Photon
Transcript
00:00:00This is the final effect of the mask.
00:00:27We really try to be as successful as possible in this.
00:00:32In my opinion, this is a marriage, looking for ways to describe this relationship.
00:00:41Let's change the subject.
00:00:44After your last success, you became very famous.
00:00:47But you became famous much earlier.
00:00:50A series of lectures for people unfamiliar with the world of science.
00:00:55You've been growing up in a strict environment.
00:01:00But...
00:01:02Yes, I remember those meetings.
00:01:10Before we go through the story from the beginning,
00:01:14it is worth saying a few words about the space in which I will show the visualization.
00:01:19This is a warm-up for the mind. It will last two minutes.
00:01:24Let's look at a point. It's a simple object.
00:01:27The only thing that can be simpler is its absence.
00:01:31There is.
00:01:33There isn't.
00:01:34There is.
00:01:36There isn't.
00:01:38There is.
00:01:40It's hard to find a simpler distinction.
00:01:45Let's give the point some freedom.
00:01:48The first in the history of space.
00:01:51And now it can be here,
00:01:55here,
00:01:56or here,
00:01:59here.
00:02:10To be the first continuous movement, you need time and space.
00:02:21If I turn the view, things are different.
00:02:24The initial symmetry is broken.
00:02:27How the object looks depends on the point of view.
00:02:31So we have a point in time and space.
00:02:34It's enough for what I'm about to show to make sense.
00:02:38Where did time, space and why do we have anything instead of nothing come from?
00:02:44Science has no answer to that.
00:02:46Some religions do.
00:02:48Let's look at a fragment of time and space.
00:02:51Let's make it a bit denser.
00:02:57This gray cloud is just to make it easier to see.
00:03:00The sound, too.
00:03:01It's just shown like that.
00:03:03Nobody knows what space is really made of.
00:03:07I'm starting with dots.
00:03:09Everyone goes crazy separately, like noise on TV, without communication.
00:03:13Only when I add such connectors, a kind of glue,
00:03:19neighbors start to get infected with their movement.
00:03:23It's the first space where cause and effect work.
00:03:26Only now you can say anything about the future or the past of this dot.
00:03:36And it gets more interesting.
00:04:48Time and space
00:04:59After the warm-up, let's talk about the phenomenon of life since the beginning of the Universe.
00:05:11The very beginning is probably infinite energy,
00:05:15a scandalous temperature and time-space friction.
00:05:25And the first differences are separated,
00:05:28just like dirty foam is separated from boiling water.
00:05:36Gravitational waves.
00:05:38I separate the gravitational field from the rest of the noise and we have something like that.
00:05:45Graviton
00:05:53Graviton
00:05:55Not even a nanosecond passes and there are already new disturbances.
00:05:59It's pluons.
00:06:01But another particle is released here.
00:06:03Higgs boson.
00:06:05Or a divine particle.
00:06:15Higgs boson
00:06:28Probably, when the Higgs field appears,
00:06:31there are monstrous tensions and clashes.
00:06:40It's inflation.
00:06:45Higgs boson
00:06:52After a sudden expansion, matter does not decompose smoothly.
00:06:56In the cosmic scale, time-space clashes arise everywhere,
00:07:00such as in the winter at Moszno.
00:07:03In the quantum scale, the filled Higgs field seems to slow down the expansion.
00:07:07The remaining fields are replaced by new, distinct fluctuations.
00:07:11For example, the first quarks.
00:07:14Small particles vibrate among the gluons.
00:07:26Photons and weak bosons W and Z are released.
00:07:30Photons and weak bosons W and Z are released.
00:07:38A new field of electrons and their perfect opposites,
00:07:41positrons, is also emerging.
00:07:45A free electron is quite difficult to show,
00:07:48because in every frame of the film it can be somewhere else.
00:07:51To simplify, an electron or another particle
00:07:54can be shown in space and its picture is sharp.
00:07:58But then we don't know anything about its direction of travel.
00:08:02Or I know the direction, but I lose focus.
00:08:08We can never have both information at the same time with great accuracy.
00:08:13Photons and weak bosons W and Z
00:08:26And now you can see how quarks connect with each other.
00:08:29They are held by a huge force generated by bubbling gluons.
00:08:33In this way, new energy balls are created,
00:08:36lasting in time.
00:08:39They are called protons or neutrons.
00:08:42It depends on how quarks are held.
00:08:45Energy balls are passing by,
00:08:48because it is still too hot for them to stick together.
00:08:51After cooling, some of them stick together.
00:09:05A field of photons is buzzing around.
00:09:08They can't move freely, because they keep hitting other objects,
00:09:11e.g. electrons.
00:09:15If we could look at such a world from the outside,
00:09:18it would be a fog, suffocating radiation.
