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Wrinkles and Rips in Spacetime | Deirdre Shoemaker | TEDxGeorgiaTech


hi everybody so I’m gonna share with you

hi everybody so I’m gonna share with you one of my passions and it’s not Pokemon

one of my passions and it’s not Pokemon

one of my passions and it’s not Pokemon go hahaha that would be funny for a 45

go hahaha that would be funny for a 45

go hahaha that would be funny for a 45 year old woman but you everyone

year old woman but you everyone

year old woman but you everyone recognizes image how many people have

recognizes image how many people have

recognizes image how many people have played it a few you’re on camera okay

played it a few you’re on camera okay

played it a few you’re on camera okay I’m going to share with you a kind of

I’m going to share with you a kind of

I’m going to share with you a kind of strange fact that pokemons go and Albert

strange fact that pokemons go and Albert

strange fact that pokemons go and Albert Einstein have something in common and it

Einstein have something in common and it

Einstein have something in common and it wasn’t that Albert Einstein played

wasn’t that Albert Einstein played

wasn’t that Albert Einstein played Pokemon go Albert Einstein lived in a

Pokemon go Albert Einstein lived in a

Pokemon go Albert Einstein lived in a fascinating time for physics he’s

fascinating time for physics he’s

fascinating time for physics he’s probably the most famous physicist

probably the most famous physicist

probably the most famous physicist that’s ever lived

that’s ever lived

that’s ever lived maybe scientist and he lived in a time

maybe scientist and he lived in a time

maybe scientist and he lived in a time when there was some tension building and

when there was some tension building and

when there was some tension building and how we understood some fundamental

how we understood some fundamental

how we understood some fundamental physics properties we had developed a

physics properties we had developed a

physics properties we had developed a new theory of light called

new theory of light called

new theory of light called electromagnetism and it was inconsistent

electromagnetism and it was inconsistent

electromagnetism and it was inconsistent with some of the previous notions of how

with some of the previous notions of how

with some of the previous notions of how motion worked developed by Newton and

motion worked developed by Newton and

motion worked developed by Newton and Galileo there were also some interesting

Galileo there were also some interesting

Galileo there were also some interesting discrepancies about how planetary motion

