Exponential limit of a one-sided periodogram 2026-10-14
At an interior frequency, the real and imaginary Fourier coefficients of a short-memory Gaussian time series converge jointly to independent centered normal variables, each with variance , where is the one-sided spectral density. Their squared sum therefore converges to . Its variance tends to , so an unsmoothed periodogram is not consistent when . Averaging nearby ordinates can reduce this persistent variance.
Local periodogram smoothing 2026-10-14
Average neighboring periodogram ordinates with nonnegative weights summing to one. Let the number of averaged ordinates tend to infinity while their frequency span, of order , tends to zero. For a smooth spectral density and suitable short-memory or fourth-order dependence conditions, the bias tends to zero and variance is of order . Smooth second-order spectral density alone does not ensure this: a time-constant random scale multiplying independent white noise has a smooth unconditional spectrum but a nonergodic random limiting local power.
Optical trap Langevin calibration Created 2026-10-18 Updated 2026-10-20
Add the random thermal force to the deterministic optical trap relaxation time model. In one stationary coordinate of a harmonic optical trap, the overdamped Langevin equation isHere is Gaussian white noise understood through its integrals, is the Dirac delta function, and is the linear friction coefficient. The covariance coefficient has units ; multiplying by , of units , gives squared force. This fluctuation-dissipation relation for a Langevin particle makes the stationary variance , consistent with the equipartition theorem. The solution is an Ornstein-Uhlenbeck process with autocovariance functionIndeed, at positive lag the noise has zero correlation with the initial position, so ; its initial value is . This supplies both a decay time and an amplitude, making a stronger calibration test than a position histogram alone.
Specify the Fourier transform convention before using a power spectral density. For frequency in hertz, define and the one-sided density for . Integration of the exponential givesThe position power spectral density has units ; its integral is a variance, not a standard deviation. At it is half its zero-frequency plateau. Angular frequency conventions require a corresponding conversion in both axis and integration measure. If with position sensitivity in , then in before independent detector noise is added.
For an original invented calibration example, choose , dynamic viscosity , , , and . The unbounded no-slip Stokes drag law givesThe corresponding voltage standard deviation is , and the position power spectral density plateau is , or in the detector. Recovering both and is an internal model check; actual agreement also tests the assumed temperature, drag and detector response.
Synthetic harmonic optical trap fluctuations, power spectral density and optical trap drag calibration
. Original model calculations and seeded synthetic Ornstein-Uhlenbeck process samples; explicitly not measured data. The record is sampled at with no detector noise or exposure averaging. The dashed spectrum includes sampling aliases; the red continuous spectrum integrates to the exact equipartition theorem variance. The drag line is an exact steady-model prediction. Source. Details.The generator uses the exact stationary update , with and independent standard normal random variables . For a demeaned block of samples and its unnormalized discrete Fourier transform , the two-sided periodogram is ; doubling positive bins except the zero and Nyquist endpoints gives a one-sided density. Summing those bins times returns the block mean square by discrete Parseval identity. Independent detector noise, finite exposure and aliasing would alter a measured spectrum and must enter a fit before interpreting .
Past exam of the mathematics course of the University of Cambridge 2001 iii Paper 33 3 Solution Created 2026-10-03 Updated 2026-10-14
Write for the driving white noise variance and . The autoregressive polynomial factors asThe discrete Gaussian white noise values are independent. The roots of are outside the unit disc, so expanding gives an absolutely summable causal time-series representation. Hence is a centered Gaussian process formed from driving white noise values at times at most . In particular, for , every driving white noise value with is independent of . The autocovariance tail recurrence of a causal ARMA process follows by taking covariance of the recursion with :
The roots of the characteristic polynomial of this tail recurrence are and . Let . There exist constants such thatFor example, put and ; then and reproduce the two starting values and therefore the whole recurrence. Choose strictly larger than and all the finitely many values with . Symmetry now givesFor negative this is stronger than the requested bound with . It also proves .
For the Fourier calculation, take positive and positive. The supplied equal-norm trigonometric identities require ; the usual intended range is . Because is odd, at every such nonzero frequency. The geometric series of and over terms vanish. They implyOther integer values of reduce modulo ; folding a negative frequency changes the sine coefficient only by a sign. The permitted zero frequency is handled below.
Grouping the double expectation sum according to the time lag yieldsReplace the two truncated sums for lag by full sums. Their total isEach replacement adds at most terms, each of absolute value at most one. This gives the finite-record Fourier covariance bound:Both coefficients have expected value zero, so this expectation is their covariance.
For each finite , has a multivariate normal distribution because it is a linear transformation of the Gaussian observation vector. If the variances converge to , its characteristic function converges tosince the cross-covariance tends to zero. This is the characteristic function of two independent centered normal variables; zero limiting variances are allowed.
We can calculate the variance limits rather than merely assume their existence. Grouping the cosine covariance sum givesOver a full record, . Truncation changes this by at most . The same statements hold for the sine products. Consequentlyand the identical main term and bound apply to . Absolute summability now gives
Specify the spectral convention to identify this limit. LetHere is the two-sided probability density function on , and is the one-sided probability density function on , satisfying . Thus each variance limit is . For this particular model, the filter representation also gives
For the specified squared-sum estimator, an exact expectation calculation uses :The missing tail and the terms vanish; indeed the bias is by the exponential covariance bound. Therefore is asymptotically unbiased for the one-sided probability density function . Under the common two-sided convention its limit in expectation is , so is the appropriately normalized estimator.