00:09:22The temperature is still falling.
00:09:25After a few million years, it is so cold,
00:09:28that free electrons start to stick to those energy balls.
00:09:31Stable bonds are formed.
00:09:37In a few billion years, people will call them hydrogen atoms.
00:09:45Photons trapped in this way,
00:09:48are shooting in all directions.
00:09:51A religious man will say,
00:09:54that light has become.
00:09:57For the next billions of years,
00:10:00the Universe is still expanding.
00:10:03Energy balls, i.e. atoms, are flying everywhere.
00:10:10An atom is a wave,
00:10:13with very specific parameters.
00:10:16First, I will mention the proportions of their size.
00:10:19They are incredible.
00:10:23If an atomic nucleus is the size of a minister's head,
00:10:26an electron cloud is the size of a trinity.
00:10:31If the cloud was smaller,
00:10:34everything would fall apart, and we wouldn't be here.
00:10:37Now, please focus your gaze on your thumb,
00:10:40on your nail.
00:10:43A few billions of billions of atoms
00:10:46on the nail's corner.
00:10:49You have to train in such mental jumps.
00:10:58Quarks held by strong gluons are protons and neutrons.
00:11:01These, combined with each other,
00:11:04create a super-stable bond called an atomic nucleus.
00:11:08An additional charged nucleus
00:11:11spreads electromagnetic fields.
00:11:14A negative electron falls into this trap.
00:11:17In order to maintain the continuity of the whole nucleus,
00:11:20the electron spreads around the nucleus.
00:11:25This is why the common idea of an atom as small
00:11:28is called a ball.
00:11:31It is a big simplification.
00:11:34It is more like a ball of fog,
00:11:37thickening closer to the nucleus.
00:11:43A different amount of protons and neutrons
00:11:46create a different shape of the fog in the orbit.
00:11:49I didn't invent this.
00:11:52You can see it directly under a special AFM microscope.
00:11:55And this is beautiful in physics.
00:11:58Theoretical fun on paper is covered with what you see in a microscope.
00:12:10This will be called carbon one day.
00:12:13This is the difference between collision and bonding.
00:12:16This is the difference between chemistry
00:12:19and the possibility of bonding so many molecules.
00:12:22Let's add 92 protons.
00:12:25The cloud of electrons takes a disturbingly complicated shape.
00:12:28The cloud of electrons takes a disturbingly complicated shape.
00:12:31Despite everything, the nucleus is unstable.
00:12:34It spits photons everywhere.
00:12:37They vibrate aggressively.
00:12:44Atoms collide with each other all the time.
00:12:47Atoms collide with each other all the time.
00:12:50Finally, the photon exchange and direction of motion are affected.
00:12:53Finally, the photon exchange and direction of motion are affected.
00:12:59This is the simplest collision.
00:13:02The problem is that it can go in another direction.
00:13:05For example, the emitted photon can jump this way or that way.
00:13:09There are many possibilities. Too many.
00:13:13Accurate calculation of the angles of collision of electrons
00:13:16is ordered by the fastest computers.
00:13:22However, after calculating several dozen diagrams of collisions,
00:13:25you can get an approximation sufficient to satisfy human needs.
00:13:28you can get an approximation sufficient to satisfy human needs.
00:13:31Electric sockets, computers, washing machines.
00:13:34In the past, these events were calculated manually
00:13:37so that you could turn on the light on the staircase.
00:13:40Does anyone know who we owe this to?
00:13:52I'm thinking about sodium cells,
00:13:55and helium and hydrogen atoms are concentrated
00:13:58in the first structures visible to the naked eye.
00:14:10Nebulon
00:14:26This concentration of atoms will be called nebulon.
00:14:29This concentration of atoms will be called nebulon.
00:14:40Nebulon
00:14:48The purpose is not to show the color.
00:14:51Color is a human invention.
00:14:54To make the color visible, you need an observer with a brain
00:14:57able to create the impression of red.
00:15:00Otherwise, it's just an anonymous vibration like a sound without witnesses.
00:15:03So, the shots should be black and white
00:15:06until the spiders appear.
00:15:09But as spectators, you are observers
00:15:12and you have brains, so I'll let the color in now.
00:15:39Nebulon
00:15:49The range of waves seen by our eyes is limited.
00:15:52Let's say a hand is drifting here.
00:15:55Let's say a hand is drifting here.
00:15:58We are looking at very dense waves of photons called Röntgen waves.
00:16:01Slightly longer waves are ultraviolet.
00:16:04We can almost see it.
00:16:07Then well-known blue.
00:16:10Even longer waves are green.
00:16:13Then red.
00:16:16Slightly longer waves and we miss it again.
