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Listening for Black Holes in a Quiet Universe | Guido Muller | TEDxUF


[Music]

[Music] our story begins in a galaxy far far

our story begins in a galaxy far far

our story begins in a galaxy far far away long-forgotten times about 1

away long-forgotten times about 1

away long-forgotten times about 1 billion years ago in a galaxy 1 billion

billion years ago in a galaxy 1 billion

billion years ago in a galaxy 1 billion light-years away two black holes circled

light-years away two black holes circled

light-years away two black holes circled around each other they got closer and

around each other they got closer and

around each other they got closer and closer faster and faster and their speed

closer faster and faster and their speed

closer faster and faster and their speed reached 60% of the speed of light they

reached 60% of the speed of light they

reached 60% of the speed of light they finally crashed into each other this

finally crashed into each other this

finally crashed into each other this crash

crash

crash stared up the structure of space-time

stared up the structure of space-time

stared up the structure of space-time itself the generated gravitational waves

itself the generated gravitational waves

itself the generated gravitational waves which is September 2015

which is September 2015

which is September 2015 passed through earth and change the

passed through earth and change the

passed through earth and change the distance between mirrors separated by

distance between mirrors separated by

distance between mirrors separated by four kilometers in remote sites in

four kilometers in remote sites in

four kilometers in remote sites in Louisiana and Washington State by an

Louisiana and Washington State by an

Louisiana and Washington State by an unimaginably small amount a millionth of

unimaginably small amount a millionth of

unimaginably small amount a millionth of a millionth of a millionth of a meter

a millionth of a millionth of a meter

a millionth of a millionth of a meter and these changes only lasted for a

and these changes only lasted for a

and these changes only lasted for a fraction of a second the celebrated

fraction of a second the celebrated

fraction of a second the celebrated scientific breakthrough was not only the

scientific breakthrough was not only the

scientific breakthrough was not only the first direct detection of gravitational

first direct detection of gravitational

first direct detection of gravitational waves or the first detection of merging

waves or the first detection of merging

waves or the first detection of merging black holes or the first detection of

black holes or the first detection of

black holes or the first detection of stellar-mass black holes outside our own

stellar-mass black holes outside our own

stellar-mass black holes outside our own galaxy or the most powerful individual

galaxy or the most powerful individual

galaxy or the most powerful individual event ever recorded the detection was

event ever recorded the detection was

event ever recorded the detection was also also a triumph of modern technology

also also a triumph of modern technology

also also a triumph of modern technology and what is possible the significant

and what is possible the significant

and what is possible the significant number of highly talented people and me

number of highly talented people and me

number of highly talented people and me put their heads together to make the

put their heads together to make the

put their heads together to make the impossible possible but what is this all

impossible possible but what is this all

impossible possible but what is this all about and why is it so important when

about and why is it so important when

about and why is it so important when you think of a star you think of its

you think of a star you think of its

you think of a star you think of its brightness so largely you want to look

brightness so largely you want to look

brightness so largely you want to look at it now there are billions of stars in

at it now there are billions of stars in

at it now there are billions of stars in each galaxy at very far distances all

each galaxy at very far distances all

each galaxy at very far distances all awesome look like a singer merged spot

awesome look like a singer merged spot

awesome look like a singer merged spot now try to find a black hole

now try to find a black hole

now try to find a black hole of the size of Paris or New York black

of the size of Paris or New York black

of the size of Paris or New York black hole that doesn’t let any light out

hole that doesn’t let any light out

hole that doesn’t let any light out inside this spot it is impossible but

this is our advantage

this is our advantage black holes like a lot of noise when

black holes like a lot of noise when

black holes like a lot of noise when they crash into one another in the fall

they crash into one another in the fall

they crash into one another in the fall of 2015 we started listening with our

of 2015 we started listening with our

of 2015 we started listening with our new instruments Carlile detected a few

new instruments Carlile detected a few

new instruments Carlile detected a few of these crashes this whooping sound

of these crashes this whooping sound

