WEBVTT - Making Waves with Gravitational Astronomy

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<v Speaker 1>Brought to you by Toyota. Let's go places. Welcome to

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<v Speaker 1>Forward Thinking. Hey there, and welcomed up Forward Thinking, the

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<v Speaker 1>podcast that looks at the future and said, we're waxing

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<v Speaker 1>down our surfboards. We can't wait for June. I'm Jonathan

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<v Speaker 1>Strickland and I'm Joe McCormick. And today is going to

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<v Speaker 1>be Is it gonna be? What do we call it?

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<v Speaker 1>Part two? It's at least going to be a follow

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<v Speaker 1>up to our most recent podcast, the one that came

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<v Speaker 1>out right before this, which was about the discovery of

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<v Speaker 1>gravitational waves at the Ligo facilities in September. Yes, and

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<v Speaker 1>so in that last episode we talked about how the

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<v Speaker 1>discovery happened, what gravitational waves are, and how they were

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<v Speaker 1>eventually found. But in this episode, we wanted to talk

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<v Speaker 1>about what it all means now that we have found

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<v Speaker 1>and confirmed the existence of gravitational waves in our universe. Yeah,

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<v Speaker 1>so let's let's talk a little bit about some more

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<v Speaker 1>specifics about Ligo and also what this is going to

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<v Speaker 1>You know, how we see this unfolding doesn't have any

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<v Speaker 1>practical impact on your life as a what I am

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<v Speaker 1>assuming is a normal human being out there you might

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<v Speaker 1>be a crawfish monster. You could be. We talked a

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<v Speaker 1>lot about those in their last episode two. I'm not

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<v Speaker 1>going to judge either way, but I do either way

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<v Speaker 1>want to tell you about some cool things about LIGO,

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<v Speaker 1>and that's that well, and in the discovery process in general.

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<v Speaker 1>So you know, even though like three dudes started this

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<v Speaker 1>whole crazy ride back in the paper that announced the discovery,

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<v Speaker 1>which is titled by the way, Observation of Gravitational Waves

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<v Speaker 1>from a Binary black Hole Merger has over a thousand

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<v Speaker 1>authors scientific cooperation, y'all. Just that's so cool. It's very

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<v Speaker 1>inspirational to see. And you know, like we mentioned before

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<v Speaker 1>the fact that LIGO had to had to go through

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<v Speaker 1>an upgrade process from fifteen and that was an international

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<v Speaker 1>collaboration also really inspiring. Yeah. Yeah, And and now that

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<v Speaker 1>LGO is is working in this way, researchers expected to

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<v Speaker 1>make tens of observations every year. And usually when you

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<v Speaker 1>say tens of tens of anything, you're kind of making

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<v Speaker 1>fun of it. But in this case, that's really cool

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<v Speaker 1>because it will give us so much more data to

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<v Speaker 1>work with. And again, you know, we're talking about events

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<v Speaker 1>that are happening billions of years ago. So uh, it's

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<v Speaker 1>it's stuff that like, you know, if if it happened

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<v Speaker 1>a billion years ago, but the event was four billion

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<v Speaker 1>light years away, there's no way for us to detect

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<v Speaker 1>it because gravitational waves are limited, as is everything else

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<v Speaker 1>by the speed of light. They can only travel as

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<v Speaker 1>fast as the speed of light. Maybe not everything else,

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<v Speaker 1>Maybe not the expansion of space during inflation. Well that's different.

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<v Speaker 1>That's different. That's that's the universe itself, not stuff within

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<v Speaker 1>the universe. I admitted, I got you, Jonathan. I admit

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<v Speaker 1>nothing except that I did accidentally say gravity waves in

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<v Speaker 1>the last episode SI gravitational waves. I will admit that

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<v Speaker 1>it's on tape. Okay, okay, But back to what it

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<v Speaker 1>all means. So we have discovered gravitational waves that with

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<v Speaker 1>the Lego facility, we hope to discover many more and

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<v Speaker 1>and learn more about them all the time. But what

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<v Speaker 1>does this all mean for the state of physics today? Well, first,

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<v Speaker 1>it is yet another piece of evidence that supports Einstein's

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<v Speaker 1>theory of general relativity. So darn and I hate Einstein

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<v Speaker 1>being right all the time. Props to you, Mr Einstein.

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<v Speaker 1>I want him to crash and burn someday. Well he's dead,

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<v Speaker 1>so he got that going, I mean his theories. I

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<v Speaker 1>want us to discover that in fact, Newton was right.

