Insights by Danielle Fong

a wick for ideas

Month: June, 2008

The Choice of Work

During the back and forth of exchange with a technical recruiter, he finally asked me what I was looking for. And so the floodgates opened.

This may sound weird, but I pretty much choose employment based on the promise of quality work. Other factors fade into irrelevance.

When I say quality of work, I mean more than the work environment, more than the magnitude of technical challenges, and more than the IQ of those I’d be working with. I want the opportunity to walk paths with the greatest hope of leading to first-class work. Nobel-prize winning kind of work.1 This force guides me, and so inevitably I tend upstream of technological change. Money and prestige are mere proxies for what I really want: to develop and inspire fundamental changes in the way people live. That doesn’t mean I need tackle the greatest problems humanity now faces (yet). What matters is that I, personally, have a reasonable approach. So I must always remind myself to, as Richard Hamming says, ‘plant the little acorns from which the mighty oak trees grow’ — because small projects can, swiftly and strikingly, grow momentum and value.1

I find little value in submitting myself to some company culture. I instead mean to develop my professional values, ambitions, and goals: for example, I would like to develop new methods, make them available by open sourcing them and make them popular by evangelizing them. I’d love to be given the chance to teach what I’ve learned. Excellent people bring ideas and perspective to a communities of makers. Given time, I think this will evolve naturally into a company culture worth having.

Most big companies grow faster than they could build trust, to a size greater than strong values can be supported. Natural culture is the product of alignment of creative philosophies, and in BigCo, this is too often replaced with virtual company nationalism. Fascism even. I find this is more than distasteful. I haven’t really learned how to work within it at all. I could devote my efforts to such an organization only were there deeply meaningful work to be done. And why bother?

Paul Buchheit's first Google Check.

Angling to be upstream of technological change, I bait unusual questions and find surprising answers. Give me the choice between a VP position at a big five media company with oodles of benefits, and, say, work at an early netscape or google for a totally minimal salary, and I’ll choose the latter every time. I’m pulled towards organizations where I can learn about organizing, rather than learning about institutional tradition. It’s not important for me to learn about how to run a large organization: if ever I do, I won’t follow of the paths of current captains of industry. Instead, I intend to help grow large, leaderless, open organizations, and so I’d do almost anything for a chance to work with Caterina Fake, or Linus Torvalds.

I want to work on something I find deep personal meaning in. I strongly believe in supporting open culture. I don’t think I’d work for long in games or entertainment unless it could influence some social change. I worked at MochiMedia because it made possible an income stream for small independent developers where none existed before. This finally opened up professional game development from BigCos. Now, much innovation in gaming emerges from bedroom studios. Independent game developers can now commit to their art in a way they before could not.

Similarly, I’d work at YouTube rather than Hulu, even though one’s a startup and the other isn’t, because they’re more interested in involving everyone in the process. As Clay Shirky says, they’re interested in ‘finding the mouse’.

I want to work somewhere where I can truly make a difference. Why am I working in technology at all? Archimedes once said, ‘If you give me a lever and a place to stand, I can move the world.’ Technology is my lever. I need only find place to stand. This makes me wary of startups that try to do good, but aren’t particularly focused on doing it efficiently. I wouldn’t work for most charities. There’s too little pressure on them to focus — the tempering influence of market competition is replaced by government demands for ‘accountability’, which arn’t nearly so powerful.

There are numerous ‘ecogreen’ websites out there that try to promote simple, green ways of living. These may be virtuous, however, in terms of minimizing environmental impact I think they’re somewhat irrelevant.2 Saving plastic bags won’t lift a toe on our carbon footprint unless we find ways to either cut down on air and automobile travel, or do it more efficiently. And on carbon footprints — global warming is, I think, a red herring — there are thousands of nasty effects of pollution from, say, coal-fired power plants that will hit even if global warming doesn’t occur (though I think, probably, it will). Too much of China now wears breathing masks.3

I can see myself dedicating myself to the right company, so long as our goal, philosophies, and ambitions align. Yet these are stringent requirements. So far, then, I’ve found it necessary to reserve some energy and time for my own projects. So I must be open with companies: with most, I want only consulting work, to help them with some particular project, idea or problem. And I want to be completely, totally honest with everyone about it, because so far, the high road has never let me down.

Sincerely,
Danielle

———

Notes:

[1] – From the classic talk by Richard Hamming, You and Your Research. I don’t, particularly, apologize for my ambition here. Why shouldn’t I try to do first class work? The Nobel prize winning part is purely incidental. But this is the kind of work I mean — a significant contribution, one that people can build upon.

[2] – The free, online book Sustainability – Without the Hot Air is an excellent read. It is the first thing I’d suggest to someone interested in seriously starting into environmental matters. I shouldn’t claim that small contributions to green living are completely irrelevant — each does have some small effect. Perhaps raising the issue of green living in our collective consciousness will have an effect greater at second order than I imagined. But so many of our behaviors are misplaced. Many people, for example, go out of their way to buy ‘sustainable’ products at Whole Foods, say, when in reality, longer vehicle trips do more damage than almost anything you could buy. Many things are sold in a way to make you feel good about buying them. They don’t have any real effect!

[3] – This is worded provocatively, but pollution in China is a growing catastrophe. See ‘As China Roars, Pollution Reaches Deadly Extremes’ and ‘Where Breathing is Deadly’.

———


Thanks to Alex Lang, Ma’ayan Bresler, Nick Pilon, Colin Percival, Michael Nielsen, and Joel Muzzerall for reading drafts of this, and Charles Beatty, for sparking it.

PS: Certain misconceptions have been raised. Some feel that this is one demand of an over privileged generation. I reply to this here. Additionally, I am not, in fact, abandoning my startup. But I do need money, and a visa, so I am looking into either employment or seed funding.

Cosmology in Ten Minutes

Recently, unusual features of the cosmic microwave background, a ‘snapshot’ of the early universe, have raised issues with our understanding of the Big Bang. A Caltech team has shown how we might fix our theories. They suggest that there might have been an asymmetry in the energy that once powered the big bang. If this is correct, anomalies in the CMB may be traces of structure from a time before our explosive beginnings.

True to form, when a discussion appeared on Hacker News I rushed to comment, and this article erupted from that attempt. The current scientific understanding of our cosmic origins is a mystery to the public at large, but it was only after I noticed the bewilderment of my fellow hackers that I realized how poor a job we scientists have done in conveying the motivation behind our discoveries.

This article represents an attempt to replace that sense of bewilderment with that of wonder. I want more than to explain what cosmologists believe. I want give people a deep sense of why we believe it, of how we’ve come to our current understanding, and of why we care.

Look close, and it seems the universe is lopsided.

The cosmic microwave background (CMB) is like a snapshot of the early universe. It was once all hot plasma, gas so hot that the atoms inside it were broken up. Because it was hot, it emitted light. Because it was dense, it was opaque: the light emitted couldn’t just pass through, instead it had to bounce around. But once cool enough, the universe became transparent: all the light could now travel freely. It was as if the photographic shutter of the universe was lifted.

The Cosmic Microwave Background Radiation (from WMAP). False Color/ The light from this moment became the cosmic microwave background radiation. Because the universe seemed to have cooled at almost exactly the same time everywhere, the CMB is, unlike almost everything else in astronomy1, a picture of the entire universe at almost exactly the same moment in time. It is the best picture we have of the structure of the early universe.

The universe appears to have expanded evenly since then. We know it’s expanding now. Light is like a wave. Since the speed of light is constant, an illuminated object moving towards us has its wave crests squish together, turning bluer, and an object moving away from us has the distance between crests expand, turning more red. This is called a red shift. Since he knew the colors of certain celestial objects, Edwin Hubble was able to observe that the further something is from us, the more red-shifted its light, and therefore the faster it is speeding away.

Since we know that the early universe was hot, dense and small, and we know now that it’s cooler, sparse, big, and expanding, we can reasonably deduce that, long ago, there was a Big Bang. The universe exploded.

The Crab Nebula Strikingly, the CMB is almost the same everywhere you look. There are minor fluctuations, but even they seem to have the same distribution everywhere. The CMB, our best picture of the early universe, is extraordinarily smooth. It is one of the smoothest things ever observed in nature. This might not seem like a mystery. You might imagine that anything expanding, hot and dense would look roughly the same in all directions. It needn’t. Nebulae are formed by exploding stars, and they aren’t particularly smooth. In fact, in nature, it would seem, more often than not, that explosions are messy.

