Field of Science

Who's the greatest physicist in American history?

A photo of an impish Richard Feynman playing the bongos appears in Ray Monk's sweeping biography of Robert Oppenheimer. It is accompanied by the caption "Richard Feynman, Julian Schwinger's main rival for the title of greatest American physicist in history". That got me thinking; who is the greatest American physicist in history? What would your choice be?

The question is interesting because it's not as simple as asking who's the "greatest physicist in history". The answer to that question tends to usually settle on Isaac Newton or Albert Einstein; in fact few American physicists if any would show up on the top ten list of greatest physicists ever. But limit the question to American physicists and the matter becomes more complicated. Contrast this to asking who's the greatest American chemist in history; there the answer - Linus Pauling - appears much more unambiguous and widely agreed upon.

Any discussion of "greatest scientist" is always harder than it sounds. By what measure do you judge greatness?: A single, monumental discovery? Contributions to diverse fields? Theory or experiment? Creation of an influential school of physics? Or by looking at lifetime achievement which, rather than focusing on one fundamental discovery, involves many important ones? There are contenders for "greatest American physicist" who encompass all these metrics of achievement.

Here's what's concerning: Even a generous, expansive list of contenders for "greatest American physicist" in history is embarrassingly thin compared to a comparable list of European physicists. For instance, let's consider the last three hundred years or so and think up a selection which includes both Nobel Laureates and non-Nobel Laureates. The condition is to only include American-born physicists.

Here's my personal list for the title of greatest American physicist in history, in no particular order: Joseph Henry, Josiah Willard Gibbs, Albert Michelson, Robert Millikan, Robert Oppenheimer, Richard Feynman, Murray Gell-Mann, Julian Schwinger, Ernest Lawrence, Edward Witten, John Bardeen, John Slater, John Wheeler and Steven Weinberg. I am sure I am leaving someone out but I suspect other lists would be similar in length. It's pretty obvious that this list pales in comparison with an equivalent list of European physicists which would include names like Einstein, Dirac, Rutherford, Bohr, Pauli and Heisenberg; and this is just if we include twentieth-century physicists. Not only are the European physicists greater in number but their ideas are also more foundational; as brilliant as the American physicists are, almost none of them made a contribution comparable in importance to the exclusion principle or general relativity.

Note that I said "almost none". If you ask who's my personal favorite for "greatest American physicist in history", it would not be Feynman or Schwinger or Witten; instead it would be Josiah Willard Gibbs, a man who seems destined to remain one of the most underappreciated scientists of all time but who Einstein called "the greatest mind in American history". Feynman and Schwinger may have invented quantum electrodynamics, but Gibbs invented the foundations of thermodynamics and statistical mechanics, a truly seminal contribution that was key to the development of both physics and chemistry. 

It's hard to overestimate the importance of concepts like free energy, chemical potential, enthalpy and the phase rule for physics, chemistry, biology, engineering and everything in between. In fact, so influential was Gibbs's work that it inspired that of Paul Samuelson - who unlike physicists, is actually agreed upon as the greatest American economist in history. If you really want to discuss lists of great American physicists (or scientists in general), you simply cannot exclude Gibbs. In my dictionary Gibbs's contributions are comparable to that of any famous relativist or atomic physicist. Unfortunately Gibbs also remains one of the most little known scientists in America, largely because of his introverted nature and tendency to publish groundbreaking papers in journals like the Proceedings of the Connecticut Academy of Sciences.

More importantly though, the sparse list of great homegrown American physicists makes two things clear. Firstly, that America is truly a land of immigrants; it's only by including foreign-born physicists like Fermi, Bethe, Einstein, Chandrasekhar, Wigner, Yang and Ulam can the list of American physicists start to compete with the European list. Secondly and even more importantly, the selection demonstrates that even in 2018, physics in America is a very young science compared to European physics. Consider that even into the 1920s or so, the Physical Review which is now regarded as the top physics journal in the world was considered a backwater publication, if not a joke in Europe (Rhodes, 1987). Until the 1930s American physicists had to go to Cambridge, Gottingen and Copenhagen to study at the frontiers of physics. It was only in the 30s that, partly due to heavy investment in science by both private foundations and the government and partly due to the immigration of European physicists from totalitarian countries, American physics started on the road to the preeminence that it enjoys today. Thus as far as cutting-edge physics goes, America is not even a hundred years old. The Europeans had a head start of three hundred years; no wonder their physicists feature in top ten lists. And considering the very short time that this country has enjoyed at the forefront of science, we have to admit that America has done pretty well.

