Tuesday, March 26, 2013
Finally, Henderson's masterful book is back in print, issued by MIT Press in a brand new edition. The new edition begins with a magnificent "reintroduction" spanning the latter half of the 20th century (1950s - 2000), and including vital cultural connections between the fourth dimension and the visual arts (along with other media). As Henderson demonstrates, interest in higher dimensions has grown in recent decades through the emergence of string theory and other scientific ideas. This rebirth of interest has been reflected in artistic ventures of the period.
The Fourth Dimension And Non-Euclidean Geometry In Modern Art is an essential book for anyone interested in the intersection between science, mathematics and culture. It offers a riveting chronicle of the emergence of the idea of the fourth dimension in math, its popularization in literature and its adoption by the world of art that has persisted until the present day. Highly recommended!
Sunday, July 15, 2012
Saturday, July 16, 2011
By Paul Halpern
Excerpted from “Washington: A DC Circuit Tour,” P. Halpern, Physics in Perspective 12, No. 4, (2010), pp. 443-466. All photos by Aden Halpern and Paul Halpern, except for the photo of the historic Van de Graaff generator at the Department of Terrestrial Magnetism, used by permission of the Carnegie Institution of Washington.
Stop 1: Joseph Henry Statue
We start our walk at the statue of Joseph Henry located in the National Mall directly in front of the “castle” housing the headquarters of the Smithsonian Institution (Smithsonian Metro Station). Designed by William Wetmore Story, the statue was dedicated in 1883. A widely accomplished physicist, Henry served as the first Secretary of the Smithsonian Institution.
Stop 2: The Smithsonian Building
We now walk from the Henry statue to the castle-like edifice behind it, the Smithsonian Building, completed in 1855. On the south side of the Smithsonian Building is an area known as the South Yard where, from 1890 to 1955, a shed housed the Smithsonian Astrophysical Observatory, one of the first centers in the world for astrophysical research.
Stop 3: U.S. Department of Energy
Across Independence Avenue from the Smithsonian’s South Yard is the Forrestal Building, which was built in 1970 and today houses the U.S. Department of Energy.
Stop 4: The Continuum Sculpture and the National Air and Space Museum
Going east along Independence Aveue and crossing 7th Street SW, we see on our left the National Air and Space Museum. Directly in front of its entrance is the modern sculpture Continuum, which was commissioned in 1976 and designed by artist Charles O. Perry to represent a distorted region of spacetime in the vicinity of a black hole.
Stop 5: Koshland Science Museum
Crossing the National Mall and walking due north several blocks along 6th Street NW, we arrive at the corner of E Street and find ourselves at the entrance of the Marion Koshland Science Museum of the National Academy of Sciences, which specializes in contemporary scientific issues.
Stop 6: National Museum of American History
Walking six blocks west along E Street, and then the equivalent of three blocks south along 12th Street NW, we arrive at Constitution Avenue and see on the other side of it the entrance to the National Museum of American History (Federal Triangle Metro Station). Long a part of the Smithsonian, it has two significant collections on physics: the Physical Sciences Collection and the Modern Physics Collection.
Stop 7: Albert Einstein Memorial and the National Academy of Sciences
We exit the National Museum of American History and walk eight blocks west on Constitution Avenue, cross 21st Street NW, and see the Albert Einstein Memorial in a shady grove in front of the National Academy of Sciences. It features a 12-foot bronze statue of Einstein, weighing about 4 tons, that was sculpted by Robert Berks to depict the founder of relativity in his later years.
Stop 8: Corcoran Hall: George Washington University
We now stroll the equivalent of about four blocks north on 21st Street NW, cross G Street, and reach Corcoran Hall, home of the Department of Physics of George Washington University since 1924.. GWU’s Department of Physics rose to prominence internationally with the appointment of Russian physicist George Gamow in 1934 and of Hungarian physicist Edward Teller in 1935. Plaques honoring Gamow and Teller, along with the Fifth Washington Conference on Theoretical Physics are featured on the wall facing 21st Street. At that conference, which took place at GWU in 1939, Niels Bohr announced to the astonished participants the discovery of nuclear fission in Germany.