In 1981, Alan Guth suggested what might be called a ‘recipe for a universe’: inflation theory. Until then, nobody had come up with any good ideas for why the universe was so smooth and even. It is as if God2 had pressed the entire universe with a cosmic clothes iron.

Guth said, suppose you started with pretty much any initial universe. Suppose you also had an extremely strong, extremely smooth field of energy. If this field started dumping energy into the rest of the universe, it would also evenly expand space itself.3 The universe would undergo a period of exponential expansion — inflation — having the effect of flattening and smoothing the rest of the universe. Inflation is God’s clothing iron.

A flat, smooth universe isn’t the only thing that inflation predicted. For example, at small physical scales, quantum mechanical fluctuations persist. During inflation these fluctuations are blown up as well, and these would seed, almost entirely, the cosmological structure of the universe. We see these fluctuations in the CMB. According to inflation, they are tiny quantum fluctuations blown up to a cosmic scale. They are, quite literally, the ancestors of our galaxies.

It wasn’t just that there were fluctuations. Inflation theory predicted a very specific distribution and type4. When people finally had the technological capability to check, that’s just what they found. The universe appeared, at a cosmic scale, astonishingly consistent with this simple theory. Yet recently our observational capacities have improved. A CMB survey called WMAP has uncovered several surprising and unexplained features, not all of which fit well with the our previous inflation theories.

If you divided the sky in half by tracing the orbit of the earth around the sun5, and compared, in each half, the size of big fluctuations, those between 3 and 5 degrees wide, you would come to the conclusion that one side has fluctuations outweighing the other by an alarmingly large amount. One side of the universe is bumpier than the other. Moreover, the difference is larger than would be accounted for by randomness, at least 99 times out of 100.6

This asymmetry looks real. It has been checked against every known experimental error and background effect astrophysicists have been able to think of. And if it is real, our previous inflation theories, with one field of energy to inflate the early universe, won’t work. They can’t account for this anomaly.

The authors Erickcek, Kamionkowski, and Carroll don’t merely point out this problem. They posit a solution. They describe another inflation model, consistent with our new observations. They suggest the universe had not one, but many fields of universe inflating energy. There’s just one problem. At least one of these fields needs to be asymmetric.

Where could such an asymmetry come from? It is possible that we’ll never know. Cosmology offers us the hope of uncovering consistent, compelling stories of our origins. Thousands of independent observations fit neatly in cosmology’s book. But while we may discover a few lost pages from our first chapters, we may never know all reasons why our book was written in the first place.7

Nevertheless, the authors make an exciting point. Wherever the asymmetry in the inflation field came from, it must have existed before inflation. It must have existed before the big bang. We had once imagined that time before our explosive beginnings would forever remain a mystery. Yet hidden in the CMB are hints of times earlier still. In this wonderful piece of work, the authors carefully consider what anomalies in the CMB could mean. And in the process, they may have discovered a way to look farther into the past than ever before.

Notes:

[1] – Since light moves at a finite speed, when we see something far away, we’re seeing light emitted in the past. What we see of something a light-year away is (at least) one year old.

[2] – I mean ‘God’ here as in a figure of speech. Feel free to substitute ‘Mother Nature’, ‘Allah’, or the ‘Flying Spaghetti Monster’ while reading.

[3] – What does it mean, exactly, for energy to expand space itself? It’s roughly analogous to blowing up a balloon. We know that the gravity of the universe, just like the elastic outside walls of a balloon, pull its contents inward. In a balloon, air pressure pushes against that inward force of the walls. During cosmic inflation, the inflationary force pushes against gravity. There’s one important difference though. We don’t actually know what the inflationary force is. Air blows up our balloons, but we have few clues as to what blew up the universe.

[4] – The quantum fluctuations predicted by inflation follow a nearly-scale-invariant random Gaussian distribution. These fluctuations show up in the CMB, and for the most part follow these predictions pretty closely.

[5] – The line dividing the two halves of the sky here is called the ecliptic.

[6] – Formally, this statement is true at at least the 99% confidence level.

[7] – There are some questions forever beyond our grasp. Even if we knew from where the Big Bang had come, we could always probe further, and ask where that came from.

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