The 18th Annual Southwest Quantum Information and Technology (SQuInT) Workshop is an outreach and service activity of the Center for Quantum Information and Control (CQuIC), and is about to take place this February 18-20, 2016 in Albuquerque New Mexico, SQuInT2016.  With over 160 participants, 45 talks, and 60 posters, SQuInT has become one of the largest and most diverse meetings in Quantum Information Science in the United States.  Under Chief SQuInT Organizer, Prof. Akimasa Miyake, this year’s program includes reports on the ground breaking experiments in loophole-free violations Bell’s Inequalities, the latest developments in quantum dots, superconductors, and ion and neutral atom traps, and a wide range of quantum information theory.  The SQuInT 2016 Keynote will be delivered by IQIM’s very own, Prof. John Preskill.

How did SQuInT get here? Its origin stems from the history of Quantum Information Science (QIS) itself. I joined the faculty at UNM in 1995.  Those were heady times, on the heels of Shor’s  algorithm and new developments in quantum information theory, which  occurred at inflationary speeds.  Simultaneously, Bose Einstein Condensation had just been observed.  These two developments caused a revolution in quantum optics and AMO-physics from with SQuInT was founded.

I, together with my colleague and now 20-year academic partner, Prof. Poul Jessen at the College of Optical Science, University of Arizona, focused on “optical lattices,” a brand new idea at that time, and the subject of Poul’s PhD thesis.  In Poul’s dissertation, he demonstrated that the motion of laser-cooled atoms,  trapped at the antinodes of standing waves, was quantized.  This quantum motion was reminiscent of that seen in atomic ions in Paul traps, and we set out to exploit this in optical lattices.  Indeed, a hot development of the 1990s was the ability to engineer nonclassical states of motion of ions, leveraging off of the analogy with the Jaynes-Cummings model of cavity QED.  As a side note, this capability was at the heart of the 1995 proposal by  Ignacio Cirac & Peter Zoller  for ion trap quantum computing and the immediate demonstration by Chris Monroe & Dave Wineland of the first CNOT gate.  Given these connections, in 1997 I organized a small workshop at UNM entitled Quantum Control of Atomic Motion, which brought together neutral atom trappers, ion trappers, and quantum opticians. Among the participants were Rainer Blatt, Hideo Mabuchi, Hersch Rabitz, and Dave Wineland.  Hersch’s presence was a new dimension, as we began to understand that the tools of quantum optimal control, previously developed mostly in the context of NMR and in physical chemistry, would be important for quantum control of atoms.  The meeting was repeated in 1998, as Quantum Control of Atomic Motion II.  By that time quantum computing was fully taking hold in the community.  Chris Monroe presented his logic gate results and we presented the first ideas for quantum computing in optical lattices.  The attendees decided we should be broadening the scope of the meeting to Quantum Information Science and Technology.  Hideo Mabuchi corresponded with Ike Chuang, who was at IBM-Almaden in San Jose California at the time.  Ike, of course, was at the center of the QI revolution and in December 1998 assembled a meeting of some of the key players including: Carl Caves, Richard Cleve, Chris Fuchs, Paul Kwiat, Poul Jessen, Hideo Mabuchi, David Meyer, Chris Monroe, John Preskill, Lu Sham, and  Birgitta Whaley.

SQuInT Founders Meeting, IBM Almaden, San Jose CA, December 1998

And thus SQuInT was born.  The first meeting was held in 1999 (SQuInT99) in Albuquerque New Mexico at a budget hotel known as the Holiday Inn “Mountain View.”  Mostly we had a view of the nearby truck stop. But the meeting was of the highest quality.  Our first session was Chaired by Dave Wineland.  The speakers were Serge Haroche, Jeff Kimble, and Hideo Mabuchi.  I’d say we were on the right track!

First Annual SQuInT Workshop, February 1999, Albuquerque NM

At this first meeting we voted on the SQuInT Logo, created by Jon Dowling

Here’s the backstory. Alice and Bob Kokepelli, the Hopi fertility deities, play their flutes to the dreamcatcher.   What has the dreamcathcer caught?  Part of the circuit diagram for quantum teleportation of course!

At the time, SQuInT was envisioned to be a regional network.  As QIS was a new field, the plan was to facilitate collaborations and exchange of information given the local strength in the southwestern United States.  Some of the key nodes of the SQuInT Network at the time included Caltech, IBM-Almaden, Los Alamos, NIST Boulder, UA, UCB, UCSB, UCSD, and UNM.  SQuInT took as its mission two key objectives: (1) building a network where the interdisciplinary subject matter of QIS would grow through direct interactions of theoretical and experimental physicists and computer scientists, as well as chemists, engineers, and mathematicians; (2) provide training of students, postdocs, and others who were entering a newly emerging discipline.  In line with goal (2), the Annual SQuInT Workshop has been a forum friendly to young scientists, where students and postdocs give talks alongside senior leaders in the field, and where new networks and collaborations can build.  In addition, students organized “summer retreats,” which essentially served as summer schools, since there were few courses in QIS at that time.

After its initial founding, SQuInT grew and the Annual Workshop traveled amongst the node institutions.  By the fourth meeting, we had grown to over 75 participants.

