A Fleeting Shadowed Sky

“Hey, Uncle Sy, I’ve got a what‑if for you.”

“What’s that, Teena?”

“Suppose we switched Earth’s air molecules with helium. No, wait, except for the oxygen molecules. I know we need them.”

“First off, a helium-oxygen atmosphere wouldn’t last very long, not on the geological time scale. That’s an unstable situation.”

“Why, would the helium burn up like I’ve seen hydrogen do?”

“No, helium doesn’t burn. Helium atoms are smug. They’re happy with exactly the electrons they have. They don’t give, take or share electrons with oxygen or anything else. No, the issue is that helium’s so light.”

“What difference does that make?”

“The oxygen and helium won’t stay mixed together.”

“The air’s oxygen and nitrogen molecules are all mixed together. They told us that in Science class.”

“That’s correct. But oxygen and nitrogen molecules weigh nearly the same. It would take eight balloon‑fulls of helium to match the weight of one balloon‑full of oxygens. Suppose you had a bunch of equal‑weighted marbles, say red ones and blue ones. Pretend you pour them into a big bucket and stir them around like an atmosphere does. Which color would wind up on top?”

“Both, they’d stay mixed together.”

“Uh-huh. Now replace the blue marbles with marble‑sized ping‑pong balls and stir well.”

“The heavy marbles slide to the bottom. The light balls need to be somewhere so they get bullied up to the top.”

“Exactly. That’s what the oxygen molecules would do — sink down toward the ground and shove the helium atoms up to the top of the atmosphere. Funny thing though — the shoving happens faster than the sinking.”

“Why’s that?”

“It’s the mass thing again. At any given temperature, helium atoms in a gas zip around four times faster than oxygen molecules do. Anyway, the helium atoms that arrive up top won’t stay there.”

“Where else would they go?”

“Anywhere else, basically. Have you heard the phrase, ‘escape velocity‘?”

“It has something to do with rockets, doesn’t it?”

“Well, them, too. The general idea is that once you reach a certain threshold speed relative to a planet or something, you’re going too fast for its gravity to pull you back down. There’s a formula for calculating the speed. The fun thing is, the speed depends on the mass of what you’re escaping from and your distance from the object’s center, but it doesn’t depend on your own mass. It applies to everything from rockets to gas molecules.”

“And we were just talking about helium being zippy. Is it zippy enough to escape Earth?”

“Good thinking! That’s exactly where I was going. The answer is, ‘Maybe.’ It depends on temperature. Warm molecules are zippy, cold molecules not so much. At the same temperature, light molecules are zippier than heavy ones. There’s a chart that shows thresholds for different molecules escaping from different planets. Earth could hold onto its helium atoms, but only if our atmosphere were more than a hundred degrees colder than it is. Warm as we are, bye‑bye helium.”

“How long would that take?”

“That’s a complicated question with lots of ‘It depends’ in the answer. Probably the most important has to do with water.”

“I didn’t say anything about water, just helium and oxygen.”

“I know, but much of Earth’s weather is driven by water vaporizing or condensing or just carrying heat from place to place. Water‑powered hurricanes and even big thunderstorms stir up the atmosphere enough to swoosh helium up to bye‑bye territory. On the other hand, suppose our helium‑Earth is dry. The atmosphere’s layers would be mostly stable, light atoms would be slow to rise. We’d have a very odd‑looking sky.”

“No clouds.”

“Pretty much. But it wouldn’t be blue, either.”

“Would it be pink? I like pink.”

“Sorry, sweetie, it’d be dark dark blue, some lighter near the horizon. Light going past an atomic or molecular particle can scatter from its temporarily distorted electron cloud. Nitrogen and oxygen molecules distort more easily than helium atoms do. Earth skies are blue thanks to sunlight scattered by oxygen and nitrogen. Helium skies wouldn’t have much of that.”

~ Rich Olcott

  • Thanks again to Xander, who asked a really good helium question.

A Blast from The Past

Back at the beginning of the Plague Era when things were (mostly) shut down, I started posting daily memes to reflect my shelter‑in‑place state of mind. Here’s the first one

The initial day‑count reflected my expectation that the lock-down would last less than a month. Hah!

I gave up on numbers for a while

April rolled around and I went topical

Remember the Great Toilet Paper Shortage?

