So if people come around and say, yes, they see the same signal we do, and I don’t see why they can’t do that. 0:51:21 SC: Wait, sorry, I think maybe we skipped a step, or I just wasn’t paying close attention, but you’ve been explaining the future, and it has a certain nice remarkable mathematical properties.
But the thing is, if you have combinations of lenses. 0:14:44 RP: No, you’re absolutely right. Initially, there were just the odd double star system, where you would see one star and other one, it seems to be going around something else that you couldn’t see. Just that it potentially was possible. Well, I think there was an argument about it. But it’s only protoconscious, it doesn’t relate it to anything else and doesn’t have any purpose, it’s… It just does it.
And the question is why, what’s the difference?
And so it’s a point of view, that experience… So you say, there’s a sort of… There are many, many element of experience every time these reductions take place. 0:21:30 SC: And then, I mean on the theoretical side, black holes became a whole area of study, and Stephen Hawking and Brandon Carter and other people… ( You can do this just with ordinary optics. So, it looks quite a sizeable thing, but pretty small on the basis of looking at the whole sky.
So where is it low? 0:12:41 SC: Right. Well, the lifetime…. 0:22:49 SC: Although you see, except it’s not that big, it’s a small, compact heavy thing you can’t see. Do you think that this way of thinking about Quantum wave function collapse in the brain would help us understand the process of experience? But anyway, yeah, you got this huge amount of entropy in the radiation, which was a lot actually.
[chuckle] And therefore, you had this huge amount of energy coming out which is something like more than the whole galaxy. 0:59:08 RP: You see, this is the same, more or less the same team, the Polish team with Daniel An, and they were doing a slightly more sophisticated analysis, which came from a discussion I had with Krzysztof Meissner.
0:41:14 RP: Well, you can think of it as energy, people call it dark energy, yes, yes. But now suppose you pull them apart. I think it’s just as well I didn’t hear his explanation, because it might have calmed me down, but instead I’ve worried about this for ever since. 0:28:44 RP: But then he found that they did.
Unlike any other theory ever in physics. Well, you think… Go think about the Escher picture again, you see, you have an event which is taking place right up near the edge of that boundary and that means all the radiation which comes out is concentrated right at one little point.
They found an extremely good fit, an almost perfect fit to the Planck spectrum. Now, what’s the earliest evidence that we directly see of the universe? 1:04:44 SC: And we’ll see what comes out of that. Now, is it according to following some specific logical system? 0:44:07 RP: “You have to take it seriously.” So I thought, Okay, I’ll take it seriously.” [chuckle] And it wasn’t, I don’t know how long after that conversation, that I began to think about the remote future.
[chuckle] Some people think the hard problem is impossible, some people think it’s easy but everyone thinks the easy problems are hard.
1:05:12 RP: Oh, yeah. c Or something like that. So that’s the picture that a lot of people had.
[chuckle] And there were people talking about very massive stars, and so on, and I asked to give a talk on black holes. You’re the one who’s gotta make the decision about what to think at the end of the day. And yeah, people studied… I studied it, I studied and looked to see what the infinity looked like in this model, and so on. And that will be gravitational radiation, primarily likely LIGO detection of the black holes that we’ve seen, and very proud of. It could be like the Fermat’s Last Theorem that Andrew Wiles famously proved, or it could be the Goldbach conjecture, which nobody has proved yet, if it’s true. I remember talking to him about this and I was sort of thinking it was real you see. I mean, I couldn’t think of anything more boring than that. And it’s in danger of people who might say, “Well, that’s flaky. Roger Penrose (1964)
1:03:45 RP: So only at the very end would you get something which is restricted to this four degrees across the sky, and we don’t see the signal bigger than that.
It probably wasn’t terribly persuasive, but there was some indication, but not enough to rule out a model rule out a model like Einstein and the one he produced then. 1:05:37 SC: Quantum mechanics has this weird feature that there seems to be a thing that we need to include in the description that is, what happens when you look at something?
Well, he was troubled with it, you can see because he put forward this ridiculous situation of the cat, which is the superposition of alive and dead, as an example of the absurdity of following his own equation.
1:05:27 SC: If that’s okay. I’ve wondered a little bit, although I haven’t sat down and gone through the equations, but in Everett, we talk about wave functions branching because of de-coherence, because a system interacts with an environment, and one way… And there’s a big challenge in quantum computing to prevent systems from acting and reacting with the environment so that you can maintain quantum coherence. Well, yeah, same issue about their discreteness but that’s not probably the real point.
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