What if you could only see the world in UV?

July 21st, 2018

UV cameras expose a hidden world and reveal the incompleteness of our perception
The Physics Girl looks at sunscreen: https://youtu.be/GRD-xvlhGMc
How to make sunscreen from scratch: https://youtu.be/lMXAY5F28L0

In summary, ultraviolet light interacts differently with matter for a number of reasons:
1. Some pigments selectively absorb UV so they may appear white in the visible but dark in the UV. The pigments usually dissipate the UV energy as heat, though the breaking of bonds can also occur.
2. Fluorescent molecules absorb UV light and re-radiate that energy as visible light. This makes them look dark in the UV but glowing under black light.
3. Ultraviolet light scatters more than visible light because the wavelength is shorter and Raleigh scattering is proportional to the reciprocal of wavelength to the power of four.

Special thanks to HHMI BioInteractive for their awesome animations of melanocytes and how the melanin in melanosomes protect your DNA. To see the full video explaining how we get our skin color, check out: https://www.youtube.com/watch?v=VC0TL_lYLm8

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References:

Overview of main UV effects:
Visualizing Rayleigh Scattering through UV Photography
https://journals.ametsoc.org/doi/pdf/10.1175/BAMS-D-14-00260.1

Arctic animals are photographed in the UV to increase visibility and get an accurate count:
Lavigne, D. (1976). Counting Harp Seals with ultra-violet photography. Polar Record, 18(114), 269-277. doi:10.1017/S0032247400000310

Absorption spectrum of melanin: http://www.cl.cam.ac.uk/~jgd1000/melanin.html

“The spectroscopy of human melanin pigmentation,” by N. Kollias. In: Melanin: Its Role in Human Photoprotection, pp. 31 – 38. Valdenmar Publishing Co. (1995).

“Optical properties of human sclera, and their consequences for transscleral laser applications,” by A. Vogel, C. Dlugos, and R. Nuffer, Lasers in Surgery and Medicine 11(4), pp. 331 – 340 (1991).

“The incidence and time-course of latanoprost-induced iridial pigmentation as a function of eye color,” by P. Wistrand, J. Stjernschantz, and K. Olsson, Survey of Ophthalmology 41(S2), pp. S129 – S138 (1997).

Music by Epidemic Sound: https://www.epidemicsound.com “Spring Moods 5”


The Misunderstood Nature of Entropy

July 18th, 2018

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Entropy and the second law of thermodynamics has been credited with defining the arrow of time.

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Entropy is surely one of the most intriguing and misunderstood concepts in all of physics. The entropy of the universe must always increase – so says the second law of thermodynamics. It’s a law that seems emergent from deeper laws – it’s statistical in nature – and yet may ultimately be more fundamental and unavoidable than any other law of physics.

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Quantum Invariance & The Origin of The Standard Model

July 11th, 2018

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In simple terms a gauge theory is one that has mathematical parameters, or “degrees of freedom” that can be changed without affecting the predictions of the theory.

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Will A New Neutrino Change The Standard Model?
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As far as we can tell, mathematics is the language in which the universe is written. Our laws of physics are equations of motion, along with some associated constants. Previously we’ve talked a bit about the symmetries of these equations, and how they lead us to conserved quantities. But this is just the tip of the theoretical iceberg – sometimes investigating the symmetries of these equations predicts entirely new physics. The most remarkable example of this is the standard model of particle physics. You know, the most accurate physical theory in all of human history.

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Will A New Neutrino Change The Standard Model?

July 4th, 2018

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Since the discovery of the Higgs boson, physicists have searched and searched for any hint of new particles. That search has been fruitless. Until, perhaps, now. Today on Space Time Journal Club we’ll look at a paper that reports a compelling hint of a new particle outside the standard model: the sterile neutrino.

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Previous Episode:
How Asteroid Mining Will Save Earth
https://www.youtube.com/watch?v=TF6GRPaeLbk

Regular neutrinos are a bit aloof. They don’t interact by the electromagnetic or strong nuclear forces – only by the weak nuclear force and gravity. They are so weakly interacting that they pass through matter like it isn’t there. To have a 50-50 chance of stopping any given neutrino you’d need a wall of lead 
 one light year thick! If regular neutrinos are aloof, then sterile neutrinos are the complete loners. They don’t even interact via the weak interaction. Even so, detection of sterile neutrinos would be incredibly important. Besides being the first expansion of the standard model family since the Higgs boson, sterile neutrinos are a candidate for dark matter, and their existence would have had a huge influence on the expansion of the early universe.

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How Asteroid Mining Will Save Earth

June 27th, 2018

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The days of oil may be numbered, but there’s another natural resource that’s never been touched, Asteroids.

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Previous Episode:
The Black Hole Information Paradox
https://www.youtube.com/watch?v=9XkHBmE-N34

The richest person in modern history, was John Davison Rockefeller, His net worth was three times greater than that of our richest tech billionaires, inflation adjusted. And the source of that fortune? Timely exploitation of a vast, then-untapped natural resource: oil. Well, the days of oil may be numbered, but there’s another natural resource that’s never been touched, is effectively inexhaustible, and has a dollar value large enough to disrupt entire economies. That resource? Asteroids, and the precious materials they contain. Astrophysicist Neil deGrasse Tyson predicts that the world’s first trillionaire will be an asteroid miner. The Rockefellers of the 21st century may be less like the internet and tech moguls of the 20th century and more like the old-school oil barons of the 19th century.