After its establishment in 2007, CQuIC became the official administrative home of SQuInT.  The Annual Meeting alternates between New Mexico and one of the Node Institutions, of which there are now 30 across the United States and some international. These Nodes include universities, national laboratories, and industry, the latter of which has an increasing presence given the rapid developments in QI technologies (SQuInTNodes).   SQuInT Node institutions serve on the SQuInT Steering Committee and are the core participants in SQuInT, and can act as local hosts of the Annual Workshop.  Last year’s meeting took place in Berkeley CA with over 200 participants.

Seventeenth Annual SQuInT Meeting, February 2015, Berkeley CA

After 17 years serving as the Chief SQuInT Coordinator (plus 2 years of proto-SQuInT organization), I am proud to hand over the reigns to Prof. Akimasa Miyake.  SQuInT remains true to its goals of training, education, and growth of an interdisciplinary subject. Under Akimasa’s organization, we have a top-notch program, and I look forward to attending SQuInT, as a participant!

Yesterday was a special day. And no I’m not referring to #BlackFriday — but rather to #BlackHoleFriday. I just learned that NASA spawned this social media campaign three years ago. The timing of this year’s Black Hole Friday is particularly special because we are exactly 100 years + 2 days after Einstein published his field equations of general relativity (GR). When Einstein introduced his equations he only had an exact solution describing “flat space.” These equations are notoriously difficult to solve so their introduction sent out a call-to-arms to mathematically-minded-physicists and physically-minded-mathematicians who scrambled to find new solutions.

If I had to guess, Karl Schwarzschild probably wasn’t sleeping much exactly a century ago. Not only was he deployed to the Russian Front as a solider in the German Army, but a little more than one month after Einstein introduced his equations, Schwarzschild was the first to find another solution. His solution describes the curvature of spacetime outside of a spherically symmetric mass. It has the incredible property that if the spherical mass is compact enough then spacetime will be so strongly curved that nothing will be able to escape (at least from the perspective of GR; we believe that there are corrections to this when you add quantum mechanics to the mix.) Schwarzchild’s solution took black holes from the realm of clever thought experiments to the status of being a testable prediction about how Nature behaves.

It’s worth mentioning that between 1916-1918 Reissner and Nordstrom generalized Schwarzschild’s solution to one which also has electric charge. Kerr found a solution in 1963 which describes a spinning black hole and this was generalized by Newman et al in 1965 to a solution which includes both spin (angular momentum) and electric charge. These solutions are symmetric about their spin axis. It’s worth mentioning that we can also write sensible equations which describe small perturbations around these solutions.

And that’s pretty much all that we’ve got in terms of exact solutions which are physically relevant to the 3+1 dimensional spacetime that we live in (it takes three spatial coordinates to specify a meeting location and another +1 to specify the time.) This is the setting that’s closest to our everyday experiences and these solutions are the jumping off points for trying to understand the role that black holes play in astrophysics. As I already mentioned, studying GR using pen and paper is quite challenging. But one exciting direction in the study of astrophysical black holes comes from recent progresses in the field of numerical relativity; which discretizes the calculations and then uses supercomputers to study approximate time dynamics.

Artist’s rendition of dust+gas in an “accretion disk” orbiting a spinning black hole. Friction in the accretion disk generates temperatures oftentimes exceeding 10M degrees C (2000 times the temperature of the Sun.) This high temperature region emits x-rays and other detectable EM radiation. The image also shows a jet of plasma. The mechanism for this plasma jet is not yet well understood. Studying processes like this requires all of tools that we have available to us: from numerical relativity; to cutting edge space observatories like NuSTAR; to LIGO in the immediate future *hopefully.* Image credit: NASA/Caltech-JPL

I don’t expect many of you to be experts in the history outlined above. And I expect even fewer of you to know that Einstein’s equations still make sense in any number of dimensions. In this context, I want to briefly introduce a 2+1 dimensional solution called the BTZ black hole and outline why it has been astonishingly important since it was introduced 23 years ago by Bañados, Teteilboim and Zanelli (their paper has been cited over 2k times which is a tremendous number for theoretical physics.)

There are many different viewpoints which yield the BTZ black hole and this is one of them. This is a  time=0 slice of the BTZ black hole obtained by gluing together special curves (geodesics) related to each other by a translation symmetry. The BTZ black hole is a solution of Einstein’s equations in 2+1d which has two asymptotic regions which are causally separated from each other by an event horizon. The arrows leading to “quantum states” come into play when you use the BTZ black hole as a toy model for thinking about quantum gravity.

One of the most striking implications of Einstein’s theory of general relativity is that our universe is described by a curved geometry which we call spacetime. Einstein’s equations describe the dynamical interplay between the curvature of spacetime and the distribution of energy+matter. This may be counterintuitive, but there are many solutions even when there is no matter or energy in the spacetime. We call these vacuum solutions. Vacuum solutions can have positive, negative or zero “curvature.“

As 2d surfaces: the sphere is positively curved; a saddle has negative curvature; and a plane has zero curvature.

