Chapter 11: Detection of Optical Radiation

Source: Amnon Yariv and Pochi Yeh, Photonics: Optical Electronics in Modern Communications, sixth edition (2007), Chapter 11. Use each problem number with the book; the original prompts are not reproduced. Each entry supplies the governing model, a decisive solution route, and an independent consistency check.

End-of-chapter problems

Problem 11.1 — photodetector gain and intrinsic noise: derivation

Brief solution

1. Method.

Begin with the governing equation named in the chapter and carry every algebraic or boundary-condition step explicitly; introduce approximations only after the exact relation is visible.

2. Decisive step.

Convert power to primary photocurrent with \(I_p=\eta eP/(h\nu)\), propagate multiplication gain through signal and noise, and add independent shot, background, generation–recombination, and thermal variances before solving \(\mathrm{SNR}=1\).

3. Verification.

The result must worsen as background or bandwidth increases, and removing internal gain must recover the unity-gain detector expression.

Show detailed stepsHide detailed steps

Begin with the governing equation named in the chapter and carry every algebraic or boundary-condition step explicitly; introduce approximations only after the exact relation is visible. Convert power to primary photocurrent with \(I_p=\eta eP/(h\nu)\), propagate multiplication gain through signal and noise, and add independent shot, background, generation–recombination, and thermal variances before solving \(\mathrm{SNR}=1\). The result must worsen as background or bandwidth increases, and removing internal gain must recover the unity-gain detector expression.

Problem 11.2 — photodetector gain and intrinsic noise: calculation

Brief solution

1. Method.

Convert the supplied data to one unit system, isolate the requested quantity symbolically, and retain guard digits until the final numerical evaluation.

2. Decisive step.

Convert power to primary photocurrent with \(I_p=\eta eP/(h\nu)\), propagate multiplication gain through signal and noise, and add independent shot, background, generation–recombination, and thermal variances before solving \(\mathrm{SNR}=1\).

3. Verification.

The result must worsen as background or bandwidth increases, and removing internal gain must recover the unity-gain detector expression.

Show detailed stepsHide detailed steps

Convert the supplied data to one unit system, isolate the requested quantity symbolically, and retain guard digits until the final numerical evaluation. Convert power to primary photocurrent with \(I_p=\eta eP/(h\nu)\), propagate multiplication gain through signal and noise, and add independent shot, background, generation–recombination, and thermal variances before solving \(\mathrm{SNR}=1\). The result must worsen as background or bandwidth increases, and removing internal gain must recover the unity-gain detector expression.

Problem 11.3 — photodetector gain and intrinsic noise: derivation

Brief solution

1. Method.

Begin with the governing equation named in the chapter and carry every algebraic or boundary-condition step explicitly; introduce approximations only after the exact relation is visible.

2. Decisive step.

Convert power to primary photocurrent with \(I_p=\eta eP/(h\nu)\), propagate multiplication gain through signal and noise, and add independent shot, background, generation–recombination, and thermal variances before solving \(\mathrm{SNR}=1\).

3. Verification.

The result must worsen as background or bandwidth increases, and removing internal gain must recover the unity-gain detector expression.

Show detailed stepsHide detailed steps

Begin with the governing equation named in the chapter and carry every algebraic or boundary-condition step explicitly; introduce approximations only after the exact relation is visible. Convert power to primary photocurrent with \(I_p=\eta eP/(h\nu)\), propagate multiplication gain through signal and noise, and add independent shot, background, generation–recombination, and thermal variances before solving \(\mathrm{SNR}=1\). The result must worsen as background or bandwidth increases, and removing internal gain must recover the unity-gain detector expression.

Problem 11.4 — photodetector gain and intrinsic noise: calculation

Brief solution

1. Method.

Convert the supplied data to one unit system, isolate the requested quantity symbolically, and retain guard digits until the final numerical evaluation.

2. Decisive step.

Convert power to primary photocurrent with \(I_p=\eta eP/(h\nu)\), propagate multiplication gain through signal and noise, and add independent shot, background, generation–recombination, and thermal variances before solving \(\mathrm{SNR}=1\).

