In the above pdf, we address the following issue.
Consider the canonical embedding of . It is easy to see that no sub-sequence of
can weak-star converge, yet Banach-Alaoglu asserts that the unit ball of
is weak-star compact. So what is the problem?
This is the result of several discussions with Chris Gartland who explained to me a large portion of what is in the file.
Is this because
is not weak-
metrizable? So Compactness does not imply sequential compactness
Nice Amir, that’s precisely the issue.