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<v Speaker 1>I mean his brain was stolen for a while. So

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<v Speaker 1>there's that too. Yeah, yeah, you're you're already two up

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<v Speaker 1>on Einstein. Your brain is exactly where it's supposed to

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<v Speaker 1>be in yours. It was his eyeballs too, wouldn't it,

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<v Speaker 1>I think? So, yeah, yeah it was. That's a lacky

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<v Speaker 1>story for another time at any rate. Uh So, it

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<v Speaker 1>doesn't mean that the general theory of relativity is going

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<v Speaker 1>to become a scientific law, that's friend. But it does

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<v Speaker 1>support yet more predictions that were made from general relativity.

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<v Speaker 1>So if you say, if general relativity is correct, then

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<v Speaker 1>we would expect X. This was one of those X

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<v Speaker 1>things that we would expect, and in fact, we've now

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<v Speaker 1>discovered it that we've we've found that the evidence of it,

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<v Speaker 1>we can say, yes, this is definitely correct, which is phenomenal.

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<v Speaker 1>Right that that yet, again we've seen how general relativity

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<v Speaker 1>matches up with reality as we see it, as we

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<v Speaker 1>can observe it. Now, that doesn't mean that general relativity

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<v Speaker 1>is going to be absolutely all encompassing. There's still big

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<v Speaker 1>gaps for us to fill in. How about the quantum

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<v Speaker 1>level exactly. But it is really an awesome display of

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<v Speaker 1>Einstein's ability to suss things out to a level that

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<v Speaker 1>is almost inhuman as far as I'm concerned, Like, it's

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<v Speaker 1>so amazing to me that he can make these actions

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<v Speaker 1>that he had absolutely no way of testing. And then

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<v Speaker 1>a hundred years later we get the news that, yeah, no,

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<v Speaker 1>he was totally right about that. Well, they did eventually

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<v Speaker 1>have ways of testing the predictions of general relativity. But yeah,

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<v Speaker 1>what you're you're correct about is that Einstein didn't have

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<v Speaker 1>a test that he used to come up with general relativity.

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<v Speaker 1>You're correct. I was specifically thinking about the prediction of

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<v Speaker 1>gravitational waves that there was no way for him to

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<v Speaker 1>test for that. There were certainly ways to test for

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<v Speaker 1>other elements of general relativity, but the specific prediction of

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<v Speaker 1>gravitational waves that was something that they could not easily

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<v Speaker 1>test for. Back in nineteen sixteen when he published the theory,

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<v Speaker 1>other things that were becoming more sure about as a

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<v Speaker 1>result of this black holes, black holes. Yeah, so finally

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<v Speaker 1>we're we've got, like I mentioned in the previous episode,

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<v Speaker 1>the strongest evidence so far for the existence of black holes.

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<v Speaker 1>I think by and large the astronomy and astrophysics community

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<v Speaker 1>was convinced of the existence of black holes already, but

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<v Speaker 1>this is another really good piece of evidence for them. Well,

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<v Speaker 1>they were also convinced of the existence of gravitational waves.

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<v Speaker 1>But again it's one of those things where you say,

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<v Speaker 1>this evidence is yet more support for this thing that

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<v Speaker 1>we cannot directly observe, right so uh. And and furthermore,

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<v Speaker 1>that that black holes can exist in binary systems. Yes,

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<v Speaker 1>that you can get two black holes orbiting one another

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<v Speaker 1>and then coalescing into a a single black hole while

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<v Speaker 1>vaporizing three solar masses worth of material, which again still

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<v Speaker 1>blows my mind. Um. Beyond that, we also are are

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<v Speaker 1>now able to track celestial objects that don't emit visible

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<v Speaker 1>light or any electromagnetic radiation at all, as long as

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<v Speaker 1>they are massive enough, if the event that they are

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<v Speaker 1>undergoing is violent enough to generate gravitational waves, clearly, if

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<v Speaker 1>they're if they're small, if the gravitational waves are very

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<v Speaker 1>tiny and weak and really far away so that by

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<v Speaker 1>the time they get here, they're they're so weak as

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<v Speaker 1>to be under textable, that's not gonna the Lego is

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<v Speaker 1>not gonna make any difference in that. But for stuff

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<v Speaker 1>that we cannot see but does create significant gravitational waves,

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<v Speaker 1>now we have a way of detecting that, and that

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<v Speaker 1>that means that we're going to get information about stuff

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<v Speaker 1>that we know about but haven't been able to directly observe,

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<v Speaker 1>and potentially find out about stuff we didn't even know existed,

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<v Speaker 1>Like we literally had no clue because there was no

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<v Speaker 1>way to observe it. Now we've got a new way

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<v Speaker 1>to Yeah. I've read quotes from a couple of different

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<v Speaker 1>scientists involved with this project who have compared the ligo

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<v Speaker 1>method to essentially gaining a new sense for a person.