The embarrassingly thin list of famous American physicists is good news. It means that the greatest American physicist is yet to be born. Now that's an event we can all look forward to.

Why the world needs more Leo Szilards

The body of men and women who built the atomic bomb was vast, diverse, talented and multitudinous. Every conceivable kind of professional - from theoretical physics to plumber - worked on the Manhattan Project for three years over an enterprise that spread across the country and equaled the US automobile industry in its marshaling of resources like metals and electricity.

The project may have been the product of this sprawling hive mind, but one man saw both the essence and the implications of the bomb, in both science and politics, long before anyone else. Stepping off the curb at a traffic light across from the British Museum in London in 1933, Leo Szilard saw the true nature and the consequences of the chain reaction six years before reality breathed heft and energy into its abstract soul. In one sense though, this remarkable propensity for seeing into the future was business as usual for the Hungarian scientist. Born into a Europe that was rapidly crumbling in the face of onslaughts of fascism even as it was being elevated by revolutionary discoveries in science, Szilard grasped early in his youth both a world split apart by totalitarian regimes and the necessity of international cooperation engendered by the rapidly developing abilities of humankind to destroy itself with science. During his later years Szilard once told an audience, "Physics and politics were my two great interests". Throughout his life he would try to forge the essential partnership between the two which he thought was necessary to save the human species from annihilation.

A few years ago Bill Lanouette brought out a new, revised edition of his authoritative, sensitive and outstanding biography of Szilard. It is essential reading for those who want to understand the nature of science, both as an abstract flight into the deep secrets of nature and a practical tool that can be wielded for humanity's salvation and destruction. As I read the book and pondered Szilard's life I realized that the twentieth century Hungarian would have been right at home in the twenty-first. More than anything else, what makes Szilard remarkable is how prophetically his visions have played out since his death in 1962, all the way to the year 2014. But Szilard was also the quintessential example of a multifaceted individual. If you look at the essential events of the man's life you can see several Szilards, each of whom holds great relevance for the modern world.
There's of course Leo Szilard the brilliant physicist. 

Where he came from precocious ability was commonplace. Szilard belonged to the crop of men known as the "Martians" - scientists whose intellectual powers were off scale - who played key roles in European and American science during the mid-twentieth century. On a strict scientific basis Szilard was not as accomplished as his fellow Martians John von Neumann and Eugene Wigner but that is probably because he found a higher calling in his life. However he certainly did not lack originality. As a graduate student in Berlin - where he hobnobbed with the likes of Einstein and von Laue - Szilard came up with a novel way to consolidate the two microscopic and macroscopic aspects of the science of heat, now called statistical mechanics and thermodynamics. He also wrote a paper connecting entropy and energy to information, predating Claude Shannon's seminal creation of information theory by three decades. In another prescient paper he set forth the principle of the cyclotron, a device which was to secure a Nobel Prize for its recognized inventor - physicist Ernest Lawrence - more than a decade later.

Later during the 1930s, after he was done campaigning on behalf of expelled Jewish scientists and saw visions of neutrons branching out and releasing prodigious amounts of energy, Szilard helped perform some of the earliest experiments in the United States investigating fission, publishing key papers with Enrico Fermi and Walter Zinn in 1939. And while he famously disdained getting his hands dirty, he played a key role in helping Fermi set up the world's first nuclear reactor. As the scientists celebrated the historic moment with a bottle of Chianti, Szilard seems to have stood on the balcony and said, "This will go down as a dark chapter in the history of humanity". Once again he saw the Faustian bargain that the scientists were making with fate.

Szilard as scientist also drives home the importance of interdisciplinary research, a fact which hardly deserves explication in today's scientific world where researchers from one discipline routinely team up with those from others and cross interdisciplinary boundaries with impunity. After the war Szilard became truly interdisciplinary when he left physics for biology and inspired some of the earliest founders of molecular biology, including Jacques Monod, James Watson and Max Delbruck. His reason for leaving physics for biology should be taken to heart by young researchers - he said that while physics was a relatively mature science, biology was a young science where even low hanging fruits were ripe for the picking.