discrepancies about how planetary motion

discrepancies about how planetary motion you know the earth and Mercury orbiting

you know the earth and Mercury orbiting

you know the earth and Mercury orbiting the Sun was a little inconsistent tiny

the Sun was a little inconsistent tiny

the Sun was a little inconsistent tiny tiny inconsistencies with Newtonian

tiny inconsistencies with Newtonian

tiny inconsistencies with Newtonian theory of gravity and when you have

theory of gravity and when you have

theory of gravity and when you have these things happen

these things happen

these things happen attention builds and you know something

attention builds and you know something

attention builds and you know something has to change because we need everything

has to change because we need everything

has to change because we need everything to match with experiment I’m so famous

to match with experiment I’m so famous

to match with experiment I’m so famous because when he developed the theory

because when he developed the theory

because when he developed the theory that would fix some of these

that would fix some of these

that would fix some of these inconsistencies he changed the way we

inconsistencies he changed the way we

inconsistencies he changed the way we think about space and time he actually

think about space and time he actually

think about space and time he actually had to abandon a sacred belief to us

had to abandon a sacred belief to us

had to abandon a sacred belief to us that time is absolute and instead he

that time is absolute and instead he

that time is absolute and instead he discovered the time is in fact relative

discovered the time is in fact relative

discovered the time is in fact relative I don’t mean the time that you feel

I don’t mean the time that you feel

I don’t mean the time that you feel being bored on a plane there is some

being bored on a plane there is some

being bored on a plane there is some time change up there but it’s not from

time change up there but it’s not from

time change up there but it’s not from being bored we mean the fact that when

being bored we mean the fact that when

being bored we mean the fact that when two objects are emotion relative to each

two objects are emotion relative to each

two objects are emotion relative to each other time runs differently for those

other time runs differently for those

other time runs differently for those two objects if they compare clocks they

two objects if they compare clocks they

two objects if they compare clocks they will not agree and we also mean that if

will not agree and we also mean that if

will not agree and we also mean that if there’s a height difference so compared

there’s a height difference so compared

there’s a height difference so compared to something on the surface of the earth

to something on the surface of the earth

to something on the surface of the earth and something out of height from the

and something out of height from the

and something out of height from the surface of the earth clocks will again

surface of the earth clocks will again

surface of the earth clocks will again run differently and this is such a

run differently and this is such a

run differently and this is such a amazing notion that it’s really captured

amazing notion that it’s really captured

amazing notion that it’s really captured attention of a lot of people and that

attention of a lot of people and that

attention of a lot of people and that what happens

what happens

what happens when we look at something that’s a

when we look at something that’s a

when we look at something that’s a mundane example like the pokey mango

mundane example like the pokey mango

mundane example like the pokey mango it runs on GPS and the Global

it runs on GPS and the Global

it runs on GPS and the Global Positioning System is the best example I

Positioning System is the best example I

Positioning System is the best example I have to give you to understand how

have to give you to understand how

have to give you to understand how important it is to really solve

important it is to really solve

important it is to really solve equations like Einstein did which he

equations like Einstein did which he

equations like Einstein did which he called the special general theories of

called the special general theories of

called the special general theories of relativity and if you look at how GPS

relativity and if you look at how GPS

relativity and if you look at how GPS works those are satellites orbiting the

works those are satellites orbiting the

works those are satellites orbiting the Earth and those satellites beam

Earth and those satellites beam

Earth and those satellites beam information down to your phone

information down to your phone

information down to your phone pretend it’s my phone and your phone is

pretend it’s my phone and your phone is

pretend it’s my phone and your phone is what you’re usually your GPS so what’s

what you’re usually your GPS so what’s

what you’re usually your GPS so what’s happening is because the satellites are

happening is because the satellites are

happening is because the satellites are moving and it relative to your phone and

moving and it relative to your phone and

moving and it relative to your phone and because the satellites are at a

because the satellites are at a

because the satellites are at a different height from the surface the

different height from the surface the

different height from the surface the earth compared to your phone

earth compared to your phone

earth compared to your phone time is running differently for you and

time is running differently for you and

time is running differently for you and the satellites and that these things

the satellites and that these things

the satellites and that these things aren’t corrected by using Einstein’s

aren’t corrected by using Einstein’s

aren’t corrected by using Einstein’s theory you’ll be inaccurate very quickly

theory you’ll be inaccurate very quickly

theory you’ll be inaccurate very quickly you won’t find your Pokemon you won’t

you won’t find your Pokemon you won’t

you won’t find your Pokemon you won’t find Walmart whatever you’re looking for

find Walmart whatever you’re looking for

find Walmart whatever you’re looking for so believe it or not a theory that

so believe it or not a theory that

so believe it or not a theory that Einstein developed a hundred years ago

Einstein developed a hundred years ago

Einstein developed a hundred years ago you use every day if you’re like me and

you use every day if you’re like me and

you use every day if you’re like me and can’t find anything you use every day to

can’t find anything you use every day to

can’t find anything you use every day to locate stuff and so I think that set out

