# Discourse in Delft

A camel strolled past, yards from our window in the Applied-Sciences Building.

I hadn’t expected to see camels at TU Delft, aka the Delft University of Technology, in Holland. I breathed, “Oh!” and turned to watch until the camel followed its turbaned leader out of sight. Nelly Ng, the PhD student with whom I was talking, followed my gaze and laughed.

Nelly works in Stephanie Wehner’s research group. Stephanie—a quantum cryptographer, information theorist, thermodynamicist, and former Caltech postdoc—was kind enough to host me for half August. I arrived at the same time as TU Delft’s first-year undergrads. My visit coincided with their orientation. The orientation involved coffee hours, team-building exercises, and clogging the cafeteria whenever the Wehner group wanted lunch.

And, as far as I could tell, a camel.

Not even a camel could unseat Nelly’s and my conversation. Nelly, postdoc Mischa Woods, and Stephanie are the Wehner-group members who study quantum and small-scale thermodynamics. I study quantum and small-scale thermodynamics, as Quantum Frontiers stalwarts might have tired of hearing. The four of us exchanged perspectives on our field.

Mischa knew more than Nelly and I about clocks; Nelly knew more about catalysis; and I knew more about fluctuation relations. We’d read different papers. We’d proved different theorems. We explained the same phenomena differently. Nelly and I—with Mischa and Stephanie, when they could join us—questioned and answered each other almost perpetually, those two weeks.

We talked in our offices, over lunch, in the group discussion room, and over tea at TU Delft’s Quantum Café. We emailed. We talked while walking. We talked while waiting for Stephanie to arrive so that she could talk with us.

The site of many a tête-à-tête.

The copiousness of the conversation drained me. I’m an introvert, formerly “the quiet kid” in elementary school. Early some mornings in Delft, I barricaded myself in the visitors’ office. Late some nights, I retreated to my hotel room or to a canal bank. I’d exhausted my supply of communication; I had no more words for anyone. Which troubled me, because I had to finish a paper. But I regret not one discussion, for three reasons.

First, we relished our chats. We laughed together, poked fun at ourselves, commiserated about calculations, and confided about what we didn’t understand.

We helped each other understand, second. As I listened to Mischa or as I revised notes about a meeting, a camel would stroll past a window in my understanding. I’d see what I hadn’t seen before. Mischa might be explaining which quantum states represent high-quality clocks. Nelly might be explaining how a quantum state ξ can enable a state ρ to transform into a state σ. I’d breathe, “Oh!” and watch the mental camel follow my interlocutor through my comprehension.

Nelly’s, Mischa’s, and Stephanie’s names appear in the acknowledgements of the paper I’d worried about finishing. The paper benefited from their explanations and feedback.

Third, I left Delft with more friends than I’d had upon arriving. Nelly, Mischa, and I grew to know each other, to trust each other, to enjoy each other’s company. At the end of my first week, Nelly invited Mischa and me to her apartment for dinner. She provided pasta; I brought apples; and Mischa brought a sweet granola-and-seed mixture. We tasted and enjoyed more than we would have separately.

Dinner with Nelly and Mischa.

I’ve written about how Facebook has enhanced my understanding of, and participation in, science. Research involves communication. Communication can challenge us, especially many of us drawn to science. Let’s shoulder past the barrier. Interlocutors point out camels—and hot-air balloons, and lemmas and theorems, and other sources of information and delight—that I wouldn’t spot alone.

With gratitude to Stephanie, Nelly, Mischa, the rest of the Wehner group (with whom I enjoyed talking), QuTech and TU Delft.

During my visit, Stephanie and Delft colleagues unveiled the “first loophole-free Bell test.” Their paper sent shockwaves (AKA camels) throughout the quantum community. Scott Aaronson explains the experiment here.

# BTZ black holes for #BlackHoleFriday

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: $|\Psi_{CFT}\rangle = \frac{1}{\sqrt{Z}} \sum_{n=1}^{\infty} e^{-\beta E_n/2} |n\rangle_1 \otimes |n \rangle_2$. 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.

