A probability density function must be nonnegative and have definite integral one. Here
Therefore
This value is positive, so the nonnegativity requirement also holds.
The cosine function is positive on and negative on . Thus any nonzero makes negative on an interval of positive length. Taking makes the total definite integral zero. Hence
Normalization alone would suggest , but that candidate still violates nonnegativity and therefore is not a probability density function.
We need . Indeed, if , the function is negative on ; if , the improper integral diverges at zero; and if , its support interval is empty. For ,
Setting this equal to one gives the unique admissible value
On this interval , so both requirements for a probability density function are met.
Since is nonnegative, for . For , use to obtain
Thus the cumulative distribution function is
In particular it tends to one as , confirming normalization of this unit-scale Rayleigh distribution.
The cumulative distribution function is continuous and strictly increasing for , so the median is the unique positive satisfying . Consequently , giving
There is no atom at , so as required.
Since , the function is strictly increasing on its support. For ,
and for . Differentiating the cumulative distribution function gives
The density value at the single point is immaterial. Hence has an exponential distribution with rate . Direct integration by parts, or its standard expected value, yields
By the density formula for expected value,
For the standard normal distribution, the integrand in the second moment is even, so
Comparing these two integrals gives
The standard normal distribution has mean zero and variance one, so . Part (iv) therefore gives
Using the second moment from part (iii),

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