting on $n+1$ qubits with $n\approx \log_2 N$. Phase estimation on $\hat H$ provides access to the eigenvalues of $MA$, controlled rotation inserts $1/\lambda_j$ factors, and the state transformation prepares
$$
|x\rangle \propto \sum_j \frac{\beta_j}{\lambda_j}|u_j\rangle,
\qquad
|b\rangle=\sum_j\beta_j|u_j\rangle.
$$
Amplitude estimation is then used to estimate $\langle R|x\rangle$ with precision $\epsilon$ in $O(1/\epsilon)$ time, after which
$$
\sigma(\theta,\phi)=4\pi |\tilde z|^2/|E_0|^2
$$
is recovered from the estimated amplitude $\tilde z$ [2602.20553].

The circuit-level decomposition is given explicitly:
1. state preparation $O_b$ of size $O(d\log N)$,
2. Hamiltonian simulation of $\hat H$ via Trotter–Suzuki splitting,
3. phase estimation using controlled-$e^{-i\hat H t_j}$ for $t_j=2^j\Delta t$,
4. controlled rotation by $\arcsin(C/\lambda_j)$ followed by uncomputation,
5. Grover-style amplitude estimation of $|\langle R|x\rangle|$ with $O(1/\epsilon)$ calls,
6. measurement of ancillas to read off $\tilde z$ [2602.20553].

The complexity comparison is stark. For sparse FEM, the classical conjugate-gradient solver is quoted as
$$
T_{\rm CG}=O(K\,d\,\log(1/\epsilon)\,N),
\qquad
\text{memory } O(N).
$$
For the quantum CJS algorithm,
$$
T_Q=O(K\,d^7\,\epsilon^{-2}\,\log N).
$$
The same analysis gives approximately $341$ logical qubits without oracles, approximately $3\times 10^8$ logical qubits with oracles, and a Toffoli count of approximately $10^{28}$ [2602.20553].

A crossover analysis equating $T_{\rm CG}\approx T_Q$ gives
$$
N^*\approx W_{-1}(x)/x,
$$
with
$$
x=O\!\left([C_{\rm CG}/C_{\rm QJS}]\,d^{-6}\epsilon^2/\log(1/\epsilon)\right).
$$
For $d=7$ and $\epsilon=10^{-2}$, the reported crossover is $N^*\approx 5\times 10^9$ edges, corresponding to an approximately $12\,885\times 12\,885$ mesh in 2D. At $25\,\mu\mathrm{s}$/logical-gate, the wall-clock time is approximately $10^{17}$ years. A toy 2D model with $1\,\mathrm m$ wavelength, a $2\,\mathrm m$ metallic square, and $0.1\,\mathrm m$ mesh spacing gives $N\approx 3.3\times 10^8$; assuming $K\approx 10^4$, $d=7$, and $\epsilon=10^{-2}$, the reported resource estimate with oracles is $3\times 10^8$ qubits and $1.8\times 10^{29}$ logical time steps, with runtime dominated by Hamiltonian simulation calls [2602.20553].

## 6. Assumptions, implementation constraints, and practical outlook

The assumptions behind the quantum-optical QRCS models are restrictive but explicit. The operator-based treatment assumes Born scattering, far-field propagation, a stationary target, SPDC-generated biphoton wavepackets, and narrowband traveling-wave modes [2205.14000]. The two-photon signal–signal entanglement model assumes non-interacting, independent point scatterers, neglects multiple scattering between atoms, and omits polarization effects, dispersion, absorption, and noise; extension to higher-order entangled Fock states $N>2$, 3D target shapes, and full vector-field $T$-matrices is left open [2606.05603].

The computational QRCS model makes a different set of assumptions: a perfect-conductor, linear, time-invariant scatterer; neglect of material loss and surface roughness; regular FEM meshes to permit efficient oracle construction; and the existence of a sparse approximate inverse $M$ satisfying $M\approx A^{-1}$ and making $K(MA)=O(1)$. Trotter error and amplitude-estimation error contribute to the overall multiplicative error $\epsilon$ in $\sigma$, while mesh discretization error governed by $N^{-p}$ is ignored in the quantum precision budget. The dominant hardware-level noise sources are decoherence, gate infidelity—particularly for Toffoli and $T$ gates—and readout errors; the stated position is that full surface-code error correction is required and that NISQ devices cannot run CJS [2602.20553].