# How to get more girls into STEM

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.

# Wouldn’t you like to know what’s going on in my mind?

I suppose most theoretical physicists who (like me) are comfortably past the age of 60 worry about their susceptibility to “crazy-old-guy syndrome.” (Sorry for the sexism, but all the victims of this malady I know are guys.) It can be sad when a formerly great scientist falls far out of the mainstream and seems to be spouting nonsense.

Matthew Fisher is only 55, but reluctance to be seen as a crazy old guy might partially explain why he has kept pretty quiet about his passionate pursuit of neuroscience over the past three years. That changed two months ago when he posted a paper on the arXiv about Quantum Cognition.

Neuroscience has a very seductive pull, because it is at once very accessible and very inaccessible. While a theoretical physicist might think and write about a brane even without having or seeing a brane, everybody’s got a brain (some scarecrows excepted). On the other hand, while it’s not too hard to write down and study the equations that describe a brane, it is not at all easy to write down the equations for a brain, let alone solve them. The brain is fascinating because we know so little about it. And … how can anyone with a healthy appreciation for Gödel’s Theorem not be intrigued by the very idea of a brain that thinks about itself?

(Almost) everybody’s got a brain.

The idea that quantum effects could have an important role in brain function is not new, but is routinely dismissed as wildly implausible. Matthew Fisher begs to differ. And those who read his paper (as I hope many will) are bound to conclude: This old guy’s not so crazy. He may be onto something. At least he’s raising some very interesting questions.

My appreciation for Matthew and his paper was heightened further this Wednesday, when Matthew stopped by Caltech for a lunch-time seminar and one of my interminable dinner-time group meetings. I don’t know whether my brain is performing quantum information processing (and neither does Matthew), but just the thought that it might be is lighting me up like a zebrafish.

Following Matthew, let’s take a deep breath and ask ourselves: What would need to be true for quantum information processing to be important in the brain? Presumably we would need ways to (1) store quantum information for a long time, (2) transport quantum information, (3) create entanglement, and (4) have entanglement influence the firing of neurons. After a three-year quest, Matthew has interesting things to say about all of these issues. For details, you should read the paper.

Matthew argues that the only plausible repositories for quantum information in the brain are the Phosphorus-31 nuclear spins in phosphate ions. Because these nuclei are spin-1/2, they have no electric quadrupole moments and hence corresponding long coherence times — of order a second. That may not be long enough, but phosphate ions can be bound with calcium ions into objects called Posner clusters, each containing six P-31 nuclei. The phosphorus nuclei in Posner clusters might have coherence times greatly enhanced by motional narrowing, perhaps as long as weeks or even longer.

Where energy is being consumed in a cell, ATP sometimes releases diphosphate ions (what biochemists call pyrophosphate), which are later broken into two separate phosphate ions, each with a single P-31 qubit. Matthew argues that the breakup of the diphosphate, catalyzed by a suitable enzyme, will occur at an enhanced rate when these two P-31 qubits are in a spin singlet rather than a spin triplet. The reason is that the enzyme has to grab ahold of the diphosphate molecule and stop its rotation in order to break it apart, which is much easier when the molecule has even rather than odd orbital angular momentum; therefore due to Fermi statistics the spin state of the P-31 nuclei must be antisymmetric. Thus wherever ATP is consumed there is a plentiful source of entangled qubit pairs.

If the phosphate molecules remain unbound, this entanglement will decay in about a second, but it is a different story if the phosphate ions group together quickly enough into Posner clusters, allowing the entanglement to survive for a much longer time. If the two members of an entangled qubit pair are snatched up by different Posner clusters, the clusters may then be transported into different cells, distributing the entanglement over relatively long distances.

