Alltimegreat1 said:
More common than real brains or more probable do you mean?
As in the number of Boltzmann Brains > the number of real brains. If a model predicts that, then it can't be right.
This argument originally came up with the simple model of the universe as a thermal fluctuation out of equilibrium. The idea there is that when a system is at equilibrium, there are random deviations from that equilibrium. Here you might imagine the universe as a giant box. Within this box, most every time you look, there will be nothing but empty space. But every once in a while, a random drop in entropy will produce something.
The problem with this is that small drops in entropy are exponentially more common than large drops in entropy. So if you only look at the box those times that there is, say, a galaxy in the box, nearly every time there will be only a single galaxy. Two galaxies will be absurdly rare compared to just one galaxy.
Similarly, a single star system will be far, far more common than having two star systems, let alone three or an entire galaxy of stars.
A single planet, one that is temporarily at a high enough temperature to support life, will be far more common still. A single person that imagines observing an external universe will be even more common than a whole planet. Just a disembodied brain that thinks it exists will be the most common thing that thinks it exists.
You might say, "But brains and galaxies don't just pop out of nothing: they form from matter that was around earlier." But that just pushes the problem back: the entropy was always lower in the past. It's harder to form the early universe from a thermal fluctuation than it is to form the present universe!
This line of reasoning shows that there had to be something special about the early, low-entropy state of our universe. There's a fair amount of theorists who are working on possible solutions to this problem. Currently there are a lot of models that avoid this problem, but we don't yet know which (if any) of them are correct.