Any chance a non physicist / scientist can understand in a nutshell what it means? (5σ at .2) it has been a long time since college. Is that a statistical notation? or something specific to physics? Googling it (or even using symbolhound) didn't render good results for me.
Each experimental outcome has an associated probability that the outcome resulted from chance, not the thing being measured. This arises from the default scientific precept that is called the "null hypothesis", the assumption that a given measurement was produced by chance, not nature.
Scientists use a value designated by p to describe the probability that a result arose by chance rather than design. In the social sciences, a p value of 0.01 - 0.05 is common, which means a result can be explained by chance with a 1% to 5% probability. As one moves through fields of greater rigor and seriousness, the p value required to declare a discovery becomes smaller. In experimental physics, 5σ (five sigma) has become the standard.
In statistics, σ refers to an area under the normal distribution defined in terms of standard deviations (1σ = 1 standard deviation). Experimental physics uses a one-tailed 5σ value, which is quite strict -- it has a numerical value of about 3×10-7. What this means is that an experimental result must be solid enough (and/or be repeated often enough) that the probability that it arose from chance is equal to or less than 5σ.
> In statistics, σ refers to an area under the normal distribution defined in terms of standard deviations (1σ = 1 standard deviation).
No. The Gaussian (normal distribution) is not
involved. Sigma is just the symbol for
standard deviation, that is, the square root
of the variance. So, for random variable
X where with expectation E[X] that exists
and is finite (in practice a weak
assumption), the standard deviation is
square root of E[(X - E[X])^2].
So, the standard deviation is just a number,
a measure of how 'spread out' the distribution
is, and not an "area". Then 5σ is just 5 times
the standard deviation.
>> In statistics, σ refers to an area under the normal distribution defined in terms of standard deviations (1σ = 1 standard deviation).
> No.
Yes. The reason the various sigma values have the numerical values they have is because they represent integrals under the normal distribution, either one-tailed or two-tailed. Therefore in the present context sigma values represent definite integrals of the normal distribution.
> Then 5σ is just 5 times the standard deviation.
Yes, correct, except that the present conversation is about p-values and the meaning of sigma in this specific context. Five sigma has the value it does because it represents one minus the area between 0 and five sigma of the normal distribution, i.e. the one-tailed meaning of five sigma.
Quote: "A graph of the normal distribution, showing 3 standard deviations on either side of the mean µ. A five-sigma observation corresponds to data even further from the mean."
Quote: "For particle physics, the sigma used is the standard deviation arising from a normal distribution of data, familiar to us as a bell curve. In a perfect bell curve, 68% of the data is within one standard deviation of the mean, 95% is within two, and so on."
> Yes. The reason the various sigma values have the numerical values they have is because they represent integrals under the normal distribution, either one-tailed or two-tailed.
No. I defined sigma, that is, standard deviation, fully precisely and correctly.
The normal distribution has nothing to do with that
definition. And the standard deviation is a number,
just a number, just as I defined it as
σ = E[(X - E[X])^2]^(1/2)
which clearly is just a number and not an area.
Or, for random variable X
with cumulative distribution F_X, that is,
for real number x,
P(X <= x) = F_X(x)
we have, with notation from D. Knuth's TeX, that
σ^2 = \int (x - E[X])^2 dF_X(x)
This integral need not be in the sense of
Riemann (i.e., freshman calculus) because
dF_X is a measure on the real line;
so, the integral is in the sense of
measure theory (see any of Rudin, Real and Complex
Analysis; Royden, Real Analysis;
Halmos, Measure Theory; Loève, Probability
Theory).
Sigma is defined for any random variable X or its
distribution provided that E[X] exists and is
finite. Again, a "normal" or Gaussian assumption
is not necessary. So, sigma is defined for
discrete distributions, the uniform distribution,
the Poisson distribution, the exponential distribution,
etc.
For a random variable X, if don't know its distribution,
then can't say what the numerical value of its
standard distribution is.
Moreover if for some random variable X
that has a standard deviation want to know, say,
the probability
P( -5σ <= X <= 5σ)
then that is an area and need the distribution
of X to find the numerical value.
All that is 100%, completely, totally, absolutely
true. That's what σ or standard deviation is.
In particular, the statement
"In statistics, σ refers to an area under the normal distribution defined in terms of standard deviations (1σ = 1 standard deviation)."
is flatly false. The field of statistics has no
such statement or convention.