of these crashes this whooping sound from this sound we determined that this

from this sound we determined that this

from this sound we determined that this was a pair of black holes each of them

was a pair of black holes each of them

was a pair of black holes each of them around 30 times heavier than our Sun

around 30 times heavier than our Sun

around 30 times heavier than our Sun still only as large as Paris or New York

still only as large as Paris or New York

still only as large as Paris or New York and this pair collided merged and the

and this pair collided merged and the

and this pair collided merged and the witness the formation of a new heavier

witness the formation of a new heavier

witness the formation of a new heavier black hole born a billion years ago we

black hole born a billion years ago we

black hole born a billion years ago we would never have seen them these are

would never have seen them these are

would never have seen them these are black holes hiding very likely was in

black holes hiding very likely was in

black holes hiding very likely was in billions of bright stars so now we know

billions of bright stars so now we know

billions of bright stars so now we know that these black holes exist that they

that these black holes exist that they

that these black holes exist that they existed a billion years ago that they

existed a billion years ago that they

existed a billion years ago that they merge because we listened because we

merge because we listened because we

merge because we listened because we detect the gravitational waves emitted

detect the gravitational waves emitted

detect the gravitational waves emitted during this collision but what our

during this collision but what our

during this collision but what our gravitational waves

gravitational waves

gravitational waves it started astrophysicists John Wheeler

it started astrophysicists John Wheeler

it started astrophysicists John Wheeler and his way to summarize general

and his way to summarize general

and his way to summarize general relativity he said space-time that’s

relativity he said space-time that’s

relativity he said space-time that’s matter how to move metal that’s

matter how to move metal that’s

matter how to move metal that’s space-time how to curve gravity needs to

space-time how to curve gravity needs to

space-time how to curve gravity needs to be understood as geometry and curved

be understood as geometry and curved

be understood as geometry and curved space-time and not as a force that

space-time and not as a force that

space-time and not as a force that exists in absolute space and time a Big

exists in absolute space and time a Big

exists in absolute space and time a Big Bird’s right okay they alone don’t

Bird’s right okay they alone don’t

Bird’s right okay they alone don’t really help us here I think so let’s try

really help us here I think so let’s try

really help us here I think so let’s try again visualizes in our

again visualizes in our

again visualizes in our three-dimensional world imagine a

three-dimensional world imagine a

three-dimensional world imagine a bowling ball Krauser and you roll it

bowling ball Krauser and you roll it

bowling ball Krauser and you roll it across a spandex sheet the spandex the

across a spandex sheet the spandex the

across a spandex sheet the spandex the two-dimensional representation of our

two-dimensional representation of our

two-dimensional representation of our three-dimensional world the bulling

three-dimensional world the bulling

three-dimensional world the bulling water curves of spandex into its third

water curves of spandex into its third

water curves of spandex into its third dimension creates a curved space

dimension creates a curved space

dimension creates a curved space this is somewhat similar to masters

this is somewhat similar to masters

this is somewhat similar to masters which curve space-time and deform the

which curve space-time and deform the

which curve space-time and deform the geometry we live in now we can add a

geometry we live in now we can add a

geometry we live in now we can add a second bowling ball to it the two can

second bowling ball to it the two can

second bowling ball to it the two can circle around each other like two

circle around each other like two

circle around each other like two massive stars or black holes can circle

massive stars or black holes can circle

massive stars or black holes can circle around each other similar to the bowling

around each other similar to the bowling

around each other similar to the bowling balls creating waves on the spandex the

balls creating waves on the spandex the

balls creating waves on the spandex the two stars and black holes create waves

two stars and black holes create waves

two stars and black holes create waves on space-time and these are the famous

on space-time and these are the famous

on space-time and these are the famous gravitational waves we just discovered

gravitational waves we just discovered

gravitational waves we just discovered 18 months ago but these waves are

18 months ago but these waves are

18 months ago but these waves are nothing you can see they’re much more

nothing you can see they’re much more

nothing you can see they’re much more like sound waves traveling across

like sound waves traveling across