I’ll never know how many readers got this one, but I like it

This is a Physics/Astronomy/Cosmology blog so I posted this to stay on‑topic…

This was meant to be satire, but I saw posts from folks actually doing it…

Yes, cabin fever is a thing

It was a time for sudden insights

We all got used to e-meetings

and smart speakers, if only for the conversations

Soon I had to go for higher numbers

Staying at home had its bright side (unless you’re invested in Big Oil)

And its bad‑omen side

The seasons passed and the day count increased…

Ending this retrospective with one of my favorites

~~ Rich Olcott

In Which Tone of Voice?

“Oh. OH! Wow, Uncle Sy, this changes everything!”

“Which ‘this,’ Teena?”

The resonator thing. Our music teacher, Ms Searcy, has been going on about us singing too much in our heads. I thought she’s been saying we’re thinking about the music too much and should just let the singing happen.”

“Sounds very Zen.”

“I’m too young to know Zen stuff. But now I think maybe she’s saying we’re using those head resonators you just told me about — singing with our sinuses and nasal cavities instead of somewhere else. She’s never been clear on what we can do about that.”

“You’re probably right. No music teacher since Harold Hill would try to get away with ‘think the music.’ I’m sure Ms Searcy’s complaint is about head tones as opposed to chest tones. If so, she’s got a good excuse for being unclear.”

“How can I have chest tones when you said vibrations come from my voice box and that’s above my chest?”

“Sound wave energy is about molecules colliding against any neighboring molecules. Up, down left, right — none of those matter. When air from your lungs makes your vocal cords buzz against each other, much of that buzzing goes up through your throat and head resonators. However, some of the buzz energy travels into your chest cavity. That’s your biggest resonator and it’s where your lowest tones come from.”

“I guess Ms Searcy wants us to send even more buzzing there, but how do we do that?”

“That’s a hard question. People have been interested in it since they started teaching singing and oratory to other people. We learned one part of the answer in medieval times when we began studying anatomy up close and personal. For instance, your voice box, which I really ought to call your larynx now we’re getting into detail, relates to about a dozen different muscles.”

“What’re the other parts?”

“The easiest part was kinesiology — figuring out what action each muscle supports. The hardest part was teaching a student how to feel and control the right muscles to make their voice do exactly what they want.”

“How can that be hard? I can flex my arm and leg muscles any time I want.”

“Can you make your larynx move up and down in your throat?”

“Easy.”

“That motion depends on a chain of muscles running between the back of your tongue and the top of your chest. One way to send buzzes downward is to activate the muscles that pull the larynx in that direction. Shorter distance makes for more efficient buzz transmission. It can also help to pull your head back a little. That tenses those pulled‑down tissues and improves transmission even more.”

<slightly deeper voice> “Like this?”

“That’s the idea. Learning to do that without having to pay attention to it is part of vocal training. Now, can you spread your toes out?”

“That’s weird. I can on my right foot but not my left.”

“Very common. Each foot has little tiny muscles, called intrinsic muscles, buried deep inside. Some people can control the whole set, some not so much. Your larynx has two pairs of intrinsic muscles that govern how your vocal cords work together. Some voice teachers claim the intrinsic muscles inside the larynx are the key to proper voice technique. Unfortunately, you can’t see them or get a feel for controlling them other then ‘keep trying things until you get it right and remember what you did.’ That’s Ms Searcy’s strategy. It’d be much harder with helium.”

“That’s right! Our voices with the balloons were all head tones. How come?”

“The speed of sound.”

“That’s a sideways answer, Uncle Sy.”

“Okay, this is more direct. We’ve said resonance was about waves whose wavelength just fit across a cavity. Picture two waves, the same number of waves per second, but the wave in helium travels about 3½ times faster than the one in air. The helium wave stretches about 3½ times farther between peaks. Whatever peaks per second your vocal cords make, in helium your chest cavity is 3½ times too small to resonate. Your head cavities, though, can resonate to overtones of those frequencies.”

“Squeaky overtones.”

~ Rich Olcott

When Sounds Rebound

<chirp chirp> “Moire here.”

“Hi, Uncle Sy.”

“Hi, Teena, How was the birthday party?”

“Pretty fun. We had balloons but Mom wouldn’t let us fly them into the sky.”