At an interior frequency with , the joint Gaussian limit gives the exponential limit of a one-sided periodogram:Moreover, for a centered Gaussian pair,The nondegenerate exponential limiting law rules out convergence in probability to . Thus the unsmoothed periodogram is not consistent at frequencies with positive spectrum, despite its asymptotic unbiasedness. If , the nonnegative estimator has expectation tending to zero and is consistent there by Markov's inequality. Smoothing an increasing number of nearby ordinates while shrinking the frequency bandwidth can remove the positive-spectrum variance obstruction.
For , the sine coefficient is identically zero and the cosine coefficient is the normalized sum of the observations. The corrected limits areThe joint limit is , independent in the degenerate sense. The exact expectation formula for still applies and tends to , but now when , with limiting variance . The estimator is again inconsistent. This covers the zero frequency allowed by the printed inequality on .
The figure uses the allowed cancellation , so the observations reduce to white noise. Orthogonal Fourier projections give the exponential law exactly at each plotted record length; increasing the record does not narrow the individual periodogram ordinate.
Past exam of the mathematics course of the University of Cambridge 2003 iii Paper 43 5 Solution Created 2026-10-03 Updated 2026-10-14
Write and . The discrete Fourier transform coefficient is . Alternatively, by the given orthogonality relations, the harmonic obtained by linear least-squares projection has coefficients and . Thus the source's periodogram is the squared amplitude of a fitted harmonic, scaled as power per unit angular frequency:It measures how much of the centered record varies at frequency . For odd , Fourier Parseval identity givesThe positive-frequency spacing is , so summing the power ordinates times this spacing estimates the total variance. The factor corresponds to the one-sided spectral density on ; the usual two-sided periodogram is half as large.
If the observations are Gaussian white noise with common variance , the harmonic sums are jointly normally distributed. Their means are zero even with a nonzero constant series mean, because each sine and cosine sums to zero. Orthogonality givesUncorrelated coordinates of a multivariate normal distribution are independent. Therefore all and are independent standard normals, andSince the chi-squared distribution with two degrees of freedom has mean two and variance four,Here is the one-sided white-noise spectral density. Its exact unbiasedness is accompanied by a nonconcentrating distribution: along Fourier frequencies tending to any interior frequency, has the same nondegenerate exponential law at every . It therefore does not converge in probability to one, proving failure of statistical consistency, not just nonvanishing variance.
For a general stationary process, exact finite-sample unbiasedness is not implied. Expanding the Fourier square instead giveswhere is the autocovariance function. Under suitable short-memory regularity this tends to at frequencies . The periodogram is thus generally asymptotically unbiased, while the exact assertion above is for white noise.
Use local periodogram smoothing to reduce variance: average neighboring ordinates with weights summing to one, where but . At an interior frequency the shrinking frequency window makes the bias tend to zero for smooth , while averaging many weakly dependent ordinates makes the variance of order . For white noise with equal weights, the ordinates are exactly independent and the variance is exactly . For a general process, impose suitable short-memory and fourth-order dependence assumptions, such as a stationary Gaussian model with sufficiently summable autocovariances. These conditions, together with smoothness, give a consistent smoothed estimator. Boundary frequencies require an appropriately one-sided or reflected window.
Smooth spectral density alone is not enough. For example let , where is a nondegenerate random variable constant throughout the record, independent of independent unit-variance Gaussian , with . The unconditional autocovariance is zero off lag zero and its one-sided spectral density is the smooth constant . Nevertheless a long local average estimates the realized , not that deterministic unconditional value. This nonergodic example explains why a dependence/ergodicity condition accompanies the smoothing argument.
For the turning point test of randomness, the null is independent identically distributed continuous observations. Let be one if is a strict local maximum or minimum among , for , and set . Three ranks are equally likely; the middle observation is an extremum in four of the six orders, giving and . ThereforeIndicators more than two positions apart depend on disjoint observations and are independent. For neighboring indicators, both are one precisely when four observations alternate up-down-up or down-up-down. By the probability-integral transform, use four independent uniforms. The first pattern has probabilityhere , , with the two outer inequalities having probabilities and . The reverse pattern has the same probability, so and .
At separation two, the triples share only one endpoint value . Conditional on it, their other observations are independent. The probability that either triple's central observation is a turning point isIt follows that , so this covariance is . Combining all terms for givesThe standardized count is approximately standard normal for large , by a central limit theorem for bounded 2-dependent indicators. A two-sided randomness test rejects for large absolute values ofToo few turns suggests persistent movement, while too many suggests alternation. Exact rank-permutation calibration is possible at small . Ties invalidate the continuous-rank probabilities unless their handling is specified. The test probes this feature of randomness; nonrejection does not establish independence.
Past exam of the mathematics course of the University of Cambridge 2016 iii Paper 208 2 2 Solution Created 2026-10-03 Updated 2026-10-06
With angular frequency , the periodogram isAt Fourier frequencies it is the squared modulus of the normalized discrete Fourier transform. If a nonzero mean is unknown, subtract the sample mean first.
For a zero-mean stationary process, expanding the square givesUnder absolute summability of the covariances this converges to the spectral density of a stationary process. Thus the periodogram is generally biased at finite , but asymptotically unbiased under this short-memory time series condition.
It is nevertheless not a pointwise estimator with statistical consistency unless it is smoothed. For Gaussian white noise, at a nonzero Fourier frequency other than the Nyquist frequency, the real and imaginary Fourier components are independent normal variables. Exactly,where . The variance does not decrease with . Under usual short-memory time series assumptions the same exponential limit is asymptotic for general processes. Averaging nearby frequencies or using a lag-window estimator reduces variance; a frequency bandwidth tending to zero while times that bandwidth tends to infinity can give statistical consistency. The raw plot remains useful for detecting strong periodic peaks, but increasing the record length alone does not remove its pointwise noise.

