Goals of Today's Lecture:
Review of end of last time
I defined independent events and then independent random variables:
Def'n: Ai,
independent:
Def'n: Rvs
independent:
Theorem:
Proof:
Theorem: If
are independent and
Yi =gi(Xi) then
are independent.
Moreover,
and
are
independent.
Def'n:
P(A|B) = P(AB)/P(B) if
.
Def'n: For discrete X and Y the conditional
probability mass function of Y given X is
For absolutely continuous X
P(X=x) = 0 for all
x. What is P(A| X=x) or
fY|X(y|x)?
Solution: use limit
Def'n:
iff
Def'n:
iff
(a column vector for later use) with the
Zi independent and each
.
In this case according to our theorem
superscript t denotes matrix transpose.
Def'n:
has a multivariate normal distribution if it
has the same distribution as
for some
,
some
matrix of constants A and
.
If the matrix A is singular then X will not have a density. If A is
invertible then we can derive the multivariate normal density
by the change of variables formula:
For which vectors
and matrices
is this a density?
Any
but if
then
where y=At x. Inequality strict except for y=0 which
is equivalent to x=0. Thus
is a positive definite symmetric
matrix. Conversely, if
is a positive definite symmetric matrix
then there is a square invertible matrix A such that
so that
there is a
distribution. (A can be found
via the Cholesky decomposition, e.g.)
More generally X has multivariate normal distribution
if it has the same distribution as
(no
restriction that A be non-singular). When A is singular X will not
have a density:
such that
;
X is confined to a hyperplane. Still
true that the distribution of X depends only on the matrix
:
if
AAt = BBt then
and
have the same distribution.
Properties of the MVN distribution
1: All margins are multivariate normal: if
2: All conditionals are normal: the conditional distribution of X1given X2=x2 is
3:
:
affine
transformation of MVN is normal.
Theorem:
Suppose
are independent
random
variables.
Then
Proof: Let
.
Then
are
independent N(0,1) so
is multivariate
standard normal. Note that
and
Thus
So: reduced to
and
.
Step 1: Define
Solve for Z from Y:
Zi = n-1/2Y1+Yi+1for
.
Use the identity
Now we use the change of variables formula to compute the density
of Y. Let
denote vector whose
entries are
.
Note that
Note: ftn of y1 times a
ftn of
.
Thus
is independent of
.
Since sZ2 is a function of
we see that
and
sZ2 are independent.
Also, density of Y1 is a multiple of the function of y1 in
the factorization above. But factor is standard normal
density so
.
First 2 parts done. Third part is
a homework exercise. Derivation of the
density:
Suppose
are independent N(0,1). Define
distribution to be that of
.
Define angles
by
(Spherical co-ordinates in n dimensions. The
values run
from 0 to
except last
from 0 to
.)
Derivative formulas:
Fourth part is consequence of
first 3 parts and def'n of
distribution, namely,
if it has same distribution
as
Derive density of T in this definition:
Differentiate wrt t by
differentiating inner integral: