Describe a receiver by a temporal mode
Choose a receiver envelope whose squared magnitude integrates to one within the observation window. This temporal mode specifies when amplitude is large and how phase changes. A photon in it is a coherent superposition of possible arrival times.
The unnormalized collected envelope is . Its squared magnitude integrates to collection probability . Multiplying by the conjugate receiver envelope and integrating instead gives the target-mode amplitude. These operations preserve different information.
Three numbers answer three questions
Collection probability asks how often a photon reaches the port. Conditional mode fidelity asks how closely the collected photon matches the receiver mode. Unconditional target weight combines them, giving the target single-photon probability per attempt.
At , conditional fidelity is undefined. A high conditional value can coexist with almost no successful collection. High collection can coexist with a badly mismatched phase or timing.
This formula assumes a pure one-photon mode in the selected port. Unrecorded random phase or spectral mixing requires a density matrix. Averaging complex envelopes from different trials does not generally replace that calculation.
Loss need not change the collected shape
An ideal frequency-independent branch collecting a fraction changes the envelope to . The overlap amplitude receives the same factor. Collection and target weight decrease, while normalized conditional fidelity stays fixed.
Worked example: collection is and conditional mode fidelity is . Target weight per attempt is . Perfecting the shape with the same loss can raise this only to . Further gains need reduced loss or more amplitude in the receiver mode.
Equal intensity can still give a small overlap
Give one of two equal-intensity pulses a phase that rotates with time. Their intensity traces remain identical, but contributions to the inner product can cancel. A constant overall phase only rotates the final overlap arrow. A changing phase alters the mode match.
For a normalized hyperbolic-secant envelope on the whole time axis, a temporal offset has the overlap below. At , its amplitude is approximately and fidelity . A finite record needs a fresh integral over its actual window.
A delayed pulse can miss a fixed receiver mode
- Receiver
- Delayed emission
Reading: Sandbox Physics FR11
Worked example: reverse only the second half
Choose an ideal receiver on , zero elsewhere. Emit the same shape with collection probability , then reverse its phase by half a turn in the second half. Intensity remains throughout, so collection is still 0.8.
The inner product adds equal positive and negative contributions, cancelling exactly. Conditional fidelity and target weight become zero. Reversing the entire pulse instead leaves all contributions aligned and conditional fidelity one. The ideal example separates phase mismatch from energy loss.
Evaluate an interface from a finite record
The node experiment fixes a hyperbolic-secant receiver mode and varies emission bandwidth, collected branching, detuning and pulse centre. Its source survival probability and both output branches come from one controlled emission model and sum to one at every time.
A finite start requires survival to be normalized by its initial value. The target mode is normalized inside the same finite window. Moving a pulse can move part of its tail outside that window; check this before attributing the whole change to mode mismatch.
The finite bath also projects its right-port record onto a fixed receiver: its normalized default resonant output over the same window. This is separate from the node experiment’s sech target. After moving toward the band edge, project the new complex right-port record to see how returning light and tails affect collection, conditional fidelity and target weight.
Change one quantity at a time: branching first, then detuning, then pulse centre. The first mainly changes success probability. The other two expose the role of phase and timing for the same receiver.
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