“Because animals might eat them when they come down, I suppose.”

“Yeah, that’s what she said. What we did was we untied the knotty part so we could breathe in the helium and sing squeaky Happy Birthdays. It didn’t make much difference to my voice but Brian’s came out weird ’cause his voice is breaking anyway. It was almost a yodel.”

“I thought you didn’t like Brian any more.”

“That was last month, Uncle Sy. He ‘poligized on accounta he’s still learning social skills. We had fun playing with the sounds.”

“Sure you did. Do you remember the slide whistle I gave you once?”

“That was a long time ago. It was fun until Brian bent the slider and it didn’t work any more.”

“No surprise. How’d you make it give a high note?”

“I’d push the slider all the way in. Slider-out made a low note, but Brian could make a high note even there if he blew really hard.”

“Well, he would. It all has to do with resonant cavities.”

“I don’t have any cavities! Mom makes sure I brush and floss every day. And what’s resonant?”

“You don’t have dental cavities but there are other kinds. ‘Cavity‘ is another word for ‘hole‘ and some of them are important. You breathe through two nasal cavities that join up to be your posterior nasal cavity and that connects to sinus cavities in your skull and down to your voice box and lungs. Your mouth cavity resonates with all those cavities and vibrations from your voice box to make your speaking sounds.”

“That’s twice you used that ‘resonate‘ word I don’t know.”

“Break it down. ‘–son–‘ means ‘sound,’ like ‘sonic.’ Then—”

“‘Re–‘ means ‘again‘ like ‘rebuild‘ so resonate is sounding again like an echo.”

“Right. Except a resonant cavity is picky about what sounds it works with. Here, I’m sending you a video. Did you get it?”

“Yeah, I see a couple of wiggly lines. Wait, the blue line stays the same size but the orange line gets littler until it’s all gone and then the picture goes yellow and starts over.”

“What happens over on the right‑hand side?”

“The blue line bounces back from zero but the orange line waves all over the place. Is that how sound works?”

“Sort of. The air molecules in a sound wave don’t go up‑and‑down, they go to‑and‑fro. The wiggly lines are a graph of where the energy is. Where the molecules bunch together they bang into each other more often than in the in‑between places. In open air the energy pushes along even though the molecules stay pretty much where they are. In a resonant cavity, sounds are trapped like the blue line if they have just the right wavelength. A cavity’s longest trappable wavelength is its lowest note, called its fundamental. The energy in the fundamental is sustained as long as new energy’s coming in.”

“What happens to the orange line?”

“It doesn’t get a chance to build up. The energy in those waves spreads out until the wave just isn’t any more.”

“Aww, poor wavey. Wait, what about when Brian blows extra‑hard and gets that high note?”

“He gives the commotion inside the whistle enough energy to excite a second trapped wave with twice the number of crowded places. That’s called an overtone of the fundamental. Sometimes you want to do that, sometimes you don’t.”

“Brian always did on the whistle.”

“Well, he would. The resonant cavity thing also explains why Brian’s voice breaks and how talking works. Your windpipe is a resonating cavity. Brian’s windpipe has grown just large enough that sometimes it resonates in his new fundamental and sometimes switches to some other fundamental or overtone. Talking depends on tuning the resonances inside your mouth cavity. Try saying ‘ooo‑eee‘ while holding your lips steady in ‘ooo‘ position. On ‘eee‘ your tongue rises up to squeeze out the low‑pitched long waves in ‘ooo‘, right?”

oooeeeoooeeeooo

  • Thanks to Xander, whose question inspired this story arc.

~ Rich Olcott

Why Physics Is Complex

“I guess I’m not surprised, Sy.”

“At what, Vinnie?”

“That quantum uses these imaginary numbers — sorry, you’d prefer we call them i‑numbers.”

“Makes no difference to me, Vinnie. Descartes’ pejorative term has been around for three centuries so that’s what the literature uses. It’s just that most people pick up the basic idea more quickly without the woo baggage that the real/imaginary nomenclature carries along. So, yes, it’s true that both i‑numbers and quantum mechanics appear mystical, but really quantum mechanics is the weird one. And relativity.”

“Wait, relativity too? That’s hard to imagine, HAW!”

“Were you in the room for Jim’s Open Mic session where he talked about Minkowski’s geometry?”