Yes, if want to be really sloppy, make some
assumptions not clearly stated,
and have some conventions for identifying
some things in special ways, e.g., that
sigma is an area, then can do so. Maybe
some parts of physics do this. I do remember
when I was studying physics the prof handed
out a little book on how errors were
handled in physics. The book was a sloppy
mess and one of the reasons I lost respect
for accuracy and precision in physics and
majored in math instead.
It is true that about 100 years ago some
fields of study, especially parts of psychology
and much of education, concluded that the Gaussian
distribution was some universal law of data
handed down
by God. Well, God did no such thing. Still,
some people in educational statistics believe
that student test scores should have a Gaussian
distribution and, if the scores do not have
such a distribution, will, from many such
scores, find the empirical distribution and, then,
transform the scores so that the distribution
is closely Gaussian.
Maybe physics drank that Kool Aid that all
experimental errors of course, as given by
God, have a Gaussian distribution, that is
"a perfect bell curve",
and, then, yes, can get
"68% of the data is within one standard deviation of the mean, 95% is within two, and so on.",
and that σ has a particular numerical value
and regard standard deviation as an area.
Yes, maybe this is physics but it
is very sloppy thinking and
not mathematics, probability, statistics,
or anything from God.
Of course, even with a Gaussian assumption,
standard deviation does not have a
particular numerical value. Instead,
for Gaussian random variable X with
E[X} = 0 each of
Maybe physics drank that Kool Aid that all experimental errors of course, as given by God, have a Gaussian distribution, that is "a perfect bell curve", and, then, yes, can get "68% of the data is within one standard deviation of the mean, 95% is within two, and so on.", and that σ has a particular numerical value and regard standard deviation as an area. Yes, maybe this is physics but it is very sloppy thinking
That's very interesting!
What are some practical or pragmatic advantages of your way of thinking compared to the standard (sloppy) way of thinking? I don't mean to put you on the spot; I genuinely would love to know.
For example, what are some statistical problems which the standard (sloppy) mental model would have a tough time solving, but which your mental model would be able to yield tools for?
The OP's argument may be that the normal distribution is often applied to datasets with which it has no innate connection and that can only mislead the applier. This is correct -- there are any number of examples where the statistical reasoning behind the normal distribution is wildly inappropriate to the data set being analyzed. The classic example is a dataset with anomalous outliers, say, a cohort in which one person died in childbirth and another who lived to the age of 120. Average age: 60.
But the physicists who apply this method to their LHC data, and those who apply it to the newer finding of gravitational waves, know exactly what they're doing. The data being analyzed are entirely appropriate to this method, and the conclusions being drawn are sound.
Mary teaches calculus to 20 students, and Bob also teaches
calculus to 15 students. A standardized test is given
to all the students, all 35.
So, suppose we assume a null hypothesis that
all 35 student scores are independent random
variables with the same distribution, that is,
(1) Mary and Bob are equally good as teachers
and (2) their students are equally well qualified.
If the students had been appropriately randomly
assigned to Mary and Bob, then maybe we can believe
(2) so that only (1) is in question. So, we are
going to test (1), that is, that Mary and Bob are
equally good as teachers.
This hypothesis, that is, that Mary and Bob are
equally good is called a null hypothesis since
it assumes that there is no effect between
Mary's class and Bob's class (even though
Mary is teaching more students than Bob).
So, here is how we do our test: We throw all
35 scores into a pot, stir the pot energetically,
pull out 20 in one bowl
for Mary and put the other 15 scores into a bowl
for Bob. Then we average the scores in each
bowl and take the difference in the averages,
say, Mary's average minus Bob's average.
Then we repeat this many times -- for this
might want to use a computer with a good
random number generator. This process is sometimes
called 'resampling'. It's also possible to
argue that what is going on is a finite group
of measure preserving transformations that, thus,
can yield what we are doing more intuitively.
Physicists like symmetries that result in
conservation laws, but here we have symmetries
resulting in an hypothesis tests.
So, we get the empirical distribution
of the differences in the averages.
Then we look at the difference in the actual
averages, that is, from the actual students
of Mary and Bob. Call this difference
X. Now we see where X is in the empirical
distribution of differences we found.
If X is out in the tails with probability,
say, 1%, then either (A) Mary and Bob
are equally good as teachers, that is, we
accept the null hypothesis, and we have
observed something that should happen
1% of the time or less or (B) Mary and Bob
are not equally good as teachers and
we reject the null hypothesis and
conclude that there is a difference
in teaching between Mary and Bob.
