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A differential inequality for an exponential tail envelope supplies a sufficient decay condition for a global power bound. Let nonnegative $P$ be absolutely continuous on every finite interval after $b$, with $P(b)\le A$ andalmost everywhere, for constant $\tau >0$. The integrating factor argument in bounding unobserved optical energy with an exponential tail model gives $P(t)\le A{e}^{-(t-b)/\tau }$. Corners in the waveform are allowed under absolute continuity; an unmodeled upward jump is not.

The inequality is stronger than merely fitting a decay constant at a few sampled times. For example, $P(t)=A{e}^{-2(t-b)/\tau }$ obeys it and carries only $A\tau /2$ after $b$. The exponential-envelope tail-energy bound $A\tau$ remains valid but need not be tight. Conversely, a later pulse can violate the differential condition while leaving all earlier samples unchanged.

A useful extension is a time-dependent decay-rate envelope. For locally integrable $k(t)\ge 0$, the condition $P^{\prime }\le -kP$ givesThis follows from the same integrating factor and is a scalar comparison bound. If $k(t)\ge k_{\min }>0$ throughout the tail, its integrated energy is at most $A/k_{\min }$.

For an original piecewise rate, choose $A=0.20\mathrm{W}$, $k=1/(10\mathrm{ns})$ for the first $10\mathrm{ns}$ and $k=1/(5\mathrm{ns})$ thereafter. Integrating the resulting continuous envelope yieldsUsing only the minimum rate would give $2.0\mathrm{nJ}$. Faster guaranteed late decay tightens the result.

This is a conditional mathematical proof. A measured electrical waveform obeying a similar slope rule does not establish the optical condition without accounting for the detector impulse response. The primary NIST measurement procedure supplies an example of characterizing that response independently.^[ref]

A power-law tail from a decaying rate envelope arises when a positive instantaneous decay rate weakens with time. The time-dependent decay-rate envelope with $k(t)=\alpha /(t-b+t_0)$ givesfor $A\ge 0$, $t_0>0$ and $\alpha >0$. The parent article obtains this envelope by integrating the rate. Its use for recording design additionally requires integrating over the entire unrecorded tail.

For $\alpha >1$, integration after an extension $L\ge 0$ givesHence the acquisition duration from a power-law tail-energy tolerance $\epsilon >0$ is zero when $A{t}_0/(\alpha -1)\le \epsilon$; otherwise it is sufficient to choose

In an original example, $A=0.10\mathrm{W}$, $t_0=10\mathrm{ns}$ and $\alpha =2$ give an initial energy allowance $1.0\mathrm{nJ}$. Reducing the remaining allowance to $0.010\mathrm{nJ}$ requires $L\ge 990\mathrm{ns}$. An exponential envelope with the same initial allowance and a $10\mathrm{ns}$ decay time would require only $10\log 100\approx 46.05\mathrm{ns}$. Equal initial tail-energy allowances therefore do not imply equal acquisition durations.

For $0<\alpha \le 1$, the envelope tends to zero but its integral after every finite extension diverges. These assumptions then supply no finite missed-energy guarantee. They do not imply that every signal lying below the envelope has infinite energy.

This is an original comparison model, not a measured decay law attributed to a particular detector. In optical pulse metrology, NIST's response measurement separates receiver dynamics from the incident pulse before applying bandwidth corrections.^[ref] The same physical distinction is necessary before interpreting any measured slow tail as a global bound on optical power.

A validated lower bound on a power-law tail exponent is an exponent constraint that is justified over the future interval where it is used to bound unrecorded energy. A fitted slope over a finite observation window is not by itself such a guarantee. Acquisition duration from a power-law tail-energy tolerance needs a global optical-power envelope, including a lower exponent limit above one for its finite-energy guarantee.

One sufficient condition, for positive absolutely continuous power, isIntegrating the logarithmic derivative gives $P(b+u)\le A(1+u/t_0{)}^{-{\alpha }_{\min }}$. The time-dependent decay-rate envelope provides the equivalent integrating-factor argument when zeros of the power need handling. This is a sufficient condition, not a necessary characterization of every bounded tail.

For an original conditional estimation example, assume an exact power-law family with known $t_0=10\mathrm{ns}$ and initial power $A=0.10\mathrm{W}$. At $u=90\mathrm{ns}$, a measured ratio range $0.008\le P(b+u)/P(b)\le 0.012$ yieldsapproximately $1.9208\le \alpha \le 2.0969$. Within that assumed family, the lower endpoint gives a conservative extension about $123.32\mathrm{ns}$ for a $0.10\mathrm{nJ}$ remaining-energy tolerance. A nominal exponent two would instead require $90\mathrm{ns}$.

The ratio interval constrains the exponent only conditional on the exact family, known time scale and suitable measurement uncertainty. It cannot exclude a later secondary pulse or a transition to a slower law after the observed window. Future-domain validity of a fitted power-law optical envelope therefore requires independent physical justification or explicitly limited claims. If the justified exponent set reaches one, this envelope alone supplies no finite all-time energy guarantee.

Finally, the measured trace must represent optical power rather than an uncorrected receiver tail. NIST measured the detector, cable and oscilloscope together using a short characterized optical input before correcting pulse measurements.^[ref] The exponent example is an original model calculation, not an observed law attributed to that apparatus.