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<v Speaker 1>One example I want to quote is from Miriam Kramer's

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<v Speaker 1>piece on mash Double about gravitational waves, where she interviewed

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<v Speaker 1>the LEGO scientists Subull Schmarka who explained it this way quote,

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<v Speaker 1>Imagine that you have all of your senses, but you

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<v Speaker 1>can't year and the first day you gain hearing, you

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<v Speaker 1>get a new life. Imagine how your life would change

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<v Speaker 1>if you can actually observe since your surroundings in a

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<v Speaker 1>very different way. This is what we actually gain with

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<v Speaker 1>gravitational waves. And another one along the same lines was

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<v Speaker 1>David Rights to Physics World. He said, we have been deaf,

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<v Speaker 1>but now we can hear them. We now expect to

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<v Speaker 1>hear things we never expected as we opened a new

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<v Speaker 1>window of astronomy. This was a scientific moon shot, and

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<v Speaker 1>we did it. We landed on the moon. Yeah. And

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<v Speaker 1>I've seen that analogy of being able to listen to

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<v Speaker 1>the universe and hear what was going on in the universe.

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<v Speaker 1>I've seen that over and over from multiple people who

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<v Speaker 1>worked on this project and other physicists who didn't work

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<v Speaker 1>directly on the project but are obviously very much interested

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<v Speaker 1>and invested in its outcome. And that particular phrase, you know,

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<v Speaker 1>listening or hearing what is going on, has been used

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<v Speaker 1>multiple times, and I think it is a very elegant

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<v Speaker 1>way of putting it. This side. Yeah, and again it

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<v Speaker 1>kind of uh compares gravitational waves to sound waves. This

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<v Speaker 1>idea of this thing propagating out through the universe, but

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<v Speaker 1>at the speed of light and passing through everything it encounters.

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<v Speaker 1>It's not blocked by other bodies, so it will eventually

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<v Speaker 1>make its way throughout the universe, maybe not strong enough

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<v Speaker 1>for us to detect, but it will come to us

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<v Speaker 1>at some point. Uh. And it means that we're gonna

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<v Speaker 1>be able to study lots of stuff much more um

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<v Speaker 1>intricately than we could before, things like supernova explosions and

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<v Speaker 1>neutron stars and more information about black holes and learn

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<v Speaker 1>you know, all there is to learn that we can

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<v Speaker 1>so far. Uh, it expands that that possibility. Like if

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<v Speaker 1>you think about the things that um that we could

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<v Speaker 1>potentially learn before we had observatories like Lego, there was

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<v Speaker 1>a limit, right, there was there was a hard limit

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<v Speaker 1>to what we could learn just because of the limitations

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<v Speaker 1>on our instrument taition our knowledge. Now we've got a

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<v Speaker 1>brand new way to observe, so who knows what we

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<v Speaker 1>will learn. It is probably one of the most exciting

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<v Speaker 1>things about astronomy right now, in fact, maybe the most

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<v Speaker 1>exciting thing about astronomy at the moment. And it's already

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<v Speaker 1>changing some of what we thought we knew about about

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<v Speaker 1>black holes specifically, Yeah, it's changing what we know about

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<v Speaker 1>black holes. For example. One of the things that was

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<v Speaker 1>kind of interesting was they said they were looking at

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<v Speaker 1>the angular momentum, essentially the spin of the black holes,

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<v Speaker 1>so not the orbits of the black holes, but the

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<v Speaker 1>actual individual spins and they said that it ended up

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<v Speaker 1>the spin of the whole collision ended up being different

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<v Speaker 1>from what they had expected. Uh, and they're not sure why.

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<v Speaker 1>They don't know why. They they have no idea this.

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<v Speaker 1>This is really exciting because now we have to ask

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<v Speaker 1>ourselves why we're the black holes spinning at a different

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<v Speaker 1>rate than what we had anticipated. Was it perhaps that

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<v Speaker 1>the two angular momentums of the individual black holes interfered

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<v Speaker 1>with one another and therefore that's what caused the the issue?

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<v Speaker 1>Or is it something totally new, some some kind of

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<v Speaker 1>physics we don't even know. Is there is there variable

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<v Speaker 1>out there that we've totally missed before. Yeah, and it

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<v Speaker 1>could be something well, and it could be called crawfish. Okay,

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<v Speaker 1>let's not go down that dark road yet again. But

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<v Speaker 1>but it could be something that isn't predicted by general relativity.