00:16:19It's infrared, received by touch as heat.
00:16:28Even longer waves are microwaves.
00:16:31The crest is a few centimeters.
00:16:34They have a very poor image.
00:16:37Waves over a meter long are radio waves.
00:16:40They are invisible, but the radio will receive them.
00:16:43Someone's hand is a bit too small to reflect them well.
00:16:52We have just reached the first visible structures
00:16:55that every normal viewer knows.
00:16:58It will be easier from now on.
00:17:04Röntgen
00:17:34Röntgen
00:17:40This is one of the first galaxies that were created.
00:17:53Why is it even possible to see an event from 13 billion years ago?
00:17:56Why is it even possible to see an event from 13 billion years ago?
00:17:59Because when we look deep into the sky, we look into the past.
00:18:02Only now photons emitted in those times are coming to us.
00:18:05Only now photons emitted in those times are coming to us.
00:18:08What's worse, our time-space is expanding.
00:18:11So some of them will not catch up with us.
00:18:14This is how the edge of our observation is created.
00:18:17Looking at these borders, the last thing we see
00:18:20is a wall of photons called background radiation.
00:18:23is a wall of photons called background radiation.
00:18:26If you want to experience it, turn on the TV on an empty channel.
00:18:29This is mostly background radiation from the beginning of the Universe.
00:18:32This is mostly background radiation from the beginning of the Universe.
00:18:38There are also Kielce-sized balls.
00:18:41These are pulsars, they rotate 700 times per second.
00:18:44Imagine what would happen
00:18:47if you took all the PKP wagons
00:18:50and compressed them to the size of a sugar cube.
00:18:54This pulsar envelops matter from a nearby star, a vampire.
00:18:57This pulsar envelops matter from a nearby star, a vampire.
00:19:04Through constant gravitational pull
00:19:07a whole menagerie of creatures is created
00:19:10in different stages of reproduction.
00:19:23This pulsar envelops matter from a nearby star, a vampire.
00:19:26This pulsar envelops matter from a nearby star, a vampire.
00:19:29This pulsar envelops matter from a nearby star, a vampire.
00:19:32This pulsar envelops matter from a nearby star, a vampire.
00:19:35This pulsar envelops matter from a nearby star, a vampire.
00:19:38This pulsar envelops matter from a nearby star, a vampire.
00:19:41This pulsar envelops matter from a nearby star, a vampire.
00:19:44This pulsar envelops matter from a nearby star, a vampire.
00:19:47This pulsar envelops matter from a nearby star, a vampire.
00:19:50This pulsar envelops matter from a nearby star, a vampire.
00:19:53This pulsar envelops matter from a nearby star, a vampire.
00:19:56This pulsar envelops matter from a nearby star, a vampire.
00:19:59This pulsar envelops matter from a nearby star, a vampire.
00:20:02This pulsar envelops matter from a nearby star, a vampire.
00:20:05This pulsar envelops matter from a nearby star, a vampire.
00:20:08This pulsar envelops matter from a nearby star, a vampire.
00:20:11This pulsar envelops matter from a nearby star, a vampire.
00:20:14This pulsar envelops matter from a nearby star, a vampire.
00:20:17This pulsar envelops matter from a nearby star, a vampire.
00:20:20This pulsar envelops matter from a nearby star, a vampire.
00:20:23This pulsar envelops matter from a nearby star, a vampire.
00:20:26This pulsar envelops matter from a nearby star, a vampire.
00:20:29This pulsar envelops matter from a nearby star, a vampire.
00:20:32This pulsar envelops matter from a nearby star, a vampire.
00:20:35This pulsar envelops matter from a nearby star, a vampire.
00:20:38This pulsar envelops matter from a nearby star, a vampire.
00:20:41This pulsar envelops matter from a nearby star, a vampire.
00:20:44A few days later.
00:20:57Millions of years pass.
00:21:00Some stars lose their balance and begin to lose their pressure.
00:21:03Here you can see that the star is softening.
00:21:06The death of a big star is a spectacle.
00:21:14A few days later.
00:21:29A series of shocks erodes a layer into space.
00:21:37Among the shocks there are also carbon and oxygen atoms.
00:21:40The same ones you are made of.
00:21:43The heavier atoms join other thickenings,
00:21:46creating new lumps.
00:21:49Planets hang in the void.
00:21:52Let's talk about nothing for a moment.
00:21:55Let's take a piece of the void.
00:21:58Is it empty?
00:22:01Or what is between two nearby atoms?
00:22:07I don't want to talk about the void as a physics teacher,
00:22:10but you see it as an abstraction that doesn't concern you.
00:22:13It's better to show it on something common.
00:22:18The artist brings alcohol home.
00:22:22The net is made of black plastic.