It came as a great surprise when BTZ showed in 1992 that there is a vacuum solution in 2+1d which has many of the same properties as the more physical 3+1d black holes mentioned above. But most excitingly — and something that I can’t imagine BTZ could have anticipated — is that their solution has become the toy model of all toy models for trying to understand “quantum gravity.”

GR in 2+1d has many convenient properties. Two beautiful things that happen in 2+1d are that:

• There are no gravitational waves. Technically, this is because the Riemann tensor is fully determined by the Ricci tensor — the number of degrees of freedom in this system is exactly equal to the number of constraints given by Einstein’s equations. This makes GR in 2+1d something called a “topological field theory” which is much easier to quantize than its full blown gauge theory cousin in 3+1d.
• The maximally symmetric vacuum solution with negative curvature, which we call Anti de-Sitter space, has a beautiful symmetry. This manifold is exactly equal to the “group manifold” SL(2,R). This enables us to translate many challenging analytical questions into simple algebraic computations. In particular, it enables us to find a huge category of solutions which we call multiboundary wormholes, with BTZ being the most famous example.

Some “multiboundary wormhole” pictures that I made. The left shows the constant time=0 slice for a few different solutions and what you are left with after gluing according to the equations on the right. These are solutions to GR in 2+1d.

These properties make 2+1d GR particularly useful as a sandbox for making progress towards a theory of quantum gravity. As examples of what this might entail:

• Classically, a particle is in one definite location. In quantum mechanics, a particle can be in a superposition of places. In quantum gravity, can spacetime be in a superposition of geometries? How does this work?
• When you go from classical physics to quantum physics, tunneling becomes a thing. Can the same thing happen with quantum gravity? Where we tunnel from one spacetime geometry to another? What controls the transition amplitudes?
• The holographic principle is an incredibly important idea in modern theoretical physics. It stems from the fact that the entropy of a black hole is proportional to the area of its event horizon — whereas the entropy of a glass of water is proportional to the volume of water inside the glass. We believe that this reduction in dimensionality is wildly significant.

A few years after the holographic principle was introduced in the early 1990’s, by Gerard ‘t Hooft and Lenny Susskind, Juan Maldacena came up with a concrete manifestation which is now called the AdS/CFT correspondence. Maldacena’s paper has been cited over 14k times making it one of the most cited theoretical physics papers of all time. However, despite having a “correspondence” it’s still very hard to translate questions back and forth between the “gravity and quantum sides” in practice. The BTZ black hole is the gravity solution where this correspondence is best understood. Its quantum dual is a state called the thermofield double, which is given by: . This describes a quantum state which lives on two circles (see my BTZ picture above.) There is entanglement between the two circles. If an experimentalist only had access to one of the circles and if they were asked to try to figure out what state they have, their best guess would be a “thermal state.” A state that has been exposed to a heat-bath for too long and has lost all of its initial quantum coherence.

It is in this sense that the BTZ black hole has been hugely important. It’s also evidence of how mysterious Einstein’s equations still remain, even to this day. We still don’t have exact solutions for many settings of interest, like for two black holes merging in 3+1d. It was only in 1992 that BTZ came up with their solution–77 years after Einstein formulated his theory! Judging by historical precedence, exactly solvable toy models are profoundly useful and BTZ has already proven to be an important signpost as we continue on our quest to understand quantum gravity. There’s already broad awareness that astrophysical black holes are fascinating objects. In this post I hope I conveyed a bit of the excitement surrounding how black holes are useful in a different setting — in aiding our understanding of quantum gravity. And all of this is in the spirit of #BlackHoleFriday, of course.

Hey all, I’m back! I’ve been stuck in a black hole for the past couple years. Nobody ever said that doing a PhD in quantum gravity would be easy. Actually, my advisor John Preskill explicitly warned me that it would be exceptionally difficult (but in an encouraging manner; he was managing my expectations.) I wish I could say that I’ve returned w/ emergent spacetime figured out, but alas, I was simply inspired to write about a heady topic that is quite personal to me: how to increase gender diversity in STEM. (Maybe the key to understanding quantum gravity is to have more women thinking about these questions?)

I’ve been thinking about this topic for well over a decade but my interest bubbled over last week and I decided to write this post. Some entrepreneur friends were on a panel at Caltech (John Hering, Diego Berdakin and Joe Lonsdale) and during a wonderful sub-convo about increasing gender diversity in STEM a male undergrad asked: “as someone who’s only a student, what can I do to help with this issue?” The panel pretty much nailed it with their responses but this is an incredibly important issue and I want to capture some of their comments in writing, to frame this with broader context and to add some personal anecdotes.

Before providing a few recommendations here are some bullets which I think are important in terms of framing this issue.

1. Full stack problem: this isn’t an issue that can be tackled by targeting any specific age range. It especially can’t be tackled by only focusing on recruitment for colleges or STEM jobs. Our current lack of diversity literally starts the day children are born. We have a broad culture of pushing kids away from STEM but these pressures disproportionately target girls.

2. Implicit biases: one of the most damaging and least spoken about mechanisms through which this happens are implicit biases. Very few people understand the depth of this issue and as an extension how guilty WE ALL ARE. Implicit biases are pervasive and they are pushing girls out of STEM. Here are examples from my own childhood which highlight how subtle the issue is.