If the 1% is too small to believe in,
then we accept (B) and pop a Champaign
cork for the better teacher.
Here we made no assumptions at all about the
probability distributions of the scores.
So, our hypothesis test does not assume
a distribution and is distribution free
or, as is sometimes said, non-parametric
(because we did not assume a distribution,
say, Gaussian with parameters, e.g.,
mean and variance).
Look, Ma, no standard deviations!
The 1% is he significance level of our
hypothesis test and is the probability of
rejecting the null hypothesis when it is
true and, thus, is the probability of Type I
error.
Oh, consider a large server farm or network.
Suppose we identify 10,000 systems we want
to monitor for health and wellness and detect
problems never seen before. Suppose from
one of the 10,000 systems, we consider one.
Suppose from this system we receive data
100 times a second on each of 12 numerical
variables.
Suppose the server farm is supposed to be fairly
stable and we collect such data for, say,
3 months. Call this history data. Maybe
the machine learning people would call this
training data. Whatever.
Now we can construct a 12 dimensional, distribution-free
hypothesis test where the null hypothesis is
that the system is healthy and also select
our false alarm rate (probability of Type I error)
in small steps over a wide range. So, we have
a multi-dimensional, distribution-free hypothesis
test. Such are rare, but, really now we have
a large class of them. Yes, we use a group of measure preserving
transformations.
As I recall, back in 1999 there was a paper on
such things in Information Sciences.
I wouldn't call that paper machine learning,
but maybe some people would. Some of what is
interesting in the paper is how the heck to
know and adjust the false alarm rate, that is,
the probability of Type I error.
Again, look, Ma, no standard deviations or
Gaussian assumptions.
Good luck acquiring the universally accepted numerical value without applying a Gaussian distribution as shown.
Remember that this thread began with someone nontechnical asking what the significance of 5σ was to the evaluation of a physics experiment, for which I provided an uncontroversial explanation in that context.
> And the standard deviation is a number, just a number, just as I defined it as σ = E[(X - E[X])^2]^(1/2) which clearly is just a number and not an area.
Yes, and if I graph a function in terms of X and Y, where X is a function's argument and Y is the value returned by a particular function, one can argue that X and Y are just placeholders for numbers without any intrinsic meaning by themselves.
If I then say that Y represents the sine of X, surely someone will say, as you have said, "No, not at all, X is just a placeholder for a number, it's not what you say. And Y is just a placeholder for a number, it's not tied to any particular function."
In point of fact, the standard deviation is more than a particular number, it's an idea, and its statistical purpose is met when it's associated with a context in which that idea is expressed. That context is the normal distribution. In the present context, a particular sigma value refers to a specific area under a normal distribution, and in turn, to the probability that a particular result might have arisen by chance.
Without reference to a normal distribution, a standard deviation (a sigma) loses its conventional meaning. Variances are acquired by statistical tests of data sets, standard deviations (sigmas) are acquired from variances, and conclusions are drawn from sigmas only to the degree that they are applied to normal distributions.
Quote: "In statistics, the 68–95–99.7 rule, also known as the three-sigma rule or empirical rule, states that nearly all values lie within three standard deviations of the mean in a normal distribution.
About 68.27% of the values lie within one standard deviation of the mean. Similarly, about 95.45% of the values lie within two standard deviations of the mean. Nearly all (99.73%) of the values lie within three standard deviations of the mean."
According to your thesis, the above claim is obvious nonsense, because in point of fact, sigma has no association with the normal distribution. But you know what? Wikipedia can be edited by anyone, and you can correct this egregious error today, if you like. Correct this widespread erroneous thinking -- fix these errors, everywhere you find them.
Let's perform a little test. Let's submit "5 sigma" to Wolfram Alpha and see whether it makes the same mistake you say I have been making, and that the above linked article is making:
So it seems that, without prompting, Wolfram Alpha draws the same conclusion that Wikipedia does, and every other online reference does when confronted by terms such as "standard deviation" or "sigma" -- that, without providing a specific context, the default context is that sigmas refer to positions on a standard distribution and have statistical meanings associated with that default assumption.
> Of course, even with a Gaussian assumption, standard deviation does not have a particular numerical value.