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<v Speaker 1>It could be something totally new, which again really exciting. UM.

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<v Speaker 1>This also could lead to us having a greater understanding

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<v Speaker 1>of how our universe is expanding and why it's expanding

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<v Speaker 1>at the rate that it is. Um. It also could

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<v Speaker 1>end up giving us a very precise look at how

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<v Speaker 1>much dark energy is in the universe, much more precise

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<v Speaker 1>than any estimation that we have ever made before. Uh,

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<v Speaker 1>And it could open new doors to all sorts of

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<v Speaker 1>new disciplines that we can't anticipate right now. There's a

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<v Speaker 1>term being used called gravitational toronomy. That's really all about

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<v Speaker 1>taking the data from these gravitational waves that we detect

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<v Speaker 1>and then finding out what we can learn from that information.

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<v Speaker 1>And we don't know yet. It's so new that we

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<v Speaker 1>don't even know what to expect. We know that it

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<v Speaker 1>will allow us to look into supernova and neutron stars

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<v Speaker 1>and black holes, but who knows what else will learn?

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<v Speaker 1>But let's let's skip past all of this boring human curiosity.

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<v Speaker 1>I want I want to practical application for this stuff.

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<v Speaker 1>How is it going to work for me? Um? All right, well,

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<v Speaker 1>I want key line pie, but I'm not getting it.

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<v Speaker 1>So what I'm saying is that you want to why

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<v Speaker 1>aren't you getting it? There's a Kroger right next, because

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<v Speaker 1>I'm recording a podcast right now. Uh No. My point

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<v Speaker 1>here is that wanting a practical application of gravitational waves

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<v Speaker 1>is sort of being a little premature. I would argue

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<v Speaker 1>that we don't have any practical application for gravitational waves.

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<v Speaker 1>Uh right now, apart from the fact that it is

0:13:02.480 --> 0:13:06.800
<v Speaker 1>expanding our knowledge to a degree that that we otherwise

0:13:06.840 --> 0:13:09.280
<v Speaker 1>would you know, I would have no access to where's

0:13:09.320 --> 0:13:12.040
<v Speaker 1>my warp drive? Okay, so warp drive. That's an excellent

0:13:12.080 --> 0:13:15.920
<v Speaker 1>that's an excellent way of looking at Well, could gravitational

0:13:15.920 --> 0:13:21.480
<v Speaker 1>waves lead to warp drive? Who knows, maybe centuries from now.

0:13:22.160 --> 0:13:25.560
<v Speaker 1>So gravitational waves do show that spacetime is folding in

0:13:25.559 --> 0:13:28.360
<v Speaker 1>these little ripples, and you could argue that, you know,

0:13:28.440 --> 0:13:31.200
<v Speaker 1>the whole idea behind warp drive or warp systems is

0:13:31.240 --> 0:13:35.280
<v Speaker 1>that you could warp space to decrease the distance between

0:13:35.320 --> 0:13:38.680
<v Speaker 1>you and your destination. So by decreasing that space, you

0:13:38.800 --> 0:13:40.439
<v Speaker 1>decrease the amount of time it takes for you to

0:13:40.480 --> 0:13:43.480
<v Speaker 1>get to where you're going. It's kind of cheating that

0:13:43.480 --> 0:13:46.040
<v Speaker 1>that fact that you cannot travel faster than the speed

0:13:46.040 --> 0:13:48.320
<v Speaker 1>of light. Well, you don't need to trouble faster than

0:13:48.320 --> 0:13:50.120
<v Speaker 1>the speed of light if you can make your destination

0:13:50.240 --> 0:13:54.880
<v Speaker 1>closer to your departure. Right, Yes, But hold on a second. Now,

0:13:55.000 --> 0:13:58.440
<v Speaker 1>what was that figure we had earlier that uh So,

0:13:58.480 --> 0:14:02.040
<v Speaker 1>a gravitational wave of the kind we sensed with lego,

0:14:02.480 --> 0:14:05.360
<v Speaker 1>uh it would take the distance of a kilometer and

0:14:05.480 --> 0:14:09.920
<v Speaker 1>shorten that by one the width of a proton something

0:14:09.960 --> 0:14:12.400
<v Speaker 1>like that. Yeah, so that's not going to be shaving

0:14:12.440 --> 0:14:17.760
<v Speaker 1>a whole lot, maybe if you're a hyper miler in space. Yeah,