I have a younger sister who has basically the same brain as myself (truly, we can read each others minds.) I became a theoretical physicist and entrepreneur and she’s a lawyer. This is obviously a worthy profession but how did we choose these paths? For years I’ve been looking back and trying to answer this question. Upon reflection, I was astonished by the strength of my implicit biases.

a. An Uncle helped me build a computer when I was seven. No one did the same for my sister. I spent most of the ages of 7-16 hacking around on computers which provided the foundation for many of the things that I’ve done in my adult life. This gesture by my Uncle was easily one of the most impactful things that anyone has ever done for me.

b. When my sister had computer problems I would treat her like she’s stupid and simply fix the problem for her (these words are overly dramatic but I’m trying to make a point.) Whereas when my male cousin had issues I would sit next to him and patiently explain the underlying issue and teach him how to fix his problem. That teaching a man to fish metaphor is a thing.

c. When people gave us presents they would give me Legos and my sister art supplies or clothes. Gifts didn’t always fall into these categories (obviously) but they almost always had a similar gender-specific split.

d. When I was the first to finish my multiplication tables in 3rd grade, my teacher encouraged me to read science books. When my sister finished she was encouraged to draw. This teacher was female.

e. These are only a few examples of implicit biases. I wasn’t aware of the potential cause-and-effect of my actions while making them. Only after years of reflection and seeing how amplified the problem becomes by making it to the tip of the funnel was I able to connect these personal dots. These biases are so deeply engrained that addressing them requires societal-scale reprogramming — but it starts with enhanced self-awareness. I obviously feel some level of guilt for being oblivious to these actions as a kid. And I’d be delusional to think I’m beyond having similar biases today.

3. Explicit/systematic biases: there’s much broader awareness of these category of biases so I’m mainly going to explain by linking to some recent headlines. The short of it is that on their path to STEM, women have to put up with many more hurdles than men. From hiring biases to sexual harassment. These biases disproportionately adversely affect women. Here’s a tiny sample of some of the most glaring recent headlines:

a. “Geoff Marcy was a serial harasser for at least twenty years” — Gizmodo.

b. “Why women are poor at science, by Harvard president (Larry Summers)” — Guardian headline. Granted, his comments were more nuanced than the media portrayed. But in any case, extremely damaging and evidence of an outmoded way of thinking.

c. “Could it be that researchers find a hiring bias that favors women?” — NPR. I wanted to include this example to highlight that sometimes systematic biases (this isn’t exactly an explicit bias) go the other direction. But of course if we search hard enough we will be able to find specific instances in the stack where the bias favors women. My personal interpretation of this headline is: “the fearless women that have braved decades of doubt may have a minuscule advantage when competing for STEM jobs, but only after they have been disproportionately filtered out of the applicant pool on a massive scale.” Here are some statistics which show why this headline is only scratching the surface: NGCP and Techbridge.

If we acknowledge that this is a problem that literally starts the day children are born, then what can we, as individuals, do about it?

1. Constantly run a mental loop to check your implicit biases. I’m hoping we can compile a list of examples in the comments that can serve as a check-list of things NOT TO DO! E.g. When you ask: “what do you want to be when you grow-up?” Don’t answer before kids can get back to you with something like: “be a princess?” or “be a baseball player?” Those kids might want to be mathematicians! Maryam Mirzakhani or Terry Tao!

2. Provide encouragement to young girls without being over the top or condescending. Here’s a simple example from the past week. A.K. is ~8 years old and she visited Caltech recently (yes, I got permission from her mother to use this example.) This girl is a rockstar.

The tragic reality is that A.K. is going to spend her next decade being pushed away from STEM. Don’t get me wrong, she’s lucky to have encouraging parents who are preempting this push, but they will be competing with the sway of the media and her peers.

Small gestures, such as @Caltechedu reposting the above photo on Instagram provides a powerful dosage of motivation. The way I think about it is this: kids, but especially girls, are going to face a persistent push away from STEM. They are going to get teased for being “too smart” + “not girly enough” + “weird” + “nerdy” + etc. Small votes of confidence from people that have made it through and can therefore speak with authority are like little bits of body armor. Comments sting a little bit less when the freedom+success of the other side is visible and you’re being told that you can make it too. Don’t underestimate the power of small gestures. One comment can literally make a world of difference. Do this. But it absolutely must be genuine.

3. Make a conscious effort to share your passion + enthusiasm for STEM. Our culture does an abysmal job of motivating and promoting the beauty + wonder of science. This advice applies to both girls and boys and it’s incredibly important. One of my favorite essays is “A Mathematician’s Lament” by Paul Lockhart. In it he contrasts the way that we teach mathematics compared to how we teach painting and music. Imagine if before letting kids see a finished masterwork or picking up a brush and playing around, we forced them to learn: color theory, the history of art, how to hold a brush, etc! If you’re at Caltech then invite kids to the SURF seminar day or to interesting public lectures. Go give a talk at a local school and explain via examples that science is a work in progress — there’s an infinite amount that we still don’t know! For example, a brilliant non-physicist hacker friend asked me yesterday if the Casimir effect is temperature dependent? The answer is yes, but this is still barely understood theoretically. At what temperature will a gecko’s stick stop working? Questions like this are engaging. It will only take a few hours of your time to emphasize to dozens of kids how exciting science is. Outreach is usually asymmetric.