(a) Two entangled Posner clusters. Each dot is a P-31 nuclear spin, and each dashed line represents a singlet pair. (b) Many entangled Posner clusters. [From Fisher 2015]

What causes a neuron to fire is a complicated story that I won’t attempt to wade into. Suffice it to say that part of the story may involve the chemical binding of a pair of Posner clusters which then melt if the environment is sufficiently acidic, releasing calcium ions and phosphate ions which enhance the firing. The melting rate depends on the spin state of the six P-31 nuclei within the cluster, so that entanglement between clusters in different cells may induce nonlocal correlations among different neurons, which could be quite complex if entanglement is widely distributed.

This scenario raises more questions than it answers, but these are definitely scientific questions inviting further investigation and experimental exploration. One thing that is far from clear at this stage is whether such quantum correlations among neurons (if they exist at all) would be easy to simulate with a classical computer. Even if that turns out to be so, these potential quantum effects involving many neurons could be fabulously interesting. IQIM’s mission is to reach for transformative quantum science, particularly approaches that take advantage of synergies between different fields of study. This topic certainly qualifies.* It’s going to be great fun to see where it leads.

If you are a young and ambitious scientist, you may be contemplating the dilemma: Should I pursue quantum physics or neuroscience? Maybe, just maybe, the right answer is: Both.

*Matthew is the only member of the IQIM faculty who is not a Caltech professor, though he once was.

# Surprise Happens in Experiments

The discovery of high temperature superconductivity in copper-oxide-based ceramics (cuprates) in 1986 created tremendous excitement in the scientific community. For the first time superconductivity, the ability of a material to conduct electricity with zero energy loss to heat, was possible at temperatures an order of magnitude higher than what were previously thought possible. Thus began the dream of room temperature superconductivity, a dream that has been heavily sought but still unfulfilled to this day.

The difficulty in creating a room temperature superconductor is that we still do not even understand how cuprate high temperature superconductors exactly work. We have known that the superconductivity is born from removing or adding a proper amount of electrons to an insulating antiferromagnet. What is more is that the material experiences a mysterious region, usually called pseudogap, when transiting from the insulating antiferromagnet into the superconductor. For decades, scientists have debated whether the pseudogap in cuprates is a continuous evolution into superconductivity or a competing phase of matter with distinct symmetry properties, and some believe that a better understanding of its nature and relationship to superconductivity can help to pave a path towards room temperature superconductivity.

The compound that we are studying, strontium-iridium-oxide (Sr2IrO4), is a promising candidate for a new family of high temperature superconductors. Recent experimental findings in Sr2IrO4 reveal great similarities between Sr2IrO4 and cuprates. Sr2IrO4 is a novel insulator at room temperature and turns into an antiferromagnet below a critical temperature called Néel temperature (TN). With a certain amount of electrons added or removed by introducing foreign atoms in it, Sr2IrO4 enters into the pseudogap regime. At an even higher charge carrier concentration and a lower temperature, Sr2IrO4 exhibits strong signatures of unconventional superconductivity. A summary of the evolution of Sr2IrO4 as functions of charge carrier density and temperature, usually referred as a phase diagram, is depicted into a cartoon below, which mimics that of cuprates.

A cartoon showing similarities between Sr2IrO4 and cuprates.

Our experimental results on the multipolar order in Sr2IrO4 further bridges the connection between Sr2IrO4 and cuprates. On one hand, there have been growing experimental evidences in recent years to support the presence of symmetry breaking phases of matter in the pseudogap regime of cuprates. On the other hand, the discovery of multipolar order in Sr2IrO4 where the psuedogap phenomenon has also been observed suggests a possible connection between these two. To establish the relationship between the multipolar order and the pseudogap in Sr2IrO4, one needs to compare the temperature scales at which each of them happens. So far, we have bounded a line in the Sr2IrO4 phase diagram for the multipolar ordered phase that breaks the 90o rotational symmetry from its high temperature state. However, the onset temperature for the pseudogap in Sr2IrO4 remains unknown in the community.