Szilard was not only a notable theoretical scientist but he also had another strong streak, one which has helped so many scientists put their supposedly rarefied knowledge to practical use - that of scientific entrepreneur. His early training had been in chemical engineering, and during his days in Berlin he famously patented an electromagnetic refrigerator with his friend and colleague Albert Einstein; by alerting Einstein to the tragic accidents caused by leakage in mechanical refrigerators, he helped the former technically savvy patent clerk put his knowledge of engineering to good use (as another indication of how underappreciated Szilard remains, the Wikipedia entry on the device is called the "Einstein refrigerator"). Szilard was also finely attuned to the patent system, filing a patent for the nuclear chain reaction with the British Admiralty in 1934 before anyone had an inkling what element would make it work, as well as a later patent for a nuclear reactor with Fermi.

He also excelled at what we today called networking; his networking skills were on full display for instance when he secured rare, impurity-free graphite from a commercial supplier as a moderator in Fermi's nuclear reactor; in fact the failure of German scientists to secure such pure graphite and the subsequent inability of the contaminated graphite to sustain fission damaged their belief in the viability of a chain reaction and held them back. Szilard's networking abilities were also evident in his connections with prominent financiers and bankers who he constantly tried to conscript in supporting his scientific and political adventures; in attaining his goals he would not hesitate to write any letter, ring any doorbell, ask for any amount of money, travel to any land and generally try to use all means at his disposal to secure support from the right authorities. In his case the "right authorities" ranged, at various times in his life, from top scientists to bankers to a Secretary of State (James Byrnes), a President of the United States (FDR) and a Premier of the Soviet Union (Nikita Khrushchev).

I am convinced that had Szilard been alive today, his abilities to jump across disciplinary boundaries, his taste for exploiting the practical benefits of his knowledge and his savvy public relations skills would have made him feel as much at home in the world of Boston or San Francisco venture capitalism as in the ivory tower.

If Szilard had accomplished his scientific milestones and nothing more he would already have been a notable name in twentieth century science. But more than almost any other scientist of his time Szilard was also imbued with an intense desire to engage himself politically - "save the world" as he put it - from an early age. Among other scientists of his time, only Niels Bohr probably came closest to exhibiting the same kind of genuine and passionate concern for the social consequences of science that Szilard did. This was Leo Szilard the political activist. Even in his teens, when the Great War had not even broken out, he could see how the geopolitical landscape of Europe would change, how Russia would "lose" even if it won the war. When Hitler came to power in 1933 and others were not yet taking him seriously Szilard was one of the few scientists who foresaw the horrific legacy that this madman would bequeath Europe. This realization was what prompted him to help Jewish scientists find jobs in the UK, at about the same time that he also had his prophetic vision at the traffic light.

It was during the war that Szilard's striking role as conscientious political advocate became clear. He famously alerted Einstein to the implications of fission - at this point in time (July 1939) Szilard and his fellow Hungarian expatriates were probably the only scientists who clearly saw the danger - and helped Einstein draft the now iconic letter to President Roosevelt. Einstein's name remains attached to the letter, Szilard's is often sidelined; a recent article about the letter from the Institute for Advanced study on my Facebook mentioned the former but not the latter. Without Szilard the bomb would have certainly been built, but the letter may never have been written and the beginnings of fission research in the US may have been delayed. 

When he was invited to join the Manhattan Project Szilard snubbed the invitation, declaring that anyone who went to Los Alamos would go crazy. He did remain connected to the project through the Met Lab in Chicago, however. In the process he drove Manhattan Project security up the wall through his rejection of compartmentalization; throughout his life Szilard had been - in the words of the biologist Jacques Monod - "as generous with his ideas as a Maori chief with his wives" and he favored open and honest scientific inquiry. At one point General Groves who was the head of the project even wrote a letter to Secretary of War Henry Stimson asking the secretary to consider incarcerating Szilard; Stimson who was a wise and humane man - he later took ancient and sacred Kyoto off Groves's atomic bomb target list - refused.

Szilard's day in the sun came when he circulated a petition directed toward the president and signed by 70 scientists advocating a demonstration of the bomb to the Japanese and an attempt at cooperation in the field of atomic energy with the Soviets. This was activist Leo Szilard at his best. Groves was livid, Oppenheimer - who by now had tasted power and was an establishment man - was deeply hesitant and the petition was stashed away in a safe until after the war. Szilard's disappointment that his advice was not heeded turned to even bigger concern after the war when he witnessed the arms race between the two superpowers. In 1949 he wrote a remarkable fictitious story titled 'My Trial As A War Criminal' in which he imagined what would have happened had the United States lost the war to the Soviets; Szilard's point was that in participating in the creation of nuclear weapons, American scientists were no less or more complicit than their Russian counterparts. Szilard's take on the matter raised valuable questions about the moral responsibility of scientists, an issue that we are grappling with even today. 