As an aside, writing this reminded me of an outreach story from 2010. Somehow I finagled travel funds to attend the International Congress of Mathematicians (ICM) in Hyderabad, India. During our day off (one day during a two week conference), I set out early to do some sightseeing and a dude pulled up next to me on a scooter. He asked if I was there for the congress. It’s kind of a long story but after chatting for a bit I agreed to spend the day riding around on his scooter while spreading my passion for mathematics at a variety of schools in the Hyderabad area. I lectured to hundreds of kids that day. I wrote a blog post that ended up getting picked up by a few national newspapers and even made the official ICM newsletter (page six of this; FYI they condensed my post and convoluted some facts.) I’m sure that I ended up benefitting wayyyyyy more from my outreach than any of the students I spoke to. The crazy reality is that outreach is oftentimes like this.

4. There is literally nothing more rewarding than mentoring hyper talented kids and then watching them succeed. This is also incredibly asymmetric. Two hours of your time will provide direction and motivation for months. Do not discount the power of giving kids confidence and a small amount of direction.

In this post, I ignored some very important parts of the problem and also opportunities for addressing it in an attempt to focus on aspects that I think are under appreciated. Specifically how pervasive implicit biases are and how asymmetric outreach is. Increasing diversity in STEM is a societal scale problem that isn’t going to be fixed overnight. However, I believe it’s possible to make huge progress over the next two decades. We’re in the process of taking our first step, which is global-awareness of the problem. And now we need to take the next step which is broad self-awareness about the impacts of our individual actions and implicit biases. It seems to me like wildly increasing our talent pool is a useful endeavor. In the spirit of this blog, unlocking this hidden potential might even be the key to making progress with quantum gravity! And definitely towards making progress on an innumerable number of other science and engineering goals.

And, hey S, sorry for not teaching you more about computers 😦

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Now some shameless on-topic plugs to promote my friends:

One of my roommates, Jason Porath, makes Rejected Princesses. This is a great site that all young girls should be aware of. Think badass women meet Disney glorification from a feminist perspective.

Try Goldie Blox to augment your kids’ Lego collection or as an alternative. If nothing else, watch their video featuring a Rube Goldberg inspired “Princess Machine!”

IQIM is heavily involved w/ Project Scientist which is a great program for young girls with an aptitude and interest in STEM.

“BBs,” the lecturer said. I was sitting in the center of my row of seats, the two yards between me and the whiteboard empty. But I fancied I hadn’t heard correctly. “You know, like in BB guns?”

I had heard correctly. I nodded.

“Did you play with BB guns when you were a kid?”

I nodded again.

“I had BB guns,” the lecturer ruminated. “I had to defend myself from my brothers.”

I nodded more vigorously. My brother and I love each other, but we’ve crossed toy pistols.

“Photons are like BBs, like bullets.”

Light, the lecturer continued, behaves like BBs under certain conditions. Under other conditions, light behaves differently. Different behaviors correspond to different species of light. Some species, we can approximate with classical (nonquantum*) physics. Some species, we can’t.

Kids begged less for BB guns, in my experience, than for water guns. I grew up in Florida, where swimming season stretches from April till September. To reload a BB gun, you have to fetch spent BBs. But, toting a Supersoaker, you swim in ammunition.

Water guns brought to mind water waves, which resemble a species of classical light. If BBs resemble photons, I mused, what about Supersoaker sprays? Water balloons?

I resolved to draw as many parallels as I could between species of light and childhood weapons.

Under scrutiny, the Supersoaker analogy held little water (sorry). A Supersoaker releases water in a stream, rather than in a coherent wave. By coherent, I mean that the wave has a well-defined wavelength: The distance from the first crest to the second equals the distance from the second to the third, and so on. I can’t even identify crests in the Supersoaker photo below.

Coherent waves vs. Supersoaker not-really-waves

Maybe Supersoaker sprays resemble incoherent light? Incoherent light is a mixture of waves of all different wavelengths. Classical physics approximates incoherent light, examples of which include sunlight. If you tease apart sunlight into coherent components, you’ll find waves with short wavelengths (such as ultraviolet rays), waves with medium (such as light we can see), and waves with long (such as microwaves). You can’t ascribe just one wavelength to incoherent light, just as I seemed unable to ascribe a wavelength to Supersoaker sprays.

But Supersoaker sprays differ from incoherent light in other respects. I’d expect triggers, for instance, to introduce nonlinearity into the spray’s dynamics. Readers who know more than I about fluid mechanics can correct me.

Though far-reaching and forceful, Supersoakers weigh down combatants and are difficult to hide. If you need ammunition small enough for a sneak attack, I recommend water balloons. Water balloons resemble squeezed states, which form a quantum class of light related to the Uncertainty Principle.

Werner Heisenberg proposed that, the more you know about a quantum particle’s position, the less you can know about its momentum, and vice versa. Let’s represent your uncertainty about the position by Δ_x and your uncertainty about the momentum by Δ_p. The product of these uncertainties can’t dip below some number, represented by ћ/2:

.