When a scientist uses the term "5 sigma", she is in most cases using a context of a normalized normal distribution, one that follows the 68-95-99.7 rule described above. Therefore yes, 5 sigma does lead to a a particular value, by being applied to a definite integral of a normalized normal distribution that uses it as an argument. By this reasoning, 5 sigma means:
Which is correct, and is the expected one-tailed value for 5 sigma, even though according to your argument, 5 sigma has no connection to normal distributions.
> Sorry 'bout that.
What, for your specious argument? No problem, it comes with the territory. But surely you realize I have more than answered your objection.
No. Here is an important use of standard deviation
not related at all to the Gaussian distribution:
The set of all real valued random variables
that have a standard deviation and one that is
finite form a Hilbert space. The crucial part of
the argument is completeness. Of course we like to
use Hilbert space for projections and converging
sequences, so it's super nice that those random
variables form a Hilbert space.
> No. Here is an important use of standard deviation not related at all to the Gaussian distribution ...
Before you troll through the world's imaginary problems again, I am going to ask you one more time to remember how this conversation got started (the context), and why I answered as I did.
Someone nontechnical asked what the significance of 5σ was in the context of a physics experiment. I replied by saying that 5σ was mapped to a p-value this way:
And the p-value was the point, leading to a discussion of the high level of discipline in experimental physics compared, say, to the social sciences, which accept p-values of .01-.05, values I included in my original reply for comparison.
The context is the normal distribution. Wake up and smell the Cappuccino.
Maybe this will clear it up for you: That the
physicists are making a normal distribution
assumption is from shaky down to sloppy down
to silly down to
absurd. Making this assumption for
experimental data, e.g., the LHC data or
the gravitational wave data, where they are
hanging on by their fingernails anyway, is
close to treating the normal distribution as
some gift from God.
And, if some field makes a normal, or
mean 0, variance 1 normal, assumption, then
they should say so and, hopefully, justify
that assumption.
Your examples from Wolfram and Wikipedia
show that a lot of people have
guzzled that old Kool Aid on the normal
distribution. A few years ago I had a
date with a high school teacher, and she
assumed that test scores are normal.
My father had an MS in education and my
brother was a ugrad psych major, so,
when my brother's psych material got to
statistics, Dad taught him about
the normal distribution. It appears that
around 1900 and then for 80 years or so,
and still in some parts of some fields,
a normal assumption, without mention
or justification, was common and
remains in what you call the "context".
"Context" or
not, common or not, popular or not,
it's still an assumption, needs mention
and justification, and usually is not
at all well justified or justifiable.
Sure, with their normal assumption and, say,
five sigma, experimental physicists
get particular probabilities of Type I error,
so called p values. No question here.
The issue is the normal assumption.
There are places where a normal assumption
is quite solid. The most common justification
is from the central limit theorem. So,
take random variables
X(1), X(2), ... and assume that they
are independent and all have the
same distribution with
finite
standard deviation. Then the central
limit theorem says essentially that
as
positive integer n grows to infinity
the distribution of the sum
X(1) + ... + X(n)
will converge to normal (really should divide
the sum by square root of n).
So, where might we get some such
X(1) + ... + X(n)?
Sure, from Brownian motion where
there are many little bumps
and the bumps come close enough to
satisfying the hypothesis. So
can use this also in thermodynamics.
So, there are places where a normal
assumption is justified.
But just making a normal assumption
for essentially all experimental errors
as needed for the accepted five sigma
criterion is close to a weird religion
and not flattering to a modern science.
What physics is doing with their
five sigma criterion is a statistical
hypothesis test.
My examples of distribution free hypothesis
tests via resampling is a
better justified and more
conservative and robust way to do
an hypothesis test. Physicists might
consider using such.
Such distribution-free statistical methods
form a large field.
My example of the role of
Hilbert space is quite
practical.
If you want to explain to the common
man in the street why physics likes
their five sigma criterion, then,
sure, you need the normal assumption.
Then you should mention that there
physics is making a normal assumption.
There you might not confuse the common
man in the street with a claim that
in making this normal assumption physics
is close to drinking some swill of
boiled tails of rats and bats.
But with the now high interest in
computer science of big data,
machine learning, etc. I was
assuming that the HN audience could
and should hear the real stuff --
that in what physics is doing,
there's a normal (Gaussian) assumption
in there.
Are you sure? I'm pretty confident in this case the assumption is that the distribution is normal. With no knowledge of the shape of distribution, the 5 sigma bound is extremely weak (one given by Chebyshev's inequality [0], in this case, ~4%). Prove me wrong though, as I'm not a physicist or mathematician.