like sound waves traveling across space-time or spandex sheet stretching

space-time or spandex sheet stretching

space-time or spandex sheet stretching and compressing it but the changes are

and compressing it but the changes are

and compressing it but the changes are incredibly small imagine you take a

incredibly small imagine you take a

incredibly small imagine you take a meter stick you shove it up into a

meter stick you shove it up into a

meter stick you shove it up into a million pieces

million pieces

million pieces now you take one of these pieces one

now you take one of these pieces one

now you take one of these pieces one micrometer thick 100 times thinner than

micrometer thick 100 times thinner than

micrometer thick 100 times thinner than your hair you take one of these pieces

your hair you take one of these pieces

your hair you take one of these pieces that you can barely see and chop it up

that you can barely see and chop it up

that you can barely see and chop it up another million times now we are 10 to

another million times now we are 10 to

another million times now we are 10 to the minus 12 meters or picometer hundred

the minus 12 meters or picometer hundred

the minus 12 meters or picometer hundred times smaller than the smallest atom to

times smaller than the smallest atom to

times smaller than the smallest atom to hydrogen atom is two with me really

hydrogen atom is two with me really

hydrogen atom is two with me really because we take this piece and chop it

because we take this piece and chop it

because we take this piece and chop it up another million times now we have

up another million times now we have

up another million times now we have thousand times smaller than the proton

thousand times smaller than the proton

thousand times smaller than the proton and these are the length changes that we

and these are the length changes that we

and these are the length changes that we can detect with libel and here’s how it

can detect with libel and here’s how it

can detect with libel and here’s how it works in principle we take a laser beam

works in principle we take a laser beam

works in principle we take a laser beam we split it up first we draw it again as

we split it up first we draw it again as

we split it up first we draw it again as some simple lines we split up send it

some simple lines we split up send it

some simple lines we split up send it out into a two orthogonal directions

out into a two orthogonal directions

out into a two orthogonal directions four kilometers away their mirrors

four kilometers away their mirrors

four kilometers away their mirrors reflect the laser beam back we combine

reflect the laser beam back we combine

reflect the laser beam back we combine the laser field again and we set it up

the laser field again and we set it up

the laser field again and we set it up correctly then the maximum of one wave

correctly then the maximum of one wave

correctly then the maximum of one wave and a meaning of the other wave that sit

and a meaning of the other wave that sit

and a meaning of the other wave that sit on top of each other and the laser beams

on top of each other and the laser beams

on top of each other and the laser beams will cancel each other out and would be

will cancel each other out and would be

will cancel each other out and would be dark at the dark port there’s no light

dark at the dark port there’s no light

dark at the dark port there’s no light coming out now in a gravitational wave

coming out now in a gravitational wave

coming out now in a gravitational wave changes the length of each of these arms

changes the length of each of these arms

changes the length of each of these arms they are not longer in sync they are

they are not longer in sync they are

they are not longer in sync they are kind of getting out of phase and some

kind of getting out of phase and some

kind of getting out of phase and some light starts to show up it’s a dark port

light starts to show up it’s a dark port

light starts to show up it’s a dark port this technique is called laser

this technique is called laser

this technique is called laser interferometry

interferometry

interferometry there’s a most sensitive way to measure

there’s a most sensitive way to measure

there’s a most sensitive way to measure any lengths changes okay this was

any lengths changes okay this was

any lengths changes okay this was elegant right I’ll show you a little

elegant right I’ll show you a little

elegant right I’ll show you a little movie some Bigley lines and brighter and

movie some Bigley lines and brighter and

movie some Bigley lines and brighter and dimmer spots coming up there and now

dimmer spots coming up there and now

dimmer spots coming up there and now everybody can run out here and did an

everybody can run out here and did an

everybody can run out here and did an instrument that can measure millions of

instrument that can measure millions of

instrument that can measure millions of a millionth of a millionth of a meter

a millionth of a millionth of a meter

a millionth of a millionth of a meter really know in principle it is that

really know in principle it is that

really know in principle it is that simple but the technology that we had to

simple but the technology that we had to

simple but the technology that we had to develop worldwide and which we developed