“Nope, missed that.”

“Ah, okay. Do you remember the formula for the diagonal of a rectangle?”

“That’d be the hypotenuse formula, c²=a²+b². Told you I was good at Geometry.”

“Let’s use ‘d‘ for distance, because we’re going to need ‘c‘ for the speed of light. While we’re at it, let’s replace your ‘a and ‘b‘ with ‘x‘ and ‘y,’ okay?”

“Sure, why not?”

<casting image onto office monitor> “So the formula for the body diagonal of this box is…”

“Umm … That blue line across the bottom’s still √(x²+y²) and it’s part of another right triangle. d‘s gotta be the square root of x²+y²+z².”

“Great. Now for a fourth dimension, time, so call it ‘t.’ Say we’re going for light’s path between A at one moment and B some time t later.”

“Easy. Square root of x²+y²+z²+t².”

“That’s almost a good answer.”

“Almost?”

“The x, y and z are distance but t is a duration. The units are different so you can’t just add the numbers together. It’d be like adding apples to bicycles.”

“Distance is time times speed, so we multiply time by lightspeed to make distance traveled. The formula’s x²+y²+z²+(ct)². Better?”

“In Euclid’s or Newton’s world that’d be just fine. Not so much in our Universe where Einstein’s General Relativity sets the rules. Einstein or Minkowski, no‑one knows which one, realized that time is fundamentally perpendicular to space so it works by i‑numbers. You need to multiply t by ic.”

“But i²=–1 so that makes the formula x²+y²+z²–(ct)².”

“Which is Minkowski’s ‘interval between an event at A and another event at B. Can’t do relativity work without using intervals and complex numbers.”

“Well that’s nice but we started talking about quantum. Where do your i‑numbers come into play there?”

“It goes back to the wave equation— no, I know you hate equations. Visualize an ocean wave and think about describing its surface curvature.”

“Curvature?”

“How abruptly the slope changes. If the surface is flat the slope is zero everywhere and the curvature is zero. Up near the peak the slope changes drastically within a short distance and we say the surface is highly curved. With me?”

“So far.”

“Good. Now, visualize the wave moving past you at some convenient speed. Does it make sense that the slope change per unit time is proportional to the curvature?”

“The pointier the wave segment, the faster its slope has to change. Yeah, makes sense.”

“Which is what the classical wave equation says — ‘time‑change is proportional to space‑change’. The quantum wave equation is fundamental to QM and has exactly the same form, except there’s an i in the proportionality constant and that changes how the waves work.” <casting a video> “The equation’s general solution has a complex exponential factor eix. At any point its value is a single complex number with two components. From the x‑direction, the circle looks like a sine wave. From the i‑direction it also looks like a sine wave, but out of phase with the x‑wave, okay?”

“Out of phase?”

“When one wave peaks, the other’s at zero and vice‑versa. The point is, rotation’s built into the quantum waves because of that i‑component.” <another video> “Here’s a lovely example — that black dot emits a photon that twists and releases the electromagnetic field as it moves along.”

~ Rich Olcott

…With Imaginary Answers

“I’ve got another solution to Larry’s challenge for you, Vinnie.”

“Will I like this one any better, Sy?”

“Probably not but here it is. The a‑line has unit length, right?”

“That’s what the picture says.”

“And the b‑line also has unit length, along the i‑axis.”

“Might as well call it that.”

“And we’ve agreed it’s a right triangle because all three vertices touch the semicircle. A right triangle with two one‑unit sides makes it isosceles, right, so how big is the ac angle?”

“Isosceles right triangle … 45°. So’s the bc angle even though it don’t look like that in the picture.”

“Perfect. Now let me split the triangle in two by drawing in this vertical line.”

“That’s its altitude. I told you I remember Geometry.”

“So you did. Describe the ac triangle.”

“Mm, it’s a right triangle because altitudes work that way. We said the ac angle is 45° which means the top angle is also 45°.”

“What about length ca?”

“Gimme a sec, that’s buried deep. … If the hypotenuse is 1 unit long then each side is √½ units.”

“Vinnie, I’m impressed. So what’s the area of the right half of the semicircle?”

“That’s a quarter‑circle with radius ca which is √½ so the area would be ¼πca² which comes to … π/8.’

“Now play the same game with the b‑side.”