Neither uncertainty, for example, can equal zero. Heisenberg’s proposal has evolved into more rigorous, more general forms. But the story remains familiar: The lesser the “spread in the possible values” of some property (like position), the greater the “spread in the possible values” of another property (like momentum).

Imagine plotting the possible positions along a graph’s horizontal axis and the possible momenta along the vertical. The points that could characterize our quantum system form a blob of area ћ/2. Doesn’t the blob resemble a water balloon?

Imagine squeezing a water balloon along one direction. The balloon bulges out along another. Now, imagine squeezing most of the quantum uncertainty along one direction in the diagram. You’ve depicted a squeezed state.

Depiction of a squeezed state

Not all childhood weapons contain water or BBs, and not all states of light contain photons.^** A vacuum is a state that consists of zero photons. Classical physics suggests that the vacuum is empty and lacks energy. A sliver of energy, called zero-point energy, pervades each quantum vacuum. The Uncertainty Principle offers one reason why.

The vacuum reminds me of the silent treatment. Silence sounds empty, but it can harbor malevolence as quantum vacua harbor energy. Middle-school outcasts beware zero-point malice.

Retreating up Memory Lane, I ran out of analogies between classes of light and childhood weapons. Children play with lasers (with laser pointers and laser-tag guns), and lasers emit (approximately) coherent light. But laser light’s resemblance to laser light doesn’t count as an analogy. The class of incoherent light includes thermal states. (Non-experts, I’m about to spew jargon. If you have the energy, I recommend Googling the italicized terms. If you haven’t, feel free to skip to the next paragraph.) Physicists model much of the natural world with thermal states. To whichever readers identify childhood weapons that resemble them, I offer ten points. I offer 20 for mimicry of solitons or solitary waves, and 25 for that of parametric down-conversion or photon antibunching.

But if sunshine and Supersoakers lure you away from your laptop, I can’t object. Happy summer.

With thanks to Bassam Helou for corrections and discussions.

^*Pardon my simplifying inaccuracy. Some nonquantum physics is nonclassical.

^**More precisely, not all Fock states correspond to particle numbers . Alternatively: Not all states of light correspond to positive expectation values of the particle-number operator .

by Jorge Cham.

Ok, this is where things get weird. If quantum computers, femtometer motions or laser alligators weren’t enough, let’s throw in fractionalized electrons, topological surfaces and strings that go to the end of time.

To be honest, the idea that an electron can’t be split hadn’t even occurred to me before my conversation with Gil and Jason. And yet, this goes back to the very essence of the word Quantum: there’s a minimum size to everything. For electrical charge, that minimum is the electron.

Or so we thought! According to my friend, Wikipedia, the discovery of the Fractional Quantum Hall Effect in the 1980’s showed that you can form quasi-particles (or “bubbles” as Gil and Jason explain in the video) that carry 1/3 of an electron charge under certain 2D conditions. The 1998 Nobel Prize was awarded for this discovery, although, ironically, they had to split it in three (two for the experimentalists who found it and one for the theorist that explained it).

Typically, I leave a lot out of the final video. The conversation I recorded with Jason and Gil lasted several hours and yet the final product is only five minutes long. One aspect that we talked a lot about but that I did not include in the video above (you watched it already, right?), is the idea of “More is Different”. Here is audio of Jason explaining what it is using birds as an example:

source: we-are-star-stuff.tumblr.com. Click below to hear the audio.

This is the idea of “emergent properties”: that when you combine lots of something together, you don’t just get what’s inside, you get something new. Something different. I think this is a good analogy for IQIM itself, or any such grouping of researchers under one banner. Sure, technically, each person can do great research on their own, but mix them together in one soup and more interesting things can happen that you didn’t expect.

The IQIM Family:

Well, I hope you’ve been enjoying these videos and blog entries. I was going to title this blog post, “The Mysteries Are Just Piling Up” or “Quantum Knots”, but then I looked at the pageviews for all the other blog posts I made:

I guess the title of your blog post matters. So, if this video didn’t shock you, I hope at least it 1/3 shocked you.

Watch the fourth installment of this series:

Jorge Cham is the creator of Piled Higher and Deeper (www.phdcomics.com).

CREDITS:

Featuring: Gil Refael and Jason Alicea
Recorded and animated by Jorge Cham

Funding provided by the National Science Foundation and the Betty and Gordon Moore Foundation.

Burning Man… what a controversial topic these days. The annual festival received quite a bit of media attention this year, with a particular emphasis on how the ‘tech elite’ do burning man. Now that we are no longer in the early September Black Rock City news deluge I wanted to forever out myself as a raging hippie and describe why I keep going back to the festival: for the science of course!

This is a view of my camp, the Phage, as viewed from the main street in Black Rock City. I have no idea why the CH-47 is doing a flyover… everything else is completely standard for Burning Man. Notice the 3 million Volt Tesla coil which my roommates built.