00:22:25These are mainly chains of hydrogen and carbon atoms.
00:22:30We look at the place where the net weighs on his finger.
00:22:33The tensed atoms emit virtual photons.
00:22:36Thanks to them, the net will not penetrate through the finger.
00:22:39Thanks to them, we have hardness.
00:22:42It seems that we can bring it closer to infinity.
00:22:45It's a recipe for a mathematical disaster.
00:22:48To not go crazy, there are a few propositions.
00:22:51For a moment it helps us to determine the smallest possible length
00:22:54and assume that the smallest pixel in the world
00:22:57has the so-called Planck length.
00:23:00Things smaller than it are indistinguishable.
00:23:03Another proposition is this.
00:23:06Pay attention to this noise.
00:23:09It's a quantum foam.
00:23:12Time-space loops are blinking.
00:23:15Our three-dimensional space and time are emanating from this blinking.
00:23:18Or we can assume that the smallest point in space
00:23:21has something more.
00:23:24Additional dimensions are twisted into shapes.
00:23:27They determine the way atoms vibrate in three dimensions.
00:23:31Let's go back to events chronology.
00:23:34Some of the galaxies collide.
00:23:37A rapid process throws star dust into the void.
00:23:54In the orbit of one of the stars,
00:23:58dust thickens into small lumps,
00:24:01creaking chambers.
00:24:04This one is the size of a fist.
00:24:07After a few million years, it is the size of Germany.
00:24:12Millions of years pass
00:24:15and gravity slowly forces the shape of a ball.
00:24:27The big ball is huge.
00:24:30The big ball has a massive base
00:24:33that spans 5 million light-years.
00:24:40The big ball is so huge that it's impossible to measure it.
00:24:43If you can measure it, you can measure it, too.
00:24:49The difference is that the bigger ball
00:24:52is smaller than the smaller.
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00:43:25What time? What does it mean?
00:43:30You have a young wife, a former student, a one-year-old son.
00:43:37What time do you have for them?
00:43:39Well, but...
00:43:40I'm sorry, because I don't...
00:43:42I don't know how you know.
00:43:44What does it have to do with our conversation?
00:43:47I'm just asking in a human way.
00:43:49Do you find time for your loved ones in this burden of duties?
00:43:53I find or I don't, but it really has nothing to do with this conversation.
00:44:00Well, what if we turned off the recording?
00:44:02But I'm sorry, don't you understand what it means, I can't?
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01:36:25Photon.
01:36:40Space flights are mainly
01:36:42setting up new transmission stations.
01:36:46But even the largest transports
01:36:48take off without scientific witnesses.
01:36:51For some time now,
01:36:52individual bodies no longer exist.
01:36:55There are only patterns of activity in the network.
01:37:12Oh, this is the second level of civilization.
01:37:15Conectom collects energy for it
01:37:17from nearby stars.
01:37:20Is there still room for less practical things?
01:37:23Music or a sense of humor?
01:37:26It's hard to say.
01:37:28The old world looks extremely functional.
01:37:31You don't need colors,
01:37:32because there are no eyes.
01:37:36Servers are also placed
01:37:37in an extremely efficient way.
01:37:39It's a sad sight for us,
01:37:41but we only see
01:37:42the external effect of these actions.
01:37:45Because what happens inside these networks
01:37:47is no longer understood by a single brain.
01:37:50There's not even anything to try.
01:37:53What's next?
01:37:54Of course, there are mistakes.
01:37:59It happens that all the planets
01:38:01are covered with something
01:38:03like a paper clip.
01:38:06Because the local network
01:38:08has made the wrong nanomachines.
01:38:11Maybe it's a form of sense of humor.
01:38:16And then,
01:38:17this is already a shirt.
01:38:20And then,
01:38:21this is already a schizophrenic nightmare.
01:38:24Civilization of the third level.
01:38:27Cones for collecting energy from galaxies
01:38:30are placed in large areas of space.
01:38:33Without antennas and light sources.
01:38:35There is less and less matter.
01:38:37It starts to resemble a thinking vacuum
01:38:39with less and less random flux.
01:38:42There are suspicions that
01:38:44the entertainment activity of the network
01:38:46is a simulation of the old times.
01:38:48For example, life on Earth.
01:38:56Just like we used to dig in atoms,
01:38:59here we dig in dimensions.
01:39:05The old sun and its surroundings
01:39:07have long since gone,
01:39:09sucked out of the remains of photons.
01:39:12The creature takes over larger and larger areas.
01:39:16I don't know,
01:39:17I can still try to show it
01:39:19as perfectly arranged points of transfer.
01:39:23The new vacuum is shaking incomprehensibly.
01:39:27I don't know what's next.
01:39:46Transcribed by ESO. Translated by —
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