“Aw, geez, I see where you’re going. Everything’s the same except cb has an i in it which is gonna get squared. The area’s ¼πcb² which is … ¼π(i√½)² which is –π/8. Add ’em both together and the total area comes to zero again. … Wait!”

“Yes?”

“You said the i‑axis is perpendicular to everything else.” <sketching on the back of the card> “That’s not really a semicircle, it’s two arcs in different planes that happen to have the same center and match up at one point. The c‑line’s bent. Bo‑o‑o‑gus!”

“I said you wouldn’t like it. But I didn’t quite say ‘perpendicular to everything else‘ because it’s not. The problem is that the puzzle depends on a misleadingly ambiguous diagram. The only perpendicular to i that I worked with was the a‑line. You’ve also got it perpendicular to part of the c‑line.”

“Sy, if these i-number things are ambiguous like that, why do you physics and math guys spend so much time with them? And do they really call them i‑numbers?”

“Ya got me. No, they’re actually called ‘complex numbers,’ because they are complex. The problem is with what we call their components.”

“Components plural?”

“Mm‑hm. Mathematicians put numbers in different categories. There’s the natural numbers — one, two, three on up. Extend that through zero on down and you have the integers. Roll in the integer/integer fractions and you’ve got the rational numbers. Throw in all the irrationals like pi and √2 and you’re got the full number line. They call that category the reals.”

“That’s everything.”

“That’s everything along the real number axis. Complex numbers have two components, one along the real number line, the other along the perpendicular pure i‑number line. A complex number is one number but it has both real and i components.”

“If it’s not real, it’s imaginary, HAW!”

“More correct than you think. That’s exactly what the ‘i‘ stands for. If Descarte had only called the imaginaries something more respectable they wouldn’t have that mysterious woo‑quality and people wouldn’t have as much trouble figuring them out. Complex numbers aren’t mysterious or ambiguous, they’re just different from the numbers you’re used to. The ‘why’ is because they’re useful.”

“What good’s a number with two components?”

“It’s two for the price of one. The real number line is good for displaying a single variable, but suppose one quantity links two variables, x and y. You can plot them using Descartes’ real‑valued planar coordinates. Or you could use complex numbers, z=x+iy and plot them on the complex plane. Interesting things happen in the complex plane. Look at the difference between ex and eix.”

“One grows, the other cycles.”

“Quantum mechanics depends on that cycling.”

~ Rich Olcott

A Complex Question

A familiar footstep in the hall outside my office. “Door’s open, Vinnie, c’mon in.”

“Hi, Sy. Brought you something.” <lays a card on my desk> “So the question is, what’s the area inside the semicircle?”

<thoughtful pause> “Zero.”

“Dang, that’s both you and Larry say it’s zero. I don’t see it. ‘Splain, okay?”

“Larry gave you this?’

“Yeah. Can’t be zero area, it’s right there all spread out. How do you figure zero?”

“Start with the diagonal lines. The ‘a‘ line has a length of one unit, right?”

“The picture says so, but what’s i about on line ‘b‘?”

“That’s a special number, defined to be the solution x of the equation x²+1=0. Taking square roots, x=i and i²+1=0. I know you hate equations, but bear with me.”

<grumble> “Okay, go ahead.”

“If we had the radius r, the area would be ½πr². Line c is the diameter so the radius is r=c/2. We can get c by solving the triangle. We know it’s a right triangle because all three vertices touch a semicircle, right?”

“Geometry I remember; it was algebra gave me fits.”

“Then you remember good old Pythagoras and his a²+b²=c² formula, which we can use here because it’s a right triangle. Plugging in the known lengths we get c²=1²+i²=i²+1. Look familiar?”

“Yeahhh, i²+1=0 from the definition so is zero. What if b was 3?”

“We’d have c²=1²+(3i)²=1+9=1–9=–8. If both a and b are 3, then c²=3²+(3i)²=9+9=9–9 and we’re back to c²=0. It’s just arithmetic, but enhanced with i and its special rules.”

“Wait. If c²=0 then c=0 and c‘s the diameter and if that’s zero then so’s the radius and the area. The whole thing shrinks to a point but it can’t ’cause it’s right there spread out in the picture. Is this sort of thing why they told us x²–1=0 has a solution but x²+1=0 doesn’t?”