0:14:17.800 --> 0:14:20.840
<v Speaker 1>and especially considering that you have to like like vaporize

0:14:21.040 --> 0:14:24.480
<v Speaker 1>three sons in order to do it, not to make

0:14:24.520 --> 0:14:29.320
<v Speaker 1>an omelet without destroying a few star systems, Okay, at

0:14:29.400 --> 0:14:33.520
<v Speaker 1>least not a warp omelet um. So yeah, here's here's

0:14:33.520 --> 0:14:36.600
<v Speaker 1>the thing is that one, we have no practical means

0:14:36.640 --> 0:14:40.000
<v Speaker 1>of warping space time at the moment, apart from like

0:14:40.080 --> 0:14:45.600
<v Speaker 1>some some very experimental science that is of uh questionable

0:14:45.720 --> 0:14:49.960
<v Speaker 1>uh authenticity. And I use that not meaning that I

0:14:50.120 --> 0:14:52.280
<v Speaker 1>personally questioned. I just know that there's a lot of

0:14:52.400 --> 0:14:55.960
<v Speaker 1>argument within the space itself and physics about various engines

0:14:56.040 --> 0:15:00.320
<v Speaker 1>that are at least intended to be a war drive

0:15:00.400 --> 0:15:02.720
<v Speaker 1>of some sort. Well, I mean, I think we're inherently

0:15:02.760 --> 0:15:08.040
<v Speaker 1>talking about a gigantic scale problem, a mass energy scale problem,

0:15:08.120 --> 0:15:12.200
<v Speaker 1>because once you're talking about the kinds of events that

0:15:12.280 --> 0:15:16.400
<v Speaker 1>cause these big gravitational waves, these large perturbations in size

0:15:16.440 --> 0:15:20.160
<v Speaker 1>and distance in space time, you're talking about things on

0:15:20.200 --> 0:15:25.760
<v Speaker 1>the order of the mass of stars and or even yeah,

0:15:25.800 --> 0:15:28.320
<v Speaker 1>in that case, you're talking about like a stellar engineering

0:15:28.480 --> 0:15:31.280
<v Speaker 1>level of technology. Anyway, that we wed have to be

0:15:31.320 --> 0:15:35.680
<v Speaker 1>like a Cardassiev level two system or something. I I

0:15:35.680 --> 0:15:40.080
<v Speaker 1>I am extremely skeptical we will ever create a system

0:15:40.080 --> 0:15:45.920
<v Speaker 1>capable of warping space on any meaningful scale any time

0:15:46.040 --> 0:15:50.040
<v Speaker 1>in the foreseeable future without destroying everything around it in

0:15:50.080 --> 0:15:52.560
<v Speaker 1>the process. If you put that limitation on it, then

0:15:52.600 --> 0:15:57.200
<v Speaker 1>even more so. Yes, okay, alright, warp drives out. But

0:15:57.760 --> 0:16:00.640
<v Speaker 1>what about warping time? Okay, so yeah, we're talking about

0:16:00.640 --> 0:16:03.360
<v Speaker 1>space times. Time travel is clearly going to come up.

0:16:03.720 --> 0:16:07.800
<v Speaker 1>Here's the secret, guys. We can all time travel. You're

0:16:07.840 --> 0:16:10.560
<v Speaker 1>doing it right now. Just it's just called waiting around,

0:16:11.600 --> 0:16:14.920
<v Speaker 1>and you travel through time forward at a scale that

0:16:15.120 --> 0:16:20.360
<v Speaker 1>is remarkably consistent dependent upon your speed relative to an

0:16:20.400 --> 0:16:23.280
<v Speaker 1>independent observer. Though another thing we've talked about on the

0:16:23.320 --> 0:16:27.520
<v Speaker 1>podcast before is that it is just an inherent consequence

0:16:27.520 --> 0:16:31.640
<v Speaker 1>of Einstein's theories that travel into the future based on

0:16:31.680 --> 0:16:36.520
<v Speaker 1>your initial reference frame is entirely possible, like accelerating beyond

0:16:36.600 --> 0:16:39.720
<v Speaker 1>the reference frame from which you originated. So if you

0:16:39.720 --> 0:16:42.040
<v Speaker 1>get into a space ship and you travel near the

0:16:42.080 --> 0:16:44.240
<v Speaker 1>speed of light and take a round trip and come

0:16:44.280 --> 0:16:47.600
<v Speaker 1>back to planet Earth. You will have you will have

0:16:47.760 --> 0:16:50.400
<v Speaker 1>aged slower than you would have if you just stayed