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The Black Hole Information Paradox

June 20th, 2018

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We’ve established by now that black holes are weird. The result of absolute gravitational collapse of a massive body: a point of hypothetical infinite density surrounded by an event horizon. At that horizon time is frozen and the fabric of space itself cascades inwards at the speed of light. Nothing can travel faster than light, and so nothing can escape from below the event horizon- not matter, not light, not even information.

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Previous Episode:
Why Quantum Information is Never Destroyed
https://youtu.be/HF-9Dy6iB_4

These ideas are pretty mind-blowing, but as crazy as black holes are, they’re also kind of 
 simple. Don’t get me wrong; the math is complicated. But the objects themselves are simple. In fact every black hole in the universe, no matter how it formed or what happened to it afterwards, can be perfectly described with only three properties. Those properties are mass, angular momentum, and electric charge. Or at least this is the proposition behind the famous no-hair conjecture, or no-hair theorem.

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ColeslawPurdie

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Matthew O’Connor
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John Hofmann

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My Life Story

June 18th, 2018

The truth, with photons.
I hope I’ve articulated everything clearly in this video. If not, I’ll clarify in comments. Thanks to everyone who appears in this video and thanks to everyone who watches this video!

Veritasium is of course a combination of the latin ‘veritas’ meaning truth, and the common element ending ‘ium’. I guess this is my version of the ‘draw my life’ craze that rolled through YouTube many years ago. Except I wanted to tell my story with the actual moments, the photons, the stored magnetic states. There’s something about that which is so important to me (because I think the alternative involves fooling yourself) which is why I’m so fascinated by film and video.

One of my inspirations for the name Veritasium came from the end of the poem Ode on a Grecian Urn by John Keats, in which he writes:
“Beauty is truth, truth beauty,—that is all
Ye know on earth, and all ye need to know.”

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Magnified X1 – Gunnar Johnsen
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Sneaky Snitch


What Survives Inside A Black Hole?

June 13th, 2018

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We’ve established by now that black holes are weird. The result of absolute gravitational collapse of a massive body: a point of hypothetical infinite density surrounded by an event horizon. At that horizon time is frozen and the fabric of space itself cascades inwards at the speed of light. Nothing can travel faster than light, and so nothing can escape from below the event horizon- not matter, not light, not even information.

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Previous Episode:
Why Quantum Information is Never Destroyed
https://youtu.be/HF-9Dy6iB_4

These ideas are pretty mind-blowing, but as crazy as black holes are, they’re also kind of 
 simple. Don’t get me wrong; the math is complicated. But the objects themselves are simple. In fact every black hole in the universe, no matter how it formed or what happened to it afterwards, can be perfectly described with only three properties. Those properties are mass, angular momentum, and electric charge. Or at least this is the proposition behind the famous no-hair conjecture, or no-hair theorem.

Written and hosted by Matt O’Dowd
Graphics by Grayson Blackmon
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Made by Kornhaber Brown (www.kornhaberbrown.com)

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ColeslawPurdie

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Why Quantum Information is Never Destroyed

May 23rd, 2018

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If you have perfect knowledge of every single particle in the universe, can you use the laws of physics to rewind all the way back to the Big Bang? Is the entire history of the universe perfectly knowable? Or has information somehow lost along the way?

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Previous Episode:
Noether’s Theorem and The Symmetries of Reality
https://www.youtube.com/watch?v=04ERSb06dOg&t=2s

The laws of physics are equations of motion. They are mathematical rules that dictate how systems evolve in time. Newton’s equations for classical mechanics, Maxwell’s equations for electromagnetism, and the Schrodinger equation for quantum mechanics. These laws can be used to predict how the universe will evolve into the future. They are deterministic; perfect knowledge of a system in the present perfectly predicts how the system will change in the next instant, and the instant after that, ad infinitum. But determinism in the forward-time direction does NOT guarantee that the same laws can perfectly predict the past. And yet this sort of deterministic symmetry – time-reversal symmetry – is essential for information itself to be conserved. Today we learn why conservation of information is such a fundamental requirement of quantum mechanics. In a future episode we’ll see how this law might be broken by black holes.

Here’s that fun proof that independent quantum states can’t evolve into the same quantum state while preserving unitarity! Apologies for the unavoidable technical notation, but a quick college course in introductory quantum mechanics will get you up to speed in no time 😛

http://bit.ly/2Lpm6sL

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Noether’s Theorem and The Symmetries of Reality

May 16th, 2018

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Conservation laws are among the most important tools in physics. They feel as fundamental as you can get. And yet they’re wrong – or at least they’re only right sometimes. These laws are consequences of a much deeper, more fundamental principle: Noether’s theorem.

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Previous Episode:
How Gaia Changed Astronomy Forever
https://www.youtube.com/watch?v=Jdy09…

Conservation laws are the cheat codes of physics. They make it possible to solve physics problems that would otherwise be painfully difficult, or even impossible. More than cheat codes – conservation laws are close to the source code – they emerge from profound and simple truths about the basis of reality. They emerge from the fundamental symmetries of nature. The connection between conservation laws and symmetry is encapsulated in Noether’s theorem. But before we dive into this extremely elegant idea, let’s talk about the seeming paradox that inspired it, and the genius who discovered it.

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Sultan Alkhulaifi
Alex Seto
Michal-Peanut Karmi
Erik Stein
Kevin Warne
JJ Bagnell
Avi Goldfinger
John Pettit
Florian Stinglmayr
Benoit Pagé-Guitard
Nathan Leniz
Brandon Labonte
David Crane
Greg Weiss
Shannan Catalano
Brandon Cook