“It’s closely related, because i is involved. Incidentally, they lied to you in that algebra class. They showed you that famous quadratic equation ax²+bx+c=0, right, along with the magic b²–4ac formula. If that formula is positive you’ve got two roots, they said, but if it’s negative there’s no root.”

“Sounds familiar. Where’s the lie?”

“The first part’s true: with 1=0 you’ve got a=1,b=0,c=–1 with two roots x=1 and x=–1. The lie is in the second part: with x²+1=0 you’ve got a=1,b=0,c=+1 with two roots x=i and x=–i. All of those are perfectly good solutions.”

“But i‘s not a number! I can’t have i apples and I can’t write a check for i dollars. Why even play with it?”

“The i‑numbers are numbers, just not counting numbers. They’ve been part of mainstream math ever since the early Renaissance. Algebra was almost a blood sport at the time. Academics in Italy used to issue public challenges to solve problems that they’d already solved secretly. There were duels to settle questions of priority. Bombelli systematized i‑number arithmetic while working out one limited class of cubic equations. Cardano compiled solutions from multiple authors, including Bombelli, into his book Ars Magna. Then he systematically added his own solutions to a catalog of cubic and quartic equations. The Old Guard refused to believe in either i‑numbers or negative numbers, but Cardano showed you can’t escape them if you’re doing serious algebra.”

“Not even negative numbers?”

“Nope. The negatives weren’t widely accepted until the Venetian trading houses forced the issue — negatives are implicit in the merchants’ newly‑invented double‑entry bookkeeping. i‑numbers weren’t considered respectable for hundreds of years.”

“Then what happened?”

“Several advances. Euler connected i with trigonometry. Add Descarte‘s coordinate system, Fourier‘s wave analysis and Leibniz‘ notational innovations. For example, plotting an i‑number helix in 3D gives you these sine waves. When I think ‘i‑axis‘ I think ‘perpendicular to other coordinates‘.”

“Like Las Vegas.”

“Similar.”

Cardano image by R. Cooper
from Wellcome Trust
under the CCA International license
  • Thanks to Lloyd Boyer who raised several good points.

~~ Rich Olcott

Cal’s Gallery

“Goodness, Cal, you’ve redone your interior decorations.”

“I got tired of looking at the blank wall opposite the cash register, Sy. Check out the gallery. Way at the end here’s the earliest one I’ve got, goes back to 2005.”

“Yeah, ray-marching each background pixel as it passed through the distorting gravity field. That was heavy-duty computer graphics back then.”


“Here’s another one from a year later. I like it better because you can pair up stars and stuff that show up on both sides of the Einstein ring.”


“This one’s famous, comin’ from the Interstellar movie. Funny, I can’t think of any black hole pictures before Interstellar that paid much attention to the accretion disk.”

“There certainly was a lot of that in the specialist literature, but you’re probably right for what leaked out to the pop‑sci press. Most of the published imagery was about how the gravity field distorts the figures behind it. That perpendicular handle was certainly a surprise.”


“This one’s famous, too. It shows what made the first good evidence that black holes are a thing, back in 1965. That ball to the right is a blue supergiant. See how its solar wind is feeding into X-1’s accretion disk? NASA’s picture is from 2017 so it’s not really historical or anything.”


“Now this one is historical, Cal. That image was released in 2019 from data collected in 2017.”

“I knew you’d recognize it, Sy. You’ve written about it enough.”


<sly grin> “Whaddya think of this one, Sy, the gravitational waves from those two black holes that LIGO told us about?”

“You knew I wouldn’t like it.”

The final waltz of two black holes” – click for video
Credit: R. Hurt – Caltech / JPL

“It’s just another trampoline picture, right?”

“No, it’s worse than that. Gravitational waves travel at lightspeed. Massive objects like people and 30‑solar‑mass black holes can’t get up to a fraction of a percent of lightspeed without expending an enormous amount of energy. The waves travel outward much faster than objects can orbit each other, even up to the end. Those waves winding outward should be nearly straight.”


“Whoa, Cal, this one isn’t a poster, it’s a monitor screen.”

“I bought a new bigger flat‑screen for home so I brought the old small one here for videos. I like how this movie shows the complicated shape flattening out when you get above the disk. The Interstellar movie made everyone think the disk is some weird double‑handled ring but the handle’s aren’t really there.”