For experimental quantum radar implementations, the design prescriptions are correspondingly demanding: bright, narrow-band entangled-photon sources using periodically poled nonlinear crystals for collinear SPDC; bandwidth $\Delta\omega\approx\mathrm{MHz}$–$\mathrm{GHz}$; heralding and coincidence gating through local idler detection; high-efficiency, low-noise SNSPDs with $\eta>90\%$ and dark count $<1\,\mathrm{Hz}$; quantum-compatible apertures preserving mode purity; far-field illumination and collection optics matched to entangled-beam divergence; and path-length stabilization satisfying $\Delta L\ll \lambda$ using active feedback on delay lines [2205.14000].

The practical-feasibility assessments are largely negative. For the CJS algorithm, the conclusion is that QRCS via CJS is **not feasible on NISQ or early fault-tolerant machines**, with the principal bottlenecks identified as Hamiltonian simulation with its $d^7$ dependence, amplitude estimation with its $\epsilon^{-1}$ scaling, and oracle overhead. Suggested avenues for improvement include the Childs–Kothari–Somma algorithm for Hamiltonian simulation, tensor-network or block-encoding improvements, problem-specific oracle optimization, triangular or tetrahedral meshes to minimize $d$, and shadow-tomography or classical-shadows approaches to reduce amplitude-estimation cost [2602.20553].

A separate practical critique evaluates target detection rather than scattering-pattern reshaping. It uses the same classical radar cross section $\sigma$ for both classical and quantum radar link budgets, writing the two-way attenuation as
$$
a_R=\frac{G^2\lambda^2\sigma}{(4\pi)^2R^4},
$$
the classical received power as
$$
P_r=P_T\,a_R,
$$
and the quantum back-scattered power for QTMS/QI protocols as
$$
P_{r,Q}=M\,N_s\,\hbar\omega\,B\,\eta_Q\,a_R,
$$
with $M=BT$ and ideal $\eta_Q$ “up to 6 dB.” The corresponding SNR formulas are
$$
\mathrm{SNR}_Q=\frac{M\,N_s\,\eta_Q\,a_R}{N_B},
\qquad
\mathrm{SNR}_C=
\frac{P_TG^2\lambda^2\sigma}{(4\pi)^2R^4Bk_BT_s}\,I_{\rm INT},
$$
and the maximum ranges are
$$
R_{\max}^Q
=
\left[
\frac{BT\,N_s\,\eta_Q\,G^2\lambda^2\sigma}{(4\pi)^2(\mathrm{SNR})_{\min}N_B}
\right]^{1/4},
$$
$$
R_{\max}^C
=
\left[
\frac{P_TI_{\rm INT}G^2\lambda^2\sigma}{(4\pi)^2(\mathrm{SNR})_{\min}Bk_BT_s}
\right]^{1/4}.
$$
At X-band with $f\approx 9.4\,\mathrm{GHz}$, $\lambda\approx 3.2\,\mathrm{cm}$, $B=1\,\mathrm{GHz}$, $G=30\,\mathrm{dB}$, $\sigma=1\,\mathrm{m}^2$, $(\mathrm{SNR})_{\min}=13.2\,\mathrm{dB}$, and $T_s=290\,\mathrm K$, the paper states that an ideal quantum radar with $N_s\approx 1$ must integrate for days to see a $1\,\mathrm{m}^2$ target at $R=1\,\mathrm{km}$, whereas a noise radar with $P_T=100\,\mathrm{mW}$ and $I_{\rm INT}=1\,\mathrm s$ achieves $R_C\approx 1$–$2\,\mathrm{km}$; at millimeter-wave frequencies, the same critique states that quantum-illumination ranges fall below approximately $10\,\mathrm m$ for any reasonable dwell, while noise radars still reach tens to hundreds of meters with milliwatts of power [2403.00047].

Taken together, these works place QRCS at the intersection of electromagnetic scattering theory, quantum optics, quantum algorithms, and radar systems analysis. One branch develops operator-based and entanglement-sensitive scattering observables; another pursues quantum speedups for classical RCS solvers; and a third argues that, at the level of far-field target detectability and radar link budgets, the relevant cross section remains the ordinary $\sigma$. The resulting literature is therefore unified less by a single definition than by a common target problem: how quantum resources alter the modeling, measurement, or interpretation of radar cross section.

Source: https://www.emergentmind.com/topics/quantum-radar-cross-section-qrcs