I suspect that at this point, this motivation may seem counter-intuitive or even implausible, but let me elaborate. First, we should start with a question: what is Burning Man? Answer: this question is impossible to answer. The difficulty of answering this question is why I’m writing this post. Most people oversimplify and describe the event as a ‘bunch of hippies doing drugs in the desert’ or as ‘a music festival with a dash of art’ or as ‘my favorite time of the year’ and on and on. There are nuggets of truth in all of these answers but none of them convey the diversity of the event. With upwards of 65,000 people gathered for a week, my friends and I like to describe it as a “choose your own adventure” sort of experience. I choose science.

My goal for this post is to give you a sense of the sciency activities which take place in my camp. Coupling this with the fact that science is a tiny subset of the Burning Man ethos, you should come away convinced that there’s much more to the festival than just ‘a bunch of hippies doing drugs in the desert and listening to music.’

I camp with The Phage, as in bacteriophage, the incredibly abundant virus which afflicts bacteria. There are about 200 people in our camp, most of whom are scientists, with a median age of over 30. Only about 100 people camp with the Phage in any given year. The camp also houses some hackers, entrepreneurs and artists but scientific passion is unequivocally our unifying trait. Some of the things we assembled this year include:

Dr. F and Dr. B’s 3 million Volt musical Tesla coil. Humans were inserted for scale.

Musical Tesla coil: two of my roommates built a 3 million Volt musical Tesla coil. Think about this… it’s insane. The project started while they were writing their Caltech PhD theses (EE and Applied Physics) and in my opinion, the Tesla coil’s scale is a testament to the power of procrastination! Thankfully, they both finished their PhDs. After doing so, they spent the months between their defenses and Burning Man building the coil in earnest. Not only was the coil massive–with the entire structure standing well over 20 feet tall–but it was connected through MIDI to a keyboard. Sound is just pressure waves moving through air, and lightning moves lots of air, so this was one of the loudest platforms on the playa. I manned the coil one evening and one professional musician told me it was “by far the coolest instrument he has ever played.” Take a brief break from reading this and watch this video!

Dr. Brainlove getting ready for a midnight stroll and then getting a brainlift.

Dr. Brainlove: we built a colossal climbable “art car” in the shape of a brain which was covered in LEDs and controlled from a wireless EEG device. Our previous art car (Dr. Strangelove) died at the 2013 festival, so last winter our community rallied and ‘brainstormed’ the theme for this vehicle. After settling on a neuroscience theme, one of my campmates in Berkeley scanned her brain and sent a CAD file to Arcology Now in Austin, TX who created an anatomically correct steel frame. We procured a yellow school bus which had been converted to bio diesel. We raised over $30k (there were donations beyond indiegogo.) About 20 of my campmates volunteered their weekends to work at the Nimby in Oakland: hacking apart the bus, building additional structures, covering the bus with LEDs, installing a sound system, etc. One of the finishing touches was that one of my campmates who is a neurosurgeon at UCSD procured some wireless EEG devices and then he and some friends wrote software to control Dr. Brainlove’s LEDs–thus displaying someone’s live brain activity on a 30′ long by 20′ tall climbable musical art car for the entire playa to see! We already have plans to increase the LED density and therefore put on a more impressive interactive neural light show next year.

Sugarcubes: in 2013, some campmates built an epic LED sculpture dubbed “the sugarcubes”. Just watch this video and you’ll be blown away. The cubes weren’t close to operational when they arrived so there was 48 hours of hacking madness by Dan Kaminsky, Alexander Green and many brilliant others before our “Tuesday night” party. The ethos is similar to the Caltech undergrad’s party culture–the fun is in the building–don’t tell my friends but I slept through the actual party.

Ask a scientist on the left (I’m in there somewhere and so is one of my current roommates– another Caltech PhD ’13.) Science class on the right. Science everywhere!

Ask a scientist: there’s no question that this is my favorite on playa activity. This photo doesn’t do the act justice. Imagine a rotating cast of 7-8 phagelings braving dust storms and donning lab coats all FOR SCIENCE! The diversity of questions is incredible and I always learn a tremendous amount (evidenced by losing my voice three years running.) For example, this year, a senior executive at Autodesk approached and asked me a trick question related to the Sun’s magnetic field. Fear not–I was prepared! This has happened before.. and he was wearing a “space” t-shirt so my guard was up. A nuclear physicist from UCLA asked me to explain Bell test experiments (and he didn’t even know my background.) Someone asked how swamp coolers work? To be honest, I didn’t have a clear answer off the top of my head so I called over one of my friends (who was one of the earliest pioneers of optogenetics) and he nailed it immediately. Not having a clear answer to this question was particularly embarrassing because I’ve spent most of the past year thinking about something akin to quantum thermodynamics… if you can call black hole physics and holographic entanglement that.

Make/hack sessions: I didn’t participate in any of these this year but some of my campmates teach soldering/microscopy/LED programming/etc classes straight out of our camp. See photo above.

EEG and LED hacking.

Science talks: we had 4-5 science talks in a carpeted 40ft geodesic dome every evening. This is pretty self explanatory and by this point in my post, the Phage may have enough credibility that you’d believe the caliber is exceptional.