“Mm‑hm, very nice gravity‑lens demonstration. Notice how the ring’s bright in whichever side’s coming toward us whether we’re above or below it?”

Circling over a black hole structure” — Click for video
Credit: NASA’s Goddard Space Flight Center/Jeremy Schnittman

“No, I hadn’t. Cool. How come?”

“It’s called relativistic Doppler beaming. Time distortion is significant in the close‑in parts of the ring. That affects how we see the flow. In the hole’s frame of reference the brightness and rotation speed are the same all around. In our frame the moving‑closer particles look brighter because they emit more photons per unit of our time. Another one of those unexpected phenomena where physicists say, ‘Of course!’ as soon as they see it but not before.”

~~ Rich Olcott

The Ultimate Pinhole Camera

Neither Kareem nor I are much for starting conversations. We’re more the responder type so the poker hands we dealt went pretty quickly. Cathleen had a topic, though. “Speaking of black holes and polarized radio waves, I just read a paper claiming to have developed a 3‑dimensional movie of an event wider than Mercury’s orbit, all from the flickering of a single pixel.”

Eddie bets big, for him. Ten chips. “That’s a lot to ask from just a dot. And what’s polarization got to do with it?”

Cal folds but pipes up anyway. “What was the event?”

“You know Sagittarius A*, the supermassive black hole in the middle of our galaxy?”

“Yeah, one of those orange‑ring pictures.”

“Mm‑hm. Based on radio‑wave emissions from its accretion disk. That image came from a 2‑day Event Horizon Telescope study in 2017. Well, four days after that data was taken, the Chandra satellite observatory saw an X‑ray flare from the same region. The ALMA radio telescope team immediately checked the location. ALMA has excellent signal‑to‑noise and time‑resolution capabilities but it’s only one observatory, not world‑wide like the EHT. The EHT can resolve objects a hundred thousand times closer together than ALMA’s limit. But the team did a lot with what they had.”

Vinnie tends to bet big, maybe because he’s always skeptical. Fifteen chips. “You said ‘claiming‘ like there’s doubt. People don’t trust the data?”

“In science there’s always doubt. In this case, no‑one doubts the data — ALMA’s been providing good observations for over a decade. The doubt’s in the completely new AI‑driven data reduction technique the team used. Is what they did valid? Could their results have been affected by a ‘hallucination’ bug?”

Vinnie doesn’t let go. “What did they do, what have people been doing, and what’s hallucination?”

Susan reluctantly shoves fifteen chips into the pot. “Hallucination is an AI making up stuff. I just encountered that in a paper I’m reviewing. There’s a long paragraph that starts off okay but midway it goes off on a tangent quoting numbers that aren’t in the data. I don’t believe the submitting authors even read what they sent in.”

Kareem drops out of the betting but stays in the conversation. “For a lot of science, curve‑fitting’s a standard practice. You optimize a model’s parameters against measured data. X‑ray crystallography, for example. The atoms in a good crystal are arranged in a regular lattice, right? We send a narrow beam of X‑rays at the crystal and record the intensity reflected at hundreds of angles by the atoms in different lattice planes. Inside the computer we build a parameterized model of the crystal where the parameters are the x‑, y‑ and z‑coordinates of each atom. We have computer routines that convert a given set of configuration parameters into predicted reflection intensity at each observation angle. Curve‑fitting programs cycle through the routines, adjusting parameters until the predictions match the experimental data. The final parameter values give us the atomic structure of the crystal.”

“There’s a lot of that in astrophysics and cosmology, too. This new AI technique stands that strategy on its head. The researchers started with well‑understood physics outside of the event horizon — hot rotating accretion disk, strong magnetic field mostly perpendicular to that, spacetime distortion thanks to General Relativity — and built 50,000 in‑computer examples of what that would look like from a distance.”

“Why so many?”

“The examples had to cover one or two supposed flares of different sizes and brightness at different points in their orbits, plus noise from the accretion disk’s radiation, all from a range of viewpoint angles. Mind you, each example’s only output was a single signal intensity and polarization angle (that’s two dimensions) for that specific set of disk and flare configuration parameters. The team used the example suite to train an AI specialized for assembling 2‑dimensional visual data into a 3‑dimensional model. The AI identified significant patterns in those 50,000 simulated signals. Then the team confronted the trained AI with 100 minutes of real single‑pixel data. It generated this…”

Click through to video, from Levis, et al.