locate stuff and so I think that set out

locate stuff and so I think that set out to do that that’s a consequence of

to do that that’s a consequence of

to do that that’s a consequence of something of fundamental physics but

something of fundamental physics but

something of fundamental physics but other than this mundane example of GPS

other than this mundane example of GPS

other than this mundane example of GPS Einstein’s theories predicted two things

Einstein’s theories predicted two things

Einstein’s theories predicted two things that even Einstein himself wasn’t

that even Einstein himself wasn’t

that even Einstein himself wasn’t comfortable with he made the theory

comfortable with he made the theory

comfortable with he made the theory itself made two extraordinary claims one

itself made two extraordinary claims one

itself made two extraordinary claims one of them was black holes and the other

of them was black holes and the other

of them was black holes and the other was gravitational waves and even

was gravitational waves and even

was gravitational waves and even throughout his life he struggled with

throughout his life he struggled with

throughout his life he struggled with whether or not these were mathematical

whether or not these were mathematical

whether or not these were mathematical consequences of his theory with no

consequences of his theory with no

consequences of his theory with no physical realization or were they

physical realization or were they

physical realization or were they actually part of our universe and that’s

actually part of our universe and that’s

actually part of our universe and that’s where we’re going next black holes have

where we’re going next black holes have

where we’re going next black holes have long fascinated me I was apparently very

long fascinated me I was apparently very

long fascinated me I was apparently very dorky child and at 12 I was obsessed

dorky child and at 12 I was obsessed

dorky child and at 12 I was obsessed with black holes wrote a paper in

with black holes wrote a paper in

with black holes wrote a paper in seventh grade made no sense it’s okay

seventh grade made no sense it’s okay

seventh grade made no sense it’s okay everybody wrinkled on time you know all

everybody wrinkled on time you know all

everybody wrinkled on time you know all that business and I think they still

that business and I think they still

that business and I think they still capture the imagination of so many

capture the imagination of so many

capture the imagination of so many people there’s something very

people there’s something very

people there’s something very interesting about a black hole so think

interesting about a black hole so think

interesting about a black hole so think about it how does a black hole form we

about it how does a black hole form we

about it how does a black hole form we have a star like our Sun but much bigger

have a star like our Sun but much bigger

have a star like our Sun but much bigger eventually every star runs out of fuel

eventually every star runs out of fuel

eventually every star runs out of fuel we’ll stop shining runs out of fuel it

we’ll stop shining runs out of fuel it

we’ll stop shining runs out of fuel it starts to collapse because nothing will

starts to collapse because nothing will

starts to collapse because nothing will beat gravity at that point

beat gravity at that point

beat gravity at that point and if it’s really big you think of a

and if it’s really big you think of a

and if it’s really big you think of a collapsing like a balloon running out of

collapsing like a balloon running out of

collapsing like a balloon running out of air but if a star is big enough nothing

air but if a star is big enough nothing

air but if a star is big enough nothing will stop it from collapsing that we

will stop it from collapsing that we

will stop it from collapsing that we know of and it actually goes all the way

know of and it actually goes all the way

know of and it actually goes all the way down just pressure pressure until it

down just pressure pressure until it

down just pressure pressure until it sinks to a singular point and at that

sinks to a singular point and at that

sinks to a singular point and at that point we’ve created a black hole the

point we’ve created a black hole the

point we’ve created a black hole the black hole will be much smaller than the

black hole will be much smaller than the

black hole will be much smaller than the original star it’s very compact and it

original star it’s very compact and it

original star it’s very compact and it famously doesn’t even allow light to

famously doesn’t even allow light to

famously doesn’t even allow light to escape which is why you see these dark

escape which is why you see these dark

escape which is why you see these dark circles up here so black holes have

circles up here so black holes have

circles up here so black holes have captured our imagination because what

captured our imagination because what

captured our imagination because what they’ve done is informing isn’t

they’ve done is informing isn’t

they’ve done is informing isn’t collapsing to form this black hole the

collapsing to form this black hole the

collapsing to form this black hole the curvature of space and time gets so

curvature of space and time gets so

curvature of space and time gets so tense

tense

tense they’re so stretched and it’s such

they’re so stretched and it’s such

they’re so stretched and it’s such strong curvature it’s almost like we’re

strong curvature it’s almost like we’re

strong curvature it’s almost like we’re creating a rip in space and time itself

creating a rip in space and time itself

creating a rip in space and time itself up here I have two black holes because

up here I have two black holes because

up here I have two black holes because one is never enough always better to

one is never enough always better to

one is never enough always better to have to you this is a picture that’s a

have to you this is a picture that’s a

have to you this is a picture that’s a computer generation it’s not an actual

computer generation it’s not an actual

computer generation it’s not an actual photograph of two black holes and what

photograph of two black holes and what

photograph of two black holes and what we’ve done is this is a picture done by

we’ve done is this is a picture done by

we’ve done is this is a picture done by some of my colleagues and they have

some of my colleagues and they have

some of my colleagues and they have rendered on a computer what would happen

rendered on a computer what would happen

rendered on a computer what would happen if there were two black holes between us