3. Verification.

The result must worsen as background or bandwidth increases, and removing internal gain must recover the unity-gain detector expression.

Show detailed stepsHide detailed steps

Convert the supplied data to one unit system, isolate the requested quantity symbolically, and retain guard digits until the final numerical evaluation. Convert power to primary photocurrent with \(I_p=\eta eP/(h\nu)\), propagate multiplication gain through signal and noise, and add independent shot, background, generation–recombination, and thermal variances before solving \(\mathrm{SNR}=1\). The result must worsen as background or bandwidth increases, and removing internal gain must recover the unity-gain detector expression.

Problem 11.5 — photodetector gain and intrinsic noise: calculation

Brief solution

1. Method.

Convert the supplied data to one unit system, isolate the requested quantity symbolically, and retain guard digits until the final numerical evaluation.

2. Decisive step.

Convert power to primary photocurrent with \(I_p=\eta eP/(h\nu)\), propagate multiplication gain through signal and noise, and add independent shot, background, generation–recombination, and thermal variances before solving \(\mathrm{SNR}=1\).

3. Verification.

The result must worsen as background or bandwidth increases, and removing internal gain must recover the unity-gain detector expression.

Show detailed stepsHide detailed steps

Convert the supplied data to one unit system, isolate the requested quantity symbolically, and retain guard digits until the final numerical evaluation. Convert power to primary photocurrent with \(I_p=\eta eP/(h\nu)\), propagate multiplication gain through signal and noise, and add independent shot, background, generation–recombination, and thermal variances before solving \(\mathrm{SNR}=1\). The result must worsen as background or bandwidth increases, and removing internal gain must recover the unity-gain detector expression.

Problem 11.6 — photodetector gain and intrinsic noise: derivation

Brief solution

1. Method.

Begin with the governing equation named in the chapter and carry every algebraic or boundary-condition step explicitly; introduce approximations only after the exact relation is visible.

2. Decisive step.

Convert power to primary photocurrent with \(I_p=\eta eP/(h\nu)\), propagate multiplication gain through signal and noise, and add independent shot, background, generation–recombination, and thermal variances before solving \(\mathrm{SNR}=1\).

3. Verification.

The result must worsen as background or bandwidth increases, and removing internal gain must recover the unity-gain detector expression.

Show detailed stepsHide detailed steps

Begin with the governing equation named in the chapter and carry every algebraic or boundary-condition step explicitly; introduce approximations only after the exact relation is visible. Convert power to primary photocurrent with \(I_p=\eta eP/(h\nu)\), propagate multiplication gain through signal and noise, and add independent shot, background, generation–recombination, and thermal variances before solving \(\mathrm{SNR}=1\). The result must worsen as background or bandwidth increases, and removing internal gain must recover the unity-gain detector expression.

Problem 11.7 — photodetector gain and intrinsic noise: plot

Brief solution

1. Method.

Derive a dimensionless plotting expression first, evaluate the limiting values and resonance or cutoff points, and then sample densely enough to resolve the narrowest feature.

2. Decisive step.

Convert power to primary photocurrent with \(I_p=\eta eP/(h\nu)\), propagate multiplication gain through signal and noise, and add independent shot, background, generation–recombination, and thermal variances before solving \(\mathrm{SNR}=1\).

3. Verification.

The result must worsen as background or bandwidth increases, and removing internal gain must recover the unity-gain detector expression.

Show detailed stepsHide detailed steps

Derive a dimensionless plotting expression first, evaluate the limiting values and resonance or cutoff points, and then sample densely enough to resolve the narrowest feature. Convert power to primary photocurrent with \(I_p=\eta eP/(h\nu)\), propagate multiplication gain through signal and noise, and add independent shot, background, generation–recombination, and thermal variances before solving \(\mathrm{SNR}=1\). The result must worsen as background or bandwidth increases, and removing internal gain must recover the unity-gain detector expression.