0:16:50.400 --> 0:16:53.240
<v Speaker 1>on Earth. Right relative to the people who were back

0:16:53.280 --> 0:16:57.040
<v Speaker 1>on Earth, you would have experienced less time, like you

0:16:57.080 --> 0:17:00.040
<v Speaker 1>would have felt the passage that there have been a

0:17:00.040 --> 0:17:03.000
<v Speaker 1>smaller amount of time passed on the ship than people

0:17:03.000 --> 0:17:05.320
<v Speaker 1>who were still on Earth had felt, because you were

0:17:05.320 --> 0:17:08.639
<v Speaker 1>traveling at this much faster speed. Yeah, you know. And

0:17:08.680 --> 0:17:10.840
<v Speaker 1>it's not just by traveling near the speed of light.

0:17:10.840 --> 0:17:13.040
<v Speaker 1>You could also do this by being next to an

0:17:13.040 --> 0:17:15.960
<v Speaker 1>extremely massive object, and you could hang out next to

0:17:16.000 --> 0:17:18.560
<v Speaker 1>a black hole or something for a while. Yeah. These

0:17:18.600 --> 0:17:23.760
<v Speaker 1>these are both things that will warp time so effectively

0:17:23.840 --> 0:17:26.520
<v Speaker 1>it would be like traveling into the future. It looks

0:17:26.560 --> 0:17:29.119
<v Speaker 1>like from everything we've ever seen that traveling into the

0:17:29.160 --> 0:17:32.680
<v Speaker 1>past is essentially a no go um. There's nothing that

0:17:32.720 --> 0:17:35.040
<v Speaker 1>we've seen that has suggested that that would be that

0:17:35.080 --> 0:17:38.879
<v Speaker 1>would be a possibility based upon uh, these particular theories.

0:17:38.880 --> 0:17:42.000
<v Speaker 1>I mean, there are other alternative theories that have nothing

0:17:42.000 --> 0:17:44.000
<v Speaker 1>to do with what we're talking about, where people have

0:17:44.080 --> 0:17:47.680
<v Speaker 1>positive the possibility. But based upon what we're chatting about

0:17:47.760 --> 0:17:51.160
<v Speaker 1>right now, especially with gravitational waves, not so much. You're

0:17:51.160 --> 0:17:53.120
<v Speaker 1>not gonna be able to go back and have an

0:17:53.119 --> 0:17:57.399
<v Speaker 1>excellent adventure or a bogus journey. Okay, I'm willing to

0:17:57.440 --> 0:18:01.399
<v Speaker 1>scale back my expectations. If I don't to use a

0:18:01.400 --> 0:18:04.040
<v Speaker 1>warp drive or write a t rex, what about what

0:18:04.080 --> 0:18:09.240
<v Speaker 1>about just reconciling quantum physics with classical physics. I have

0:18:09.400 --> 0:18:14.000
<v Speaker 1>heard people say that the did you hear it through

0:18:14.040 --> 0:18:19.280
<v Speaker 1>a grapevine? I did not, not much longer. Will you

0:18:19.359 --> 0:18:22.960
<v Speaker 1>be mine? Joe? I don't think you ever were, honestly,

0:18:22.960 --> 0:18:25.400
<v Speaker 1>when I look at you at all? This took a turn.

0:18:25.440 --> 0:18:29.280
<v Speaker 1>Do you guys want to be alone? Not anymore? Okay?

0:18:29.359 --> 0:18:33.440
<v Speaker 1>So yeah, alright, So so I have I have read

0:18:33.480 --> 0:18:35.960
<v Speaker 1>at least a couple of different accounts that have suggested

0:18:36.000 --> 0:18:39.320
<v Speaker 1>that perhaps the information we learned from gravitational waves could

0:18:39.359 --> 0:18:43.520
<v Speaker 1>help us bridge some gaps between quantum physics and classical physics.

0:18:44.040 --> 0:18:46.359
<v Speaker 1>When I tried to find out what they meant, like,

0:18:46.440 --> 0:18:50.440
<v Speaker 1>how would this bridge any gaps? I started coming up empty.

0:18:50.520 --> 0:18:53.960
<v Speaker 1>So I don't know precisely if the person who was

0:18:54.040 --> 0:18:59.960
<v Speaker 1>saying that was just kind of yeah, just just like maybe,

0:19:00.760 --> 0:19:02.760
<v Speaker 1>or if they were saying it from a place of

0:19:02.800 --> 0:19:07.280
<v Speaker 1>expertise and they just didn't verbalize how they meant it um.