if there were two black holes between us

if there were two black holes between us in the centre of the Milky Way has

in the centre of the Milky Way has

in the centre of the Milky Way has anyone actually gotten a chance to see

anyone actually gotten a chance to see

anyone actually gotten a chance to see what it looks like to look towards the

what it looks like to look towards the

what it looks like to look towards the Milky Way and a dark night can’t do it

Milky Way and a dark night can’t do it

Milky Way and a dark night can’t do it in Atlanta you can see beautiful images

in Atlanta you can see beautiful images

in Atlanta you can see beautiful images of it it’s a big stretch of starry milky

of it it’s a big stretch of starry milky

of it it’s a big stretch of starry milky light and if you have two black holes

light and if you have two black holes

light and if you have two black holes between us and that milky light the

between us and that milky light the

between us and that milky light the light gets so distorted as it goes near

light gets so distorted as it goes near

light gets so distorted as it goes near those black holes the curvature of space

those black holes the curvature of space

those black holes the curvature of space and time is all funky and warped and

and time is all funky and warped and

and time is all funky and warped and twisted but the light looks warped and

twisted but the light looks warped and

twisted but the light looks warped and twisted because they had a travel curved

twisted because they had a travel curved

twisted because they had a travel curved path to reach our eyes now this isn’t

path to reach our eyes now this isn’t

path to reach our eyes now this isn’t really a picture this is just a

really a picture this is just a

really a picture this is just a rendition of what it would look like but

rendition of what it would look like but

rendition of what it would look like but think about what’s happening if I have a

think about what’s happening if I have a

think about what’s happening if I have a star and a companion star and both of

star and a companion star and both of

star and a companion star and both of them collapse to form a black hole then

them collapse to form a black hole then

them collapse to form a black hole then they’re orbiting around each other just

they’re orbiting around each other just

they’re orbiting around each other just like the Earth orbits the Sun and

like the Earth orbits the Sun and

like the Earth orbits the Sun and eventually they’re going to merge

eventually they’re going to merge

eventually they’re going to merge together they’re attracted to each other

together they’re attracted to each other

together they’re attracted to each other think about what’s happening to the

think about what’s happening to the

think about what’s happening to the space and time around it it’s just

space and time around it it’s just

space and time around it it’s just whipping and curving and it’s gotta be

whipping and curving and it’s gotta be

whipping and curving and it’s gotta be the most intense thing out there there

the most intense thing out there there

the most intense thing out there there has to be a physical consequence of such

has to be a physical consequence of such

has to be a physical consequence of such a dynamic and intense environment and

a dynamic and intense environment and

a dynamic and intense environment and that leads us to our second

that leads us to our second

that leads us to our second extraordinary claim of Einstein his

extraordinary claim of Einstein his

extraordinary claim of Einstein his theories claim that when when space and

theories claim that when when space and

theories claim that when when space and time are agitated like that when a

time are agitated like that when a

time are agitated like that when a something as compact as a black hole is

something as compact as a black hole is

something as compact as a black hole is accelerate

accelerate

accelerate then we must give off some kind of

then we must give off some kind of

then we must give off some kind of energy it’s called gravitational waves

energy it’s called gravitational waves

energy it’s called gravitational waves and near the source of this energy it’s

and near the source of this energy it’s

and near the source of this energy it’s gonna be really intense intense

gonna be really intense intense

gonna be really intense intense radiation but we can’t see it at all

radiation but we can’t see it at all

radiation but we can’t see it at all it’s not light so I’m showing you a

it’s not light so I’m showing you a

it’s not light so I’m showing you a computer graphic this is done by solving

computer graphic this is done by solving

computer graphic this is done by solving here at Georgia Tech we solve a science

here at Georgia Tech we solve a science

here at Georgia Tech we solve a science equations for two black holes colliding

equations for two black holes colliding

equations for two black holes colliding and we predict what the radiation and

and we predict what the radiation and

and we predict what the radiation and what the gravitational waves would look

what the gravitational waves would look

what the gravitational waves would look like so this is the movie and you see

like so this is the movie and you see

like so this is the movie and you see that it’s color-coded blue and orange to

that it’s color-coded blue and orange to

that it’s color-coded blue and orange to give you a sense of what the waves would