develop worldwide and which we developed

develop worldwide and which we developed in part also here at UF they used to

in part also here at UF they used to

in part also here at UF they used to build the most sensitive complex and

build the most sensitive complex and

build the most sensitive complex and complicated instrument humans ever built

complicated instrument humans ever built

complicated instrument humans ever built the details and science behind these

the details and science behind these

the details and science behind these instruments is overwhelming on its own

instruments is overwhelming on its own

instruments is overwhelming on its own and it is impossible to cover this in

and it is impossible to cover this in

and it is impossible to cover this in any presentation so let’s not try to

any presentation so let’s not try to

any presentation so let’s not try to explain these things here but what I

explain these things here but what I

explain these things here but what I want to say is that it took guts for

want to say is that it took guts for

want to say is that it took guts for scientific fathers to start on a journey

scientific fathers to start on a journey

scientific fathers to start on a journey now more than 50 years ago to detect

now more than 50 years ago to detect

now more than 50 years ago to detect these gravitational waves to prove

these gravitational waves to prove

these gravitational waves to prove Einstein wrong who thought that they

Einstein wrong who thought that they

Einstein wrong who thought that they will never be detected because they are

will never be detected because they are

will never be detected because they are so small let us summarize the last

so small let us summarize the last

so small let us summarize the last centuries we’ve studied the universe as

centuries we’ve studied the universe as

centuries we’ve studied the universe as our eyes and then with our telescopes we

our eyes and then with our telescopes we

our eyes and then with our telescopes we figured out that the visible light is

figured out that the visible light is

figured out that the visible light is only a small fraction of the

only a small fraction of the

only a small fraction of the electromagnetic spectrum and we observe

electromagnetic spectrum and we observe

electromagnetic spectrum and we observe the universe and all electromagnetic

the universe and all electromagnetic

the universe and all electromagnetic colors and frequencies ranging from the

colors and frequencies ranging from the

colors and frequencies ranging from the four microwaves to gamma rays we look at

four microwaves to gamma rays we look at

four microwaves to gamma rays we look at the universe but we never listen to it

the universe but we never listen to it

the universe but we never listen to it and the closer we look the more obvious

and the closer we look the more obvious

and the closer we look the more obvious it became that there are things out

it became that there are things out

it became that there are things out there that are hidden from sight like

there that are hidden from sight like

there that are hidden from sight like black holes so closing our eyes and

black holes so closing our eyes and

black holes so closing our eyes and starting to listen it’s a natural thing

starting to listen it’s a natural thing

starting to listen it’s a natural thing to do except that the sound is so feeble

to do except that the sound is so feeble

to do except that the sound is so feeble we first had to build detectors so

we first had to build detectors so

we first had to build detectors so naturally unimaginable sensitivity light

naturally unimaginable sensitivity light

naturally unimaginable sensitivity light but light was barely the beginning of

but light was barely the beginning of

but light was barely the beginning of our adventure into the sound of the

our adventure into the sound of the

our adventure into the sound of the universe we continued to improve the

universe we continued to improve the

universe we continued to improve the library tectors we started planning new

library tectors we started planning new

library tectors we started planning new ones we also plan to send a detector in

ones we also plan to send a detector in

ones we also plan to send a detector in space

space

space this space detector called Lisa will use

this space detector called Lisa will use

this space detector called Lisa will use three spacecraft separated by two and a

three spacecraft separated by two and a

three spacecraft separated by two and a half million kilometres and we play Star

half million kilometres and we play Star

half million kilometres and we play Star Wars and shoot laser beams between the

Wars and shoot laser beams between the

Wars and shoot laser beams between the satellites and use again laser

satellites and use again laser

satellites and use again laser interferometry to measure lengths

interferometry to measure lengths

interferometry to measure lengths changes ask gigantic as ten thousand

changes ask gigantic as ten thousand

changes ask gigantic as ten thousand proton diameters which by the way is

proton diameters which by the way is

proton diameters which by the way is still ten million times smaller than a

still ten million times smaller than a

still ten million times smaller than a human hair but this would be enough to

human hair but this would be enough to

human hair but this would be enough to detect gravitational waves from the

detect gravitational waves from the

detect gravitational waves from the biggest crashes in the universe the

biggest crashes in the universe the

biggest crashes in the universe the crashes between supermassive black holes

crashes between supermassive black holes

crashes between supermassive black holes of a million to 100 million solar masses

of a million to 100 million solar masses

of a million to 100 million solar masses which sit inside the center of nearly

which sit inside the center of nearly

which sit inside the center of nearly every galaxy in the universe

every galaxy in the universe

every galaxy in the universe so Lisa and I go after the history and

so Lisa and I go after the history and

so Lisa and I go after the history and evolution of black holes the heaviest

evolution of black holes the heaviest

evolution of black holes the heaviest and darkest objects in our universe

and darkest objects in our universe

and darkest objects in our universe their evolution is closely linked to the

their evolution is closely linked to the

their evolution is closely linked to the evolution of our galaxies and to

evolution of our galaxies and to

evolution of our galaxies and to structure formation in the universe

structure formation in the universe

structure formation in the universe itself but legal and especially Iza will

itself but legal and especially Iza will

itself but legal and especially Iza will also see many other signals but this

also see many other signals but this

also see many other signals but this should be a topic of another talk this

should be a topic of another talk this

should be a topic of another talk this new sense that we just opened up will

new sense that we just opened up will

new sense that we just opened up will open a new era in astronomy and

open a new era in astronomy and

open a new era in astronomy and astrophysics which will revolutionize

astrophysics which will revolutionize

astrophysics which will revolutionize again our understanding of the universe

again our understanding of the universe

again our understanding of the universe thanks

”

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