0:19:07.800 --> 0:19:10.760
<v Speaker 1>I on the face of it, I don't know how

0:19:10.840 --> 0:19:13.560
<v Speaker 1>it would bridge gaps. But then I'm not a quantum physicist.

0:19:13.960 --> 0:19:19.120
<v Speaker 1>I have a very very basic grasp of some elementary

0:19:20.400 --> 0:19:24.000
<v Speaker 1>some some some basic elements I should say, of quantum physics,

0:19:24.119 --> 0:19:29.840
<v Speaker 1>and beyond that it is completely uh mystery to me.

0:19:30.480 --> 0:19:34.480
<v Speaker 1>And so I'm not sure if gravitational waves, if our

0:19:34.600 --> 0:19:38.399
<v Speaker 1>our study of them, will lead to this, the bridging

0:19:38.440 --> 0:19:41.600
<v Speaker 1>of gaps. But if it does, that would be great. Yeah,

0:19:41.600 --> 0:19:43.639
<v Speaker 1>I mean, I I think it's easy for people to

0:19:43.720 --> 0:19:47.560
<v Speaker 1>lose sight of the extent in some ways to which

0:19:47.600 --> 0:19:50.920
<v Speaker 1>gravity is still mysterious to us, Like we understand gravity

0:19:51.040 --> 0:19:55.159
<v Speaker 1>very well. Einstein's theories give us an extremely accurate model

0:19:55.200 --> 0:19:57.720
<v Speaker 1>of gravity that we can use to predict the behavior

0:19:57.840 --> 0:20:00.520
<v Speaker 1>of objects in the universe, and it were is great,

0:20:01.280 --> 0:20:05.160
<v Speaker 1>So it's not like Einstein was wrong with general relativity.

0:20:05.200 --> 0:20:08.840
<v Speaker 1>But yeah, there are these lingering questions like how come

0:20:08.880 --> 0:20:13.800
<v Speaker 1>gravity does not reign at the quantum level? Uh, what effect,

0:20:13.840 --> 0:20:18.080
<v Speaker 1>if any, does gravity have on various quantum processes? Well,

0:20:18.200 --> 0:20:21.639
<v Speaker 1>I remember hearing the problem is wise gravity so relatively

0:20:21.640 --> 0:20:25.200
<v Speaker 1>weak compared to the other fundamental forces of the universe, right, Yeah,

0:20:25.240 --> 0:20:28.600
<v Speaker 1>the strong and weak nuclear force, that kind of thing. Yeah,

0:20:28.720 --> 0:20:31.320
<v Speaker 1>that's a These are all questions that we're still looking,

0:20:32.080 --> 0:20:34.840
<v Speaker 1>you know, to try and find those answers. Gravity for

0:20:34.880 --> 0:20:37.480
<v Speaker 1>the longest time has been kind of the big like

0:20:38.480 --> 0:20:41.240
<v Speaker 1>where do we fit this in with our other or

0:20:41.320 --> 0:20:46.600
<v Speaker 1>other models, And maybe through gravitational waves and through studying them,

0:20:46.600 --> 0:20:48.720
<v Speaker 1>will be able to answer some of those questions and

0:20:48.760 --> 0:20:51.400
<v Speaker 1>come up with a more complete model of the universe,

0:20:51.960 --> 0:20:54.600
<v Speaker 1>which means we understand reality a little bit better and

0:20:54.640 --> 0:20:58.560
<v Speaker 1>that is phenomenal. Uh. One thing I would say about

0:20:58.560 --> 0:21:00.959
<v Speaker 1>all this, while I I've been kind of you know,

0:21:01.280 --> 0:21:05.160
<v Speaker 1>dismissing these practical application ideas, is that we can never

0:21:05.200 --> 0:21:09.520
<v Speaker 1>anticipate what sort of practical applications may come of scientific discovery,

0:21:10.080 --> 0:21:14.560
<v Speaker 1>and in fact, there may be some awesome practical applications

0:21:14.600 --> 0:21:18.520
<v Speaker 1>that we cannot even guess at right now that in

0:21:18.600 --> 0:21:22.280
<v Speaker 1>twenty years time will just be a part of everyday lives.