The story played a small part in inspiring Soviet physicist Andrei Sakharov in his campaign for nuclear disarmament. Szilard also helped organize the Pugwash Conferences for disarmament, gave talks around the world on nuclear weapons, and met with Nikita Khrushchev in Manhattan in 1960; the result of this amiable meeting was both the gift of a Schick razor to Khrushchev and, more importantly, Khrushchev agreeing with Szilard's suggestion that a telephone hot-line be installed between Moscow and Washington for emergencies. The significance of this hot-line was acutely highlighted by the 1962 Cuban missile crisis. Sadly Szilard's later two attempts at meeting with Khrushchev failed.

After playing a key role in the founding of the Salk Institute in California, Szilard died peacefully in his sleep in 1964, hoping that the genie whose face he had seen at the traffic light in 1933 would treat human beings with kindness.

Since Szilard the common and deep roots that underlie the tree of science and politics have become far clearer. Today we need scientists like Szilard to stand up for science every time a scientific issue such as climate change or evolution collides with politics. When Szilard pushed scientists to get involved in politics it may have looked like an anomaly, but today we are struggling with very similar issues. As in many of his other actions, Szilard's motto for the interaction of science with politics was one of accommodation. He was always an ardent believer in the common goals that human beings seek, irrespective of the divergent beliefs that they may hold. He was also an exemplar of combining thought with action, projecting an ideal meld of the idealist and the realist. Whether he was balancing thermodynamic thoughts with refrigeration concerns or following up political idealism with letters to prominent politicians, he taught us all how to both think and do. As interdisciplinary scientist, as astute technological inventor, as conscientious political activist, as a troublemaker of the best kind, Leo Szilard leaves us with an outstanding role model and an enduring legacy. It is up to us to fill his shoes.

The Ten Commandments of Molecular (and other) Modeling

Thou shalt not extrapolate too much beyond the training data.

Thou shalt prioritize simple experiments over complex models.

Thou shalt never forget the difference between accuracy and precision.

Thou shalt never try to woo thy audience with pretty pictures or tales of fast GPUs.

Thou shalt not worship “physics-based” models that are not actually physics-based.

Thou shalt not be biased toward favorite models and should use whatever gets the job done.

Thou shalt use good statistics as much as possible.

Thou shalt always remember that modeling is a means and a tool, not an end unto itself.

Thou shalt always understand and explain the limitations of thy models.

Thou shalt never forget: Only good experiments can uncover facts. The rest is crude poetry and imagination. 