No, I think you're wrong. See my comment above. Note that nowhere in the article you link does it say there's an assumption of normality. Doubtless the journalist or whoever chose the picture of th normal distribution was a bit confused also.
Edit: oh, no, actually I think you're right :). I thought it was referring to the location of the test statistic in its null distribution. But it seems it's a scale for measuring p-values. This explains it clearly:
What does "five sigma" mean? It means that the results would occur by chance alone as rarely as a value sampled from a Gaussian distribution would be five standard deviations from the mean.
All that aside, remember that the context is a nontechnical person asking what 5σ means in statistical analysis in physics. That greatly narrows the possible interpretations.
By the way, this same conversation took place after the LHC Higgs anouncement -- the same five-sigma standard for discovery, and the same detailed discussion of what that means.
> But it seems it's a scale for measuring p-values.
Yes, and that was a point I made in my reply to the OP -- that the context assumed an association with p-values, which in turn assume a normal distribution.
Sorry, I'm either not understanding or I still am not convinced you are correct. p-values don't assume a normal distribution. A p-value is the probability of generating an equal or more extreme value of your test statistic under the null hypothesis. Normal distributions are nowhere in sight.
The only way that the Normal distribution comes into play is that physicists are measuring the smallness of their p-values by stating a number of standard deviations from the Normal mean that would have the same p-value.
I'm finding this discussion helpful by the way. I have worked in applied statistics but not in any fields which use this "sigma" scale or would talk about "sigma values".
No, not unless a p-value is expressed in terms of sigma as in this case and similar ones. In this case, and commonly in experimental physics, there's a relationship between n-sigma (usually 3σ or 5σ in different circumstances) and how a p-value is acquired from a sigma expression. The p-value is acquired from a sigma value like this:
My point? In experimental physics there's a connection between (a) an expression including an integer and "sigma", (b) a resulting, widely quoted numerical value, and (c) the method for converting one to the other, using a Gaussian distribution as shown.
Quote: "But what does a 5-sigma result mean, and why do particle physicists use this as a benchmark for discoveries?
To answer these questions, we'll have to look at one of the statistician's oldest friends and C-student's worst enemies: the normal distribution or bell curve."
Couldn't have said it better myself.
> The only way that the Normal distribution comes into play is that physicists are measuring the smallness of their p-values by stating a number of standard deviations from the Normal mean that would have the same p-value.
Hmm. Yes, that's right. That's why I replied as I did in my original post.
It's correct that a normal distribution is assumed in physics, but you are not correct that a standard deviation is defined in terms of a normal distribution.
The present conversation got started by someone non-technical asking what 5 sigma meant in a physics context. Within that context, and with the intent to avoid exotic digressions, my reply is correct.
In physics, a sigma value maps to a p-value, and that relationship is most often defined with respect to a normal distribution. Therefore, in most cases, to go from a sigma value to a p-value, one performs this integral:
Specifically, the above definite integral, when performed with arguments of 5 and +oo, yields the often-quoted one-tailed p-value for "5 sigma", which we can get here as well:
It seems Wolfram Alpha makes the same default assumption I do: a normal distribution. If I weren't answering an inquiry from someone who wanted the clearest possible answer, I might have replied differently.
But it appears that you are correct that
that part of physics makes some Gaussian
assumptions and, then, has some conventions
based on those assumptions. In this case,
apparently physics is not making its
mathematical assumptions clear and explicit
and is doing sloppy writing. For more
detail, see my longer explanation in
this thread
Maybe the situation is a little like
getting from a little French restaurant
the recipe for French salad
dressing, sauce vinaigrette, making
it at home, and concluding it tasted
better in the little French restaurant.
Hmm .... But the French restaurant
did something not in the recipe --
took a large clove of garlic, peeled it,
cut it in half, and wiped the salad bowl
with the cut surface of the garlic!
The recipe didn't mention that!
I don't think those physicists are making any Gaussian assumptions, right? They're computing a p-value as normal (how often would my test statistic generated under the null be more extreme than observed), and then using the Gaussian distribution as a scale to communicate how small their p-value is.
They are definitely making a Gaussian assumption, and wouldn't feel the need to clarify that as it's a widely accepted convention in the field. In your restaurant analogy, it's like you overheard two chefs talking.
> The poster he was responding to made an idiotic statement:
> "In statistics, σ refers to an area under the normal distribution defined in terms of standard deviations (1σ = 1 standard deviation)."