give you a sense of what the waves would

give you a sense of what the waves would look like even though they’re not

look like even though they’re not

look like even though they’re not viewable by the eye because they’re not

viewable by the eye because they’re not

viewable by the eye because they’re not electromagnetism so the two black holes

electromagnetism so the two black holes

electromagnetism so the two black holes or each other and they collide they form

or each other and they collide they form

or each other and they collide they form a bigger black hole and then there’s

a bigger black hole and then there’s

a bigger black hole and then there’s gravity waves it comes pouring out of

gravity waves it comes pouring out of

gravity waves it comes pouring out of the event and then we ask ourselves a

the event and then we ask ourselves a

the event and then we ask ourselves a question super dynamic crazy curvature

question super dynamic crazy curvature

question super dynamic crazy curvature is happening near that system but we’re

is happening near that system but we’re

is happening near that system but we’re really really far away it’s a good thing

really really far away it’s a good thing

really really far away it’s a good thing really far away from these black holes

really far away from these black holes

really far away from these black holes they’re far away into the universe so

they’re far away into the universe so

they’re far away into the universe so what happens by the time they reach us

what happens by the time they reach us

what happens by the time they reach us on planet earth and can we figure out a

on planet earth and can we figure out a

on planet earth and can we figure out a way to measure them to find out was

way to measure them to find out was

way to measure them to find out was Einstein’s theory predicting things that

Einstein’s theory predicting things that

Einstein’s theory predicting things that are right or not so this is a scale it’s