An artistic rendition of rotational anisotropy patterns both above and below the transition temperature T_Ω where the multipolar order happens, showing the 90^o rotational symmetry breaking across T_Ω.

Retrospectively, the scientific story was told as above in which it seems our experiment perfectly fits in a void in the connections between Sr2IrO4 and cuprates. In reality, this experiment is my first encounter of serendipity in scientific researches. When we started our experiment, there were no experimental indications about pseudogap or superconductivity in Sr2IrO4, and we were just planning to refine its antiferromagnetic structure based upon its recently refined crystallographic structure. This joyful surprise makes me aware of the importance of sensitivity to unexpected results, especially in a developing field. Another surprise to me is the technique that we used in this study, namely rotational anisotropy optical second harmonic generation. This technique is as simple as shining light of frequency ω at the sample from a series of angles and collecting light of frequency 2ω reflected from the sample. The novelty of our setup is to move the light around the sample as opposed to the other way in the traditional version of this technique. Exactly thank to this seemingly trivial novelty, we are able to probe the multipolar order that is still challenging for other more sophisticated symmetry sensitive techniques. To me, it is this experience that is more valuable, and that is what I feel happiest to share.

Although the dream of room temperature superconductivity is still unfulfilled, the cross comparisons between Sr2IrO4 and cuprates could be insightful in determining the important factors for superconductivity, and eventually make the journey towards the dream.

Please find more details in our paper and Caltech media.

Artist’s rendition of spatially segregated domains of multipolar order in the Sr2IrO4 crystal.

# Explaining Quantum Physics to Newton… in 140 characters

Sir Isaac Newton is considered by many as the greatest physicist of all time. But despite Newton’s contributions to classical physics, the man never even fathomed that the world was actually governed by the equations of quantum mechanics. We think it is time to right that wrong. With your help, we plan to send a Tweet back in time (something about time machines restricts quantum telegraphs to 140 characters) that explains what quantum is all about to Sir Isaac. This mini competition is taking place on our Twitter account over @IQIM_Caltech and ends on November 5th, 2015. The prize is a one-year digital subscription to Scientific American.

For more details, please see below. This mini competition is part of Quantum Shorts, a flash fiction competition conceived and executed by our friends at the Center for Quantum Technologies.

Let the games begin!

# Nothing has been done yet. The world is your oyster…still.

The three things that come to mind when I watch Simon’s video are: travel, perspective and discomfort. They remind me of some of the things I also said in my TEDx talk titled “Get Uncomfortable Now”.

Simon’s video exemplifies a lot of what I feel is true in filmmaking as well. He goes running to clear his mind and get more creative, I take long walks when I’m stuck at a point in my screenplays or edits. He travels to learn more about what’s out there, I travel to absorb culture as well, he tries diversity of experiences to enrich his mind, so do I in a selfish desire to enrich every character I write or direct; all with the ultimate goal of growth & transience: emotional, physical, mental.

Simon also says something very exciting in the film, “there’s so much left to do out there”, a thought that isn’t expressed that often, the idea that “I can do something novel right here in the lab” makes the chance of innovation, success and achievement very tangible; achievable. That honesty, excitement and drive is important to be repeated in an otherwise very jaded and intimidated world. The belief in the power of the individual driving forward and having the potential to change the status quo, in the lab and outside, is critical.

It was hard to get Simon to narrow it down to the one hobby that drove him. After Debaleena’s video being internal and about family, we knew we wanted something more external. Filming in Griffith park is usually a nightmare but that early morning, we got everything we wanted minus possibly a clearer view of downtown LA, thanks to Marcia Brown’s usual detailed planning.

The shoot was complete with a steadicam operator, running videos and even the spotting of a snake!

The most memorable thing for me are Simon’s slow motion shots that highlight the sound of foot steps, of pushing forward, step by step, one ahead of the other; that basic contact that lunges us into the future. There was something very “grounding” about watching that, no pun intended.

Without further ado, here’s the video: