Spiegazione per gradi di libertà non interi in t test con varianze disuguali

La procedura T-Test SPSS riporta 2 analisi quando si confrontano 2 medie indipendenti, un'analisi con varianze uguali assunta e una con varianze uguali non ipotizzata. I gradi di libertà (df) quando si assumono varianze uguali sono sempre valori interi (e uguale n-2). I df quando non si ipotizzano varianze uguali sono non interi (es. 11.467) e in nessun luogo vicino a n-2. Sto cercando una spiegazione della logica e del metodo utilizzato per calcolare questi df non interi.

Si può dimostrare che Welch-Satterthwaite df è una media armonica ponderata in scala dei due gradi di libertà, con pesi proporzionati alle corrispondenti deviazioni standard.

L'espressione originale recita:

$$\nu_{_W} = \frac{\left(\frac{s_1^2}{n_1}+\frac{s_2^2}{n_2}\right)^2}{\frac{s_1^4}{n_1^2\nu_1}+\frac{s_2^4}{n_2^2\nu_2}}$$

Notare che è la varianza stimato i esimo campione medio o quadrato della i -esimo errore standard della media . Sia r = r 1 / r 2 (il rapporto delle varianze stimate della media del campione), quindi$r_i=s_i^2/n_i$$i^\text{th}$$i$$r=r_1/r_2$

$$\begin{align} \nu_{_W} &= \frac{\left(r_1+r_2\right)^2}{\frac{r_1^2}{\nu_1}+\frac{r_2^2}{\nu_2}} \newline \newline &=\frac{\left(r_1+r_2\right)^2}{r_1^2+r_2^2}\frac{r_1^2+r_2^2}{\frac{r_1^2}{\nu_1}+\frac{r_2^2}{\nu_2}} \newline \newline &=\frac{\left(r+1\right)^2}{r^2+1}\frac{r_1^2+r_2^2}{\frac{r_1^2}{\nu_1}+\frac{r_2^2}{\nu_2}} \end{align}$$

$1+\text{sech}(\log(r))$$1$$r=0$$2$$r=1$$1$$r=\infty$$\log r$

Il secondo fattore è una media armonica ponderata :

$$H(\underline{x})=\frac{\sum_{i=1}^n w_i }{ \sum_{i=1}^n \frac{w_i}{x_i}}\,.$$

of the d.f., where $w_i=r_i^2$ are the relative weights to the two d.f.

Which is to say, when $r_1/r_2$ is very large, it converges to $\nu_1$. When $r_1/r_2$ is very close to $0$ it converges to $\nu_2$. When $r_1=r_2$ you get twice the harmonic mean of the d.f., and when $s_1^2=s_2^2$ you get the usual equal-variance t-test d.f., which is also the maximum possible value for $\nu_{_W}$.

--

With an equal-variance t-test, if the assumptions hold, the square of the denominator is a constant times a chi-square random variate.

The square of the denominator of the Welch t-test isn't (a constant times) a chi-square; however, it's often not too bad an approximation. A relevant discussion can be found here.

A more textbook-style derivation can be found here.

What you are referring to is the Welch-Satterthwaite correction to the degrees of freedom. The $t$-test when the WS correction is applied is often called Welch's $t$-test. (Incidentally, this has nothing to do with SPSS, all statistical software will be able to conduct Welch's $t$-test, they just don't usually report both side by side by default, so you wouldn't necessarily be prompted to think about the issue.) The equation for the correction is very ugly, but can be seen on the Wikipedia page; unless you are very math savvy or a glutton for punishment, I don't recommend trying to work through it to understand the idea. From a loose conceptual standpoint however, the idea is relatively straightforward: the regular $t$-test assumes the variances are equal in the two groups. If they're not, then the test should not benefit from that assumption. Since the power of the $t$-test can be seen as a function of the residual degrees of freedom, one way to adjust for this is to 'shrink' the df somewhat. The appropriate df must be somewhere between the full df and the df of the smaller group. (As @Glen_b notes below, it depends on the relative sizes of $s^2_1/n_1$ vs $s_2^2/n_2$; if the larger n is associated with a sufficiently smaller variance, the combined df can be lower than the larger of the two df.) The WS correction finds the right proportion of way from the former to the latter to adjust the df. Then the test statistic is assessed against a $t$-distribution with that df.