“Curve‑fitting but we don’t know the curves!”

“True, Sy, but the AI does.”

“Maybe.”

~ Rich Olcott

A Non-political Polarizing Topic

Vinnie gets the deck next, but first thing he does is plop a sheet of paper onto the table. “Topic is black holes, of course. Everybody’s seen this, right?”

“Sure, it’s the new view of the Milky Way’s super-massive black hole with the extra lines. So deal already.”

“Hold your horses, Cal.” <Vinnie starts dealing.> “I’m looking for explanations. Where’d those lines come from? They swirl across the accretion disk like so much rope, right? Why aren’t they just going straight in orderly‑like? The whole thing just don’t make sense to me.”

Susan bets a few chips. “I saw a similar pop‑sci article, Vinnie. It said the lines trace out polarization in the light waves the Event Horizon Telescope captured. Okay, radio waves — same thing just longer wavelength. Polarized radio waves. I’ve measured concentrations of sugar and amino acid solutions by how much the liquid rotates polarized light, but the light first went through a polarizing filter. How does a black hole make polarized waves?”

Kareem matches Susan’s bet. “Mm‑hm. We use polarized light passing through thin sections of the rocks we sample to characterize the minerals in them. But like Susan says, we don’t make polarized light, we use a filter to subtract out the polarization we don’t want. You’re the physicist, Sy, how does the black hole do the filtering?”

Plane‑polarized electromagnetic wave
 Electric (E) field is red
 Magnetic (B) field is blue
(Image by Loo Kang Wee and Fu-Kwun Hwang from Wikimedia Commons)

My hand’s good so I match the current ante. “It doesn’t. There’s no filtering, the light just comes out that way. I’d better start with the fundamentals.” <displaying Old Reliable> “Does this look familiar, Vinnie?”

“Yeah, Sy, you’ve used it a lot. That blue dot in the back’s an electron, call it Alice, bobbing straight up and down. That’s the polarization it’s puttin’ on the waves. The red lines are the force that another electron, call it Bob, feels at whatever distance away. Negative‑negative is repelling that so Bob goes down where the red line goes up but you get the basic idea.”

“The blue lines are important here.”

“I’m still hazy on those. They twist things, right?”

“That’s one way to put it. Hendrik Lorentz put it better when he wrote that Bob in this situation experiences one force with two components. There’s the red‑line charge‑dependent component, plus the blue‑line component that depends on the charge and Bob’s motion relative to Alice. If the two are moving in parallel—”

“The same frame, then. I knew frames would get into this somehow.”

“It’s hard to avoid frames when motion’s the subject. Anyway, if the two electrons are moving in parallel, the blue‑line component has zero effect. If the two are moving in different directions, the blue‑line component rotates Bob’s motion perpendicular to Alice’s red‑line polarization plane. How much rotation depends on the angle between the two headings — it’s a maximum when Bob’s moving perpendicular to Alice’s motion.”

“Wait, if this is about relative motion, then Bob thinks Alice is twisting, too. If she thinks he’s being rotated down, then he thinks she’s being rotated up, right? Action‑reaction?”

“Absolutely, Vinnie. Now let’s add Carl to the cast.”

“Carl?”

Alice and Bob’s electromagnetic interaction
begets motion that generates new polarized light.

“Distant observer at right angles to Alice’s polarization plane. From Carl’s point of view both electrons are just tracking vertically. Charges in motion generate lightwaves so Carl sees light polarized in that plane.”

Cathleen’s getting impatient, makes her bet with a rattle of chips. “What’s all this got to do with the lines in the EHT image?”

“The hole’s magnetic field herds charged particles into rotating circular columns. Faraday would say each column centers on a line of force. Alice and a lot of other charged particles race around some column. Bob and a lot of other particles vibrate along the column and emit polarized light which shows up as bright lines in the EHT image.”

“But why are the columns twisted?”

“Orbit speed in the accretion disk increases toward its center. I’d bet that’s what distorts the columns. Also, I’ve got four kings.”

“That takes this pot, Sy.”

~~ Rich Olcott