The only two equations that you should know

“Chemistry”, declared the Nobel laureate Roger Kornberg in an interview, “is the queen of all sciences. Our best hope of applying physical principles to the world around us is at the level of chemistry. In fact if there is one subject which an educated person should know in the world it is chemistry.” Kornberg won the 2006 Nobel Prize in chemistry for his work on transcription which involved unraveling the more than dozen complicated proteins involved in the copying of DNA into RNA. He would know how important chemistry is in uncovering the details of a ubiquitous life process.
I must therefore inevitably take my cue from Kornberg and ask the following question: What equation would you regard as the most important one in science? For most people the answer to this question would be easy: Einstein’s famous mass-energy formula, E=mc2. Some people may cite Newton’s inverse square law of gravitation. And yet it should be noted that both of these equations are virtually irrelevant for the vast majority of practicing physicists, chemists and biologists. They are familiar to the public mainly because they have been widely publicized and are associated with two very famous scientists. There is no doubt that both Einstein and Newton are supremely important for understanding the universe, but they both suffer from the limitations of reductionist science that preclude the direct application of the principles of physics to the everyday workings of life and matter.
Take Einstein’s formula for instance. About the only importance it has for most physical scientists is the fact that it is responsible for the nuclear processes that have forged the elements in stars and supernova. Chemists deal with reactions that involve not nuclear processes but the redistribution of electrons. Except in certain special cases, Einstein therefore does not figure in chemical or biological processes. Newton’s gravitational formula is equally distant for most chemists' everyday concerns. Chemistry hinges on the attraction and repulsion of charges, processes overwhelmingly governed by the electromagnetic force. This force is stronger than the gravitational force by a factor of 1036, an unimaginably large number. Gravity is thus too weak for chemists and biologists to bother with in their work. The same goes for many physicists who deal with atomic and molecular interactions.
Instead here are two equations which have a far greater and more direct relevance to the work done by most physical and biological scientists. The equations lie at the boundary of physics and chemistry, and both of them are derived from a science whose basic truths are so permanently carved in stone that Einstein thought they would never, ever need to be modified. The man who contributed the most to their conception, Josiah Willard Gibbs, was called "the greatest mind in American science" by Einstein. The science that Gibbs, Helmholtz, Clausius, Boltzmann and others created is thermodynamics, and the equations we are talking about involve its most basic quantities. They apply without exception to every important physical and chemical process you can think of, from the capture of solar energy by plants and solar cells to the combustion of fuel inside trucks and human bodies to the union between sperm and egg.
Two thermodynamic quantities govern molecular behavior, and indeed the behavior of all matter in the universe. One is the enthalpy, usually denoted by the symbol H, and roughly representing the quantity of energy and the strength of interactions and bonds between different atoms and molecules. The other is the entropy, usually denoted by the symbol S, and roughly representing the quality of energy and the disorder in any system. Together the enthalpy and entropy make up the free energy G, which roughly denotes the amount of useful work that can be extracted from any living or non-living system. In practical calculations, what we are concerned with are changes in these quantities rather than their absolute values, so each one of them is prefaced by the symbol ∆, indicating change. The celebrated second law of thermodynamics states that the entropy of a spontaneous process always increases, and it is indeed one of the universal facts of life, but that is not what we are concerned with here.
Think about what happens when two molecules – of any kind – interact with each other. The interaction need not even be an actual reaction, it can simply be the binding of two molecules to one another by strong or weak forces. The process is symbolized by an equilibrium constant Ke, which is simply the ratio of the concentrations of the products of the reaction to the starting materials (reactants). The bigger the equilibrium constant, the more the amount of the products. Ke thus tells us how much of a reaction has been completed and how much reactant has been converted to product. Our first great equation relates this equilibrium constant to the free energy of the interaction through the following formula:
∆G0 = -RT ln Ke
or, in other words
Ke = e-∆G0/RT
Here ln is the natural logarithm to base e, R is a fundamental constant called the gas constant, T is the ambient temperature and ∆Gis the free energy change under so-called 'standard conditions' (a detail which can be ignored by the reader for the sake of this discussion). This equation tells us two major things and one minor thing. The minor thing is that reactions can be driven in particular directions by temperature increases, and exponentially so. But the major things are what's critical here. Firstly, the equation says that the free energy in a spontaneous process with a favorable positive equilibrium constant is always going to be negative; the more negative it is the better. And that is what you find. The free energy change for many of biology's existential reactions like the coupling of biological molecules with ATP (the “energy currency” of the cell), the process of electron transfer mediated by chlorophyll and the oxidation of glucose to provide energy is indeed negative. Life has also worked out ingenious little tricks to couple reactions with positive (unfavorable) ∆G changes to those with negative ∆G0 values to give an overall favorable free energy profile.