are right or not so this is a scale it’s

are right or not so this is a scale it’s vastly exaggerated this is an image out

vastly exaggerated this is an image out

vastly exaggerated this is an image out of the LIGO collaboration and what

of the LIGO collaboration and what

of the LIGO collaboration and what you’re going to see is what happens when

you’re going to see is what happens when

you’re going to see is what happens when a gravitational wave hits the earth so

a gravitational wave hits the earth so

a gravitational wave hits the earth so we’re gonna let the gravitational wave

we’re gonna let the gravitational wave

we’re gonna let the gravitational wave come from very far away or we might not

come from very far away or we might not

come from very far away or we might not this is why they tell you don’t show

this is why they tell you don’t show

this is why they tell you don’t show movies at a TEDx talk but I’m stubborn

movies at a TEDx talk but I’m stubborn

movies at a TEDx talk but I’m stubborn so a gravitational wave comes hits the

so a gravitational wave comes hits the

so a gravitational wave comes hits the earth and the earth would actually

earth and the earth would actually

earth and the earth would actually wobble like a bowl of jelly and what our

wobble like a bowl of jelly and what our

wobble like a bowl of jelly and what our job is as experimental physicists I’m a

job is as experimental physicists I’m a

job is as experimental physicists I’m a theorist and I work with them and I say

theorist and I work with them and I say

theorist and I work with them and I say this is what a gravitational wave should

this is what a gravitational wave should

this is what a gravitational wave should look like and then they go and look for

look like and then they go and look for

look like and then they go and look for it and the way they look for it is

it and the way they look for it is

it and the way they look for it is called the LIGO experiment this is an

called the LIGO experiment this is an

called the LIGO experiment this is an experiment in Louisiana and there’s

experiment in Louisiana and there’s

experiment in Louisiana and there’s another one in Washington State

another one in Washington State

another one in Washington State and so when a gravitational wave travels

and so when a gravitational wave travels

and so when a gravitational wave travels to the surface of the earth what’s it’s

to the surface of the earth what’s it’s

to the surface of the earth what’s it’s doing is it’s stretching space and time

doing is it’s stretching space and time

doing is it’s stretching space and time as it comes and if I have two masses in

as it comes and if I have two masses in

as it comes and if I have two masses in an l-shaped arm like we have here one’s

an l-shaped arm like we have here one’s

an l-shaped arm like we have here one’s hanging at one end station another is

hanging at one end station another is

hanging at one end station another is hanging at the other when the

hanging at the other when the

hanging at the other when the gravitational wave passed it literally

gravitational wave passed it literally

gravitational wave passed it literally distorts space as it passes and it

distorts space as it passes and it

distorts space as it passes and it causes these arms to change in length

causes these arms to change in length

causes these arms to change in length and the LIGO experiment

and the LIGO experiment

and the LIGO experiment actually detects a way to detect this

actually detects a way to detect this

actually detects a way to detect this change in length and translate that into

change in length and translate that into

change in length and translate that into the fact that we’ve seen for the first

the fact that we’ve seen for the first

the fact that we’ve seen for the first time a gravitational wave this is the

time a gravitational wave this is the

time a gravitational wave this is the ugliest image I showed you and this one

ugliest image I showed you and this one

ugliest image I showed you and this one is the most spectacular so you have a

is the most spectacular so you have a

is the most spectacular so you have a hundred years after Albert Einstein’s

hundred years after Albert Einstein’s

hundred years after Albert Einstein’s theory has been developed we have some

theory has been developed we have some

theory has been developed we have some twenty years of scientists Polly more

twenty years of scientists Polly more

twenty years of scientists Polly more than that 30 years of scientists and

than that 30 years of scientists and

than that 30 years of scientists and engineers building experiment and what

engineers building experiment and what

engineers building experiment and what it has to do this experiment has to

it has to do this experiment has to

it has to do this experiment has to basically see a wrinkle of space-time

basically see a wrinkle of space-time

basically see a wrinkle of space-time oscillation coming towards it

oscillation coming towards it

oscillation coming towards it that’s so subtle that it’s almost

that’s so subtle that it’s almost

that’s so subtle that it’s almost impossible to detect and then it took 20

impossible to detect and then it took 20

impossible to detect and then it took 20 years for scientists like myself to

years for scientists like myself to

years for scientists like myself to solve Einstein’s equations for two black

solve Einstein’s equations for two black

solve Einstein’s equations for two black holes so we could all come together and

holes so we could all come together and

holes so we could all come together and for the first time detect gravitational

for the first time detect gravitational

for the first time detect gravitational waves so on September 14 2015 we a

waves so on September 14 2015 we a

waves so on September 14 2015 we a binary black hole so these two black

binary black hole so these two black

binary black hole so these two black holes were orbiting 1.4 billion years

holes were orbiting 1.4 billion years

holes were orbiting 1.4 billion years ago and that information and finally

ago and that information and finally

ago and that information and finally traveled to the earth so we were still

traveled to the earth so we were still

traveled to the earth so we were still single-celled organisms when this

single-celled organisms when this

single-celled organisms when this collision happened and it took 1.4

collision happened and it took 1.4

collision happened and it took 1.4 billion years for the information to

billion years for the information to

billion years for the information to reach earth that’s how far away it was

reach earth that’s how far away it was

reach earth that’s how far away it was by the time it reaches us it’s super

by the time it reaches us it’s super

by the time it reaches us it’s super weak barely detected and this is it’s

weak barely detected and this is it’s

weak barely detected and this is it’s picture signature so it looks like a

picture signature so it looks like a

picture signature so it looks like a goofy sine wave you know with some mask

goofy sine wave you know with some mask

goofy sine wave you know with some mask because the detector is noisy and it

because the detector is noisy and it

because the detector is noisy and it took about 0.2 seconds after traveling

took about 0.2 seconds after traveling

took about 0.2 seconds after traveling 1.4 billion years to pass through the

1.4 billion years to pass through the

1.4 billion years to pass through the earth but we were there we were ready

earth but we were there we were ready

earth but we were there we were ready everything was in place

everything was in place

everything was in place so it might not doesn’t look very

so it might not doesn’t look very

so it might not doesn’t look very impressive this is the one from the

impressive this is the one from the

impressive this is the one from the Washington detector but nonetheless if

Washington detector but nonetheless if

Washington detector but nonetheless if you imagine the timing it was pretty

you imagine the timing it was pretty

you imagine the timing it was pretty exciting to be one of the scientists

exciting to be one of the scientists

exciting to be one of the scientists working on this having devoted my whole

working on this having devoted my whole

working on this having devoted my whole career studying these black holes and

career studying these black holes and

career studying these black holes and Einstein’s theory it’s actually be

Einstein’s theory it’s actually be

Einstein’s theory it’s actually be present when the first one was detected

present when the first one was detected

present when the first one was detected and I think it says something about

and I think it says something about

and I think it says something about humanity that a human brain can think of

humanity that a human brain can think of

humanity that a human brain can think of a theory come up with stuff that doesn’t

a theory come up with stuff that doesn’t

a theory come up with stuff that doesn’t even make sense for a hundred years and

even make sense for a hundred years and

even make sense for a hundred years and we could actually build the detector and

we could actually build the detector and

we could actually build the detector and find out it really exists in the

find out it really exists in the

find out it really exists in the universe thank you

”

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