0:21:22.880 --> 0:21:25.840
<v Speaker 1>And it's hard for us to imagine that. This is

0:21:25.840 --> 0:21:29.000
<v Speaker 1>one of those times where when people make predictions about

0:21:29.000 --> 0:21:32.119
<v Speaker 1>the future, they hit that stumbling block because it's something

0:21:32.160 --> 0:21:35.439
<v Speaker 1>you could not possibly have anticipated unless you were you know,

0:21:35.520 --> 0:21:41.240
<v Speaker 1>some brilliant madman like Einstein and you had really considered

0:21:41.280 --> 0:21:43.600
<v Speaker 1>this to a point where you had reached that logical

0:21:43.640 --> 0:21:46.800
<v Speaker 1>progression and said, if this is true, then we could

0:21:46.840 --> 0:21:50.760
<v Speaker 1>do this. Um. But I am certainly not at that point.

0:21:51.480 --> 0:21:55.159
<v Speaker 1>I'm not nearly an expert on the subject. So I

0:21:55.200 --> 0:21:57.200
<v Speaker 1>think that we probably will end up seeing some practical

0:21:57.240 --> 0:22:00.879
<v Speaker 1>applications as a result of this. You're saying gravity bombs,

0:22:00.880 --> 0:22:06.720
<v Speaker 1>aren't you. Uh, who knows? Maybe, you know, maybe it'll

0:22:06.760 --> 0:22:08.800
<v Speaker 1>be one of those things where you know, everyone will

0:22:08.840 --> 0:22:11.960
<v Speaker 1>have that extra you know, that one switch in your

0:22:12.000 --> 0:22:14.879
<v Speaker 1>house that doesn't seem to control anything. Maybe in the

0:22:14.920 --> 0:22:18.720
<v Speaker 1>future that's just gravity, and like everything just starts floating,

0:22:18.720 --> 0:22:21.399
<v Speaker 1>and like, oh, that's what that one does. You know,

0:22:21.600 --> 0:22:24.000
<v Speaker 1>you flip it in the and the TV remote is

0:22:25.080 --> 0:22:29.040
<v Speaker 1>width of a proton closer to your hand. Right, Well,

0:22:29.080 --> 0:22:31.639
<v Speaker 1>that saves me that that much effort of getting up

0:22:31.640 --> 0:22:34.320
<v Speaker 1>and picking it up, so now I can finally switch

0:22:34.359 --> 0:22:37.520
<v Speaker 1>it to America's funny film videos. Alright, So that wraps

0:22:37.640 --> 0:22:43.840
<v Speaker 1>up this quick discussion about the future implications of our discovery.

0:22:43.840 --> 0:22:48.200
<v Speaker 1>Gravitational waves are our our actual uh you know, measurement

0:22:48.280 --> 0:22:50.960
<v Speaker 1>of them, the analysis of them, what that might lead to.

0:22:51.200 --> 0:22:53.719
<v Speaker 1>The best part about this the reason why it's so

0:22:53.720 --> 0:22:56.639
<v Speaker 1>short is because there's so little that we can know

0:22:56.880 --> 0:22:59.960
<v Speaker 1>right now. But that's the exciting part because we will

0:23:00.000 --> 0:23:03.359
<v Speaker 1>will fill those gaps in in our knowledge. Like you know,

0:23:03.600 --> 0:23:06.920
<v Speaker 1>ten years from now, think of all the things that

0:23:07.040 --> 0:23:09.240
<v Speaker 1>we know if we were to still be doing this,

0:23:09.960 --> 0:23:12.159
<v Speaker 1>which would amaze me. But here's from now. If we

0:23:12.160 --> 0:23:14.040
<v Speaker 1>were still doing this, we could revisit this topic and

0:23:14.040 --> 0:23:17.440
<v Speaker 1>talk about here's all the stuff we didn't anticipate when

0:23:17.440 --> 0:23:21.439
<v Speaker 1>we recorded that episode back in and that's really exciting. Guys.

0:23:21.440 --> 0:23:24.040
<v Speaker 1>If you have any suggestions for future episodes beforeward Thinking,

0:23:24.040 --> 0:23:28.359
<v Speaker 1>whether it is about science, technology, culture, anything. Really, if

0:23:28.400 --> 0:23:31.399
<v Speaker 1>you just want to know how is X what's that

0:23:31.440 --> 0:23:34.520
<v Speaker 1>going to be like in the future, you should write

0:23:34.560 --> 0:23:36.440
<v Speaker 1>us and let us know Our email addresses f W

0:23:36.680 --> 0:23:39.359
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0:23:39.440 --> 0:23:42.479
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0:23:42.480 --> 0:23:44.800
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0:23:44.840 --> 0:23:47.440
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0:23:47.440 --> 0:23:49.960
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0:23:50.000 --> 0:23:58.760
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0:23:58.760 --> 0:24:03.440
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0:24:03.440 --> 0:24:15.640
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