The second feature of the equation is a testament to the wonder that is life, and it never ceases to amaze me. It attests to what scientists and philosophers have called “fine-tuning”, the fact that evolution has somehow succeeded in minimizing the error inherent in life’s processes, in carefully reining in the operations of life to within a narrow window. Look again at that expression. It says that ∆G0 is related to Ke not linearly but exponentially. That is a dangerous proposition because it means that even a tiny change in ∆G0 will correspond to a large change in Ke. How tiny? It should be no bigger than 3 kcal/mol.
A brief digression to appreciate how small this value is. Energies in chemistry are usually expressed as kilocalories per mole. A bond between two carbon atoms is about 80 kcal/mol. A bond between two nitrogen atoms is 226 kcal/mol: this is why nitrogen can be converted to ammonia by breaking this bond only at very high temperatures and pressures and in the presence of a catalyst. A hydrogen bond - the "glue" that holds biological molecules like DNA and proteins together - is anywhere between 2 and 10 kcal/mol.
3 kcal/mol is thus a fraction of the typical energy of a bond. It takes just a little jiggling around to overcome this energy barrier. The exponential, highly sensitive dependence of Ke on ∆G0 means that changing ∆G from close to zero to 3 kcal/mol will translate to changing Ke from 1:99.98 in favor of products to 99.98:1 in favor of reactants (remember that Ke is a ratio). This is a simple mathematical truth. Thus, a tiny change in ∆G0 can all but completely shift a chemical reaction from favoring products to favoring reactants. Naturally this will be very bad if the goal of a reaction is to create products that are funneled into the next chemical reaction. Little changes in the free energy can therefore radically alter the flux of matter and energy in life’s workings. But this does not happen. Evolution has fine-tuned life so well that it has remained a game played within a 3 kcal/mol energy window for more than 2.5 billion years. It's so easy for this game to quickly spiral out of hand, but it doesn’t. It doesn’t for the trillions of chemical transactions which trillions of cells execute everyday in every single organism on this planet.
And it doesn’t happen for a reason; because cells would have a very hard time modulating their key chemical reactions if the free energies involved in those reactions had been too large. Life would be quickly put into a death trap if every time it had to react, fight, move or procreate it had to suddenly change free energies for each of its processes by tens of kilocalories per mole. There are lots of bonds broken and formed in biochemical events, of course, and as we saw before, these bond energies can easily amount to dozens of kcals/mol. But the tendency of the reactants or products containing those bonds to accumulate is governed by these tiny changes in free energy which nudge a reaction one way or another. In one sense then, life is optimizing small changes (in free energy of reactions) between two large numbers (bond energies). This is always a balancing act on the edge of a cliff, and life has managed to be successful in it for billions of years. It's one of the great miracles of the universe.
The second equation is also a relationship between free energy, enthalpy and entropy. It's simpler than the first, but no less important:
∆G = ∆H - T∆S
The reason this equation is also crucial to the operation of the universe is because it depicts a fine dance between entropy and enthalpy that dictates whether physical processes will happen. Note that entropy is multiplied by the temperature here and the sign is negative. So if it decreases in a process then ∆S becomes negative and the overall product (T∆S) becomes positive. In that case the change in enthalpy needs to be negative enough to compensate, otherwise the free energy will not be negative and the process won't take place. 
For instance, consider the schoolboy experiment of oil and water not mixing. When oil is put into water, the water molecules have to order themselves around oil molecules, leading their entropy to decrease and become negative. The attraction between water and oil on the other hand is weak, so the change in enthalpy does not compensate for the change in entropy, and oil does not mix. This is called the hydrophobic effect. It's a fundamental effect governing a myriad of critical phenomena; drugs interacting with signaling proteins, detergents interacting with grease, food particles attracting or repelling each other inside saucepans and human bodies. On the other hand, salt and water mix easily; in this case, while the entropy is still unfavorable because of the ordering of water molecules around salt molecules, the enthalpy is overwhelmingly favorable (negative) because the positive and negatively charged sodium and chloride ions strongly attract water.
Because temperature is part of the equation it too plays an important role. For instance consider a phenomenon like a chemical reaction in which the change in entropy is favorable but quite small. We can then imagine that this reaction will be greatly accelerated if T is high, making the product of it and the entropy large. This explains why the free energy of chemical reactions can be made much more favorable at high temperatures (there is a subtlety here, however: making the free energy more favorable is not the same as accelerating the reactions, it's simply making the products more stable. The difference is between thermodynamics and kinetics).
Even the origin of life during which the exact nature of molecular interactions was crucial in deciding which ones would survive, replicate and thrive was critically dependent on enthalpy and entropy. When little oily molecules called micelles repelled water molecules because of the unfavorable entropy and enthalpy described above, they sequestered themselves into tiny bags inside which fragile molecules like DNA and RNA could safely isolate themselves from the surrounding water. These DNA and RNA molecules could then experiment with copying themselves at leisure, not having to worry about being hydrolyzed by water. The ones with higher fitness survived, kickstarting the process which, billions of years later, finally led to this biped typing these words on his computer.
That's really all there is to life. We all thus hum along smoothly, beneficiaries of a 3 kilocalorie energy window and of the intricate dance of entropy and enthalpy, going about our lives even as we are held hostage to the quirks of thermodynamic optimization, walking along an exponential energy precipice.
And all because Ke = e-∆G0/RT