Stop 9: Carnegie Institution of Washington
We now leave GWU and stroll seven blocks north along 21st Street NW to P Street. Then we turn right and go five blocks east to the corner of 16th Street NW and P Street where the Carnegie Institution of Washington (also known as the Carnegie Institution for Science) is situated (Dupont Circle Metro Station). Its three divisions with the deepest connections to physics are the Observatories Department (originally just Mount Wilson Observatory), the Department of Terrestrial Magnetism, and the Geophysical Laboratory.
The Carnegie Institution’s Department of Terrestrial Magnetism, founded in 1904 under the directorship of American physicist Louis Agricola Bauer, is housed in separate quarters at 5241 Broad Branch Road NW in the leafy northwestern corner of the District. It includes a pioneering Van de Graaff accelerator, completed in 1933 by physicist Merle Tuve, and used to explore the realm of the nucleus.
The Geophysical Laboratory was founded in 1905 and was located on Upton Street NW before it was relocated to the Broad Branch Road campus near the DTM in 1990. (Mt. Wilson Observatory is in California and not included on this walking tour except for the very athletic.)
Stop 10: Oak Hill Cemetery in Georgetown
From the main headquarters of the Carnegie Institution on the corner of 16th Street NW and P Street, we go two blocks north to Q Street and then the equivalent of eight blocks west, crossing the bridge over Rock Creek, to reach Oak Hill Cemetery in venerable Georgetown. Among the notables buried there is Joseph Henry whose grave is prominently located in the section called “Henry Crescent” near the East Gate.
Stop 11: American Center for Physics in College Park
Visiting the American Center for Physics, the final stop on our tour, requires a trip by Metro to the College Park Metro Station and a brief walk. Established in 1993 under the leadership of Kenneth W. Ford, the American Center for Physics houses the American Institute of Physics, the American Physical Society, the American Association of Physics Teachers, the American Association of Physicists in Medicine, and the Society of Physics Students. The ACP also houses the AIP Center for History of Physics with its Niels Bohr Library and Archives and the Emilio Segrè Visual Archives.
Thanks to Roger Stuewer for suggesting and editing the article on which this guide is based, to Greg Good for helpful suggestions, and to Shaun Hardy for suggesting that I post a web version of my guide.
Wednesday, February 16, 2011
Wednesday, May 19, 2010
Saturday, May 1, 2010
THE CAVE OF PORTENTS by Paul Halpern (1999)
Deep within the cave of portents, carved out over the eons by the currents of possibility, lies a chamber known for its auspicious acoustic qualities. Explorers stumbling upon that cavern have reported hearing beautiful melodies played out among the stony columns like the sonorant tones of wind chimes. Some have also recalled hearing soft whispering sounds, almost like the murmur of human voices. They have attributed these strange phenomena to peculiar resonant effects--a remarkable auditory illusion.
What makes matters even more intriguing are the presence of rocky formations in the chamber that seem to resemble human visages. Throughout the years since the cave was discovered, adventurers have nicknamed each of the stone faces after a historical or scientific figure.
One explorer, with a passion for philosophy, nicknamed one of the figures, “Pythagoras,” and another neighboring image, “Cicero,” because of their marked resemblances to those illustrious personages. A German exchange student, who gained admission to the caves as part of a summer research project, dubbed a craggy pillar close to the others, “Johannes Kepler,” after the 16th century astronomer of whose portrait it reminded him. A French spelunker, with a fondness for astrology, proudly selected the nickname “Nostradamus” for another rockface that seemed to have fiery, visionary eyes. Finally, to add to the eclectic mix of personalities, another caver, who knew modern physics very well, swore he saw the wild-haired image of Albert Einstein in one column, and the warm smile and deep, expressive glance of Richard Feynman in another.
With lanterns positioned well, these illusions were often enhanced by the strange rhythmic movements of shadows near the figures--suggesting the graceful gestures of musicians. Some have jokingly attributed the "concerts" and "conversations" seen and heard in the cavern to apparitions of the late scientists and philosophers, hovering near their stony likenesses. Hence the nickname for the chamber "harmony of the spirits."