Not only is that not idiotic, that's the default definition in a statistical context (see below). Anyone can argue that σ is just another Greek letter with no special significance, but that require one to ignore the context in which the term is used.
Quote: "In statistics and probability theory, the standard deviation (SD) (represented by the Greek letter sigma, σ) shows how much variation or dispersion from the average exists."
> He was just stating that the standard deviation is a general concept of spread, that any distribution has, and not just the normal one.
Again, this disregards context. When nontechnical people ask what the significance of 5σ is to scientific statistical analysis in physics (which is how this thread got started), there is precisely one answer.
* "In statistics, σ refers to an area under the normal distribution defined in terms of standard deviations*
that's the default definition in a statistical context
No, you're quite wrong about that. greycat is correct in his/her corrections of what you're saying. In statistics sigma is used to represent one of two things:
- a parameter of a probability distribution, typically one which influences the spread of the distribution
- a measure of dispersion in an actual data set, which may be an estimator of a parameter in a probability distribution
Neither of those things necessarily involve the Gaussian density.
In physics it seems that "sigma values" are used as a scale to measure p-values, so that instead of saying 0.0000003, they can just say 5σ. But the critical point here, which your comments seem to be missing, is that there is no distributional assumption being made; there is no implication that the Normal distribution describes any data-generating process, merely that the probability of an equal or more extreme value of a test statistic under some model, is the same as the probability of observing a value more than 5 standard deviations from the mean under a Gaussian model.
>> * "In statistics, σ refers to an area under the normal distribution defined in terms of standard deviations* that's the default definition in a statistical context
> No, you're quite wrong about that.
It is the default, actually. There are plenty of exceptions to the default, but it certainly is common in the context of experimental physics, the present context.
Quote: "But what does a 5-sigma result mean, and why do particle physicists use this as a benchmark for discoveries?
To answer these questions, we'll have to look at one of the statistician's oldest friends and C-student's worst enemies: the normal distribution or bell curve."
> ... your comments seem to be missing, is that there is no distributional assumption being made ...
Do read some experimental physics -- see what assumptions are made. Here is how a physicist maps a sigma value to a p-value:
> Do read some experimental physics -- see what assumptions are made.
lutusp, the way in which you are using the word "assumption" carries a very high risk that people will misunderstand you. The critical point here is that the physicists are nowhere using the Normal distribution as a modeling assumption. They are not suggesting that the Normal distribution is a reasonable model for any real data generating process in their problem domain. They are simply using it as a scale, like Celsius of Fahrenheit. There's a crucial philosophical distinction there that, even if you get, your readers will not.
In statistics, σ refers to an area under the normal distribution defined in terms of standard deviations (1σ = 1 standard deviation).
In statistics and probability theory, the standard deviation (SD) (represented by the Greek letter sigma, σ) shows how much variation or dispersion from the average exists.
If the unit normal distribution is the distribution under discussion, there's no difference. In that case they become the same. Here's how a physicist computes a p-value given a sigma value:
> The probability that it arose from chance is equal to or less than 5σ
That's not what p value means. The p value is the probability that a high-variance random effect (centered around an average behavior of "nothing interesting") would yield a result as extreme as the observation, assuming that random distribution. You need Bayes theorem and highly subjective assumptons if you want to derive a posterior probability that an observed result was drawn by chance from a sample with a boring/interesting mean.
"Particle physics uses a standard of "5 sigma" for the declaration of a discovery. At five-sigma there is only one chance in nearly two million that a random fluctuation would yield the result. This level of certainty prompted the announcement that a particle consistent with the Higgs boson has been discovered in two independent experiments at CERN."
"When the uncertainty represents the standard error of the measurement, then about 68.2% of the time, the true value of the measured quantity falls within the stated uncertainty range. For example, it is likely that for 31.8% of the atomic mass values given on the list of elements by atomic mass, the true value lies outside of the stated range. If the width of the interval is doubled, then probably only 4.6% of the true values lie outside the doubled interval, and if the width is tripled, probably only 0.3% lie outside. These values follow from the properties of the normal distribution, and they apply only if the measurement process produces normally distributed errors. In that case, the quoted standard errors are easily converted to 68.3% ("one sigma"), 95.4% ("two sigma"), or 99.7% ("three sigma") confidence intervals."
"It's 5σ at .2"
His wife, also a theoretical physicist - blank stare "Discovery?" - immediately melts into a hug.
What a great thing, to be able to see the human side, makes you all warm and fuzzy for human progress.