Impromptu conversations: this is another indescribable aspect. I’ll risk undermining the beauty of these conversations by using a cheap word: the ‘networking’ at Burning Man is unrivaled. I don’t mean in the for-dollar-profit sense, I mean in the intellectual and social sense. For example, one of my campmates’ brother is a string theory postdoc at Stanford. He came by our camp one evening, we were introduced, and then we met up again in the default world when I visited Stanford the following week. Burning Man is the type of place where you’ll start talking about MPEG/EFF/optogenetics/companyX/etc and then someone will say: “you know that the inventor/spokesperson/pioneer/founder/etc is at the next table over right?”

Yup, Burning Man is just a bunch of hippies doing drugs in the desert. You shouldn’t come. You definitely wouldn’t enjoy it. No fun is had and no ideas are shared. Or in other words, Burning Man: where exceptionally capable people prepare themselves for the zombie apocalypse.

Check out my friend Peretz Partensky’s Flickr feed if you want to see more photos (and credit goes to him for the photos in this post.)

At 9:10 AM, the lab next door was blasting “Born to Be Wild.”

I was at Oxford, moonlighting as a visiting researcher during fall 2013. My hosts included quantum theorists in Townsend Laboratory, a craggy great-uncle of a building. Poke your head out of the theory office, and Experiment would flood your vision. Our neighbors included laser wielders, ion trappers, atom freezers, and yellow signs that warned, “DANGER OF DEATH.”

Down the corridor in Townsend Laboratory.

Hardly the neighborhood Mr. Rogers had in mind.

The lab that shared a wall with our office blasted music. To clear my head of calculations and of Steppenwolf, I would roam the halls. Some of the halls, that is. Other halls had hazmat warnings instead of welcome mats. I ran into “RADIATION,” “FIRE HAZARD,” “STRONG MAGNETIC FIELDS,” “HIGH VOLTAGE,” and “KEEP THIS TOILET NEAT AND TIDY.” Repelled from half a dozen doors, I would retreat to the office. Kelly Clarkson would be cooing through the wall.

“We can hear them,” a theorist observed about the experimentalists, “but they can’t hear us.”

Dangers lurked even in the bathroom.

Experiment should test, disprove, and motivate theories; and theory should galvanize and (according to some thinkers) explain experiments. But some theorists stray from experiment like North America from Pangaea.

The theoretical physics I’ve enjoyed is abstract. I rarely address platforms, particular physical systems in which theory might incarnate. Quantum-information platforms include electrons in magnetic fields, photons (particles of light), ion traps, quantum dots, and nuclei such as the ones that image internal organs in MRI machines.

Instead of addressing electrons and photons, I address mathematics and abstract physical concepts. Each of these concepts can incarnate in different forms in different platforms. Examples of such concepts include preparation procedures, evolutions, measurements, and memories. One preparation procedure defined by one piece of math can result from a constant magnetic field in one platform and from a laser in another. Abstractness has power, enabling one idea to describe diverse systems.

I’ve enjoyed wandering the hills and sampling the vistas of Theory Land. Yet the experimentalist next door cranked up the radio of reality in my mind. “We can hear them,” a theorist said. In Townsend Laboratory, I began listening. My Oxford collaborators and I interwove two theoretical frameworks that describe heat transferred and work performed on small scales. One framework, one-shot statistical mechanics, has guest-starred on this blog.

The other framework consists of fluctuation relations, which describe deviations from average behaviors by small physical systems. A quantum particle on one side of a wall has a tiny probability of tunneling through without boring any hole. Since the probability is tiny, the average particle doesn’t tunnel (during any reasonably short amount of time). When analyzing macroscopic systems—say, the roughly 10²⁴ atoms that form your left thumbnail—we assume that every particle behaves like the average particle. We can’t when analyzing minuscule systems such as one short strand of DNA. Deviations from average behaviors appear in experimental data about small systems as they do not appear in data about large systems. Fluctuation relations help us understand those deviations.

My colleagues and I addressed “information,” “systems,” and “interactions.” We deployed abstract ideas, referencing platforms only when motivating our work. Then a collaborator challenged me to listen through the wall.

Experimentalists have tested fluctuation relations. Why not check whether their data supports our theory? At my friend’s urging, I contacted experimentalists who’d shown that DNA obeys a fluctuation relation. The experimentalists had unzipped and re-zipped single DNA molecules using optical tweezers, which resemble ordinary tweezers but involve lasers. Whenever the experimentalists pulled the DNA, they measured the force they applied. They concluded that their platform obeyed an abstract fluctuation theorem. The experimentalists generously shared their data, which supported our results.

Experimentalists unzipped and rezipped DNA to test fluctuation relations. This depiction of the set-up comes from this article.

My colleagues and I didn’t propose experiments. We didn’t explain why platforms had behaved in unexpected ways. We checked calculations with recycled data. But we ventured outside Theory Land. We learned that one-shot theory models systems modeled also by fluctuation relations, which govern experiments. This link from one-shot theory to experiment, like the forbidden corridors in Townsend Laboratory, invite exploration.

In Townsend, I didn’t suffer the electric shocks or the explosions advertised on the doors (though the hot water in the bathroom nearly burned me). I turned out not to need those shocks. Blasting rock music at 9:10 AM can wake even a theorist up to reality.