Imagine the glorious music that would be made, and the striking and curious conversations that would resonate throughout the chamber, if the cave’s illusion suddenly and magically became real...
* * *
One Sunday morning, after an especially tuneful performance on his limestone "piano," the spirit of Kepler sighed and uttered, "Did you ever think we'd all end up here making music together?"
Nostradamus, who was chanting verses at the time, responded, "I knew. I pictured this strange cave, where great minds might harmonize, during one of my psychic excursions into the time of the third millennium. Like my other prophecies, it appeared to me during my nightly meditations upon water-filled glass. Through such exercises, I have witnessed all of history until the year 3797."
Cicero winced. "Another one of your preposterous claims. As usual, with unmatched zeal, but without a crumb of proof, you purport that the future is wholly predictable."
Nostradamus remarked in a huff, "It is predictable only to those who possess the powers of prophecy. Only those who lack the God-given vision to foresee the unraveling of the ages call my work preposterous."
At that point Pythagoras put down his lyre and joined in on the conversation. "Oh that vision thing again," he sneered. "You act as if the skill of foretelling the future is your exclusive domain. The gods have revealed man's destiny in the miraculous properties of numbers, and in the harmonious relationships between musical tones. Like a child taught the alphabet, any intelligent individual, properly trained in a superior academy, might be made aware of the wonders of the cosmos, deciphering its marvelous code."
Kepler spoke up. "Indeed, like Nostradamus, I've offered my share of horoscopes. The public expected me to provide such a service. But I've never claimed to be a prophet. My most fulfilling task, the discovery of the patterns of planetary orbits, I can attribute to my background in classical geometry. Simple, beautiful mathematics, not superstition, was the key to my success."
Pythagoras nodded his head. "Exactly. The cosmos is a vast fruit and mathematics is its pith. Those who peel off the outer layers of corporeal illusion, and savor the rich pulp of numerical truth, might truly taste their destinies."
Cicero looked up. "But what then. Suppose you use instinct, mathematics, examining animal entrails, or whatever your favorite method to discern the future. Does that mean, then, that you have discovered what must be in times to come or what could be in times to come? If you have found the former--the immutable future, then what's that point? What's the purpose of knowing something that you can't change? Just to be depressed? If Caesar knew his fate well in advance, but couldn't change it, perhaps he would have been an unhappy, ineffective leader. Bitter certainty would have engulfed him in a cloak of despair. And he would have been assassinated anyway.
On the other hand, if through your prognosticative abilities you have found mere possibilities or probabilities for the future--then there also would be no point. The winds of destiny could blow in another direction, and your prediction would be dead wrong anyway. You'd be chasing after specters in the dark, while reality passes you by."
Feynman, who had been banging his beloved bongo drums, glanced over when he heard the word "probability."
"Well that's all you can really know. Probabilities."
Cicero replied, "What do you mean?"
Feynman assumed his familiar pedagogical role. "Its too bad I don't have a blackboard here, but I'll try to explain without diagrams. Let me point out some of the ways classical physics and quantum mechanics fundamentally differ in how they treat basic interactions between particles. I’d like to consider the simple case of one electron exerting a force on another electron by means of exchanging a photon.
In classical physics, which is extraordinarily more intuitive than quantum theory, given their initial locations and speeds, one can map out the exact paths that the two electrons first take. Then one can examine how the first electron gives off a photon, and then recoils, like a gun firing off a bullet. Next, one can calculate precisely how the second electron absorbs the photon. Lastly, by means of the principles of conservation of energy and conservation of momentum, one can determine the ultimate trajectories and velocities of the particles. In short, by knowing the initial conditions one can infer exactly which routes are traveled, knowing with perfect precision the position and speed of each object for all times."
Kepler looked at Feynman and smiled. “Richard, I wish I could explain things so well. It all makes such perfect sense.”
Feynman chuckled. “Unfortunately everything I just said was wrong. Why? The reason is crazy, and I expect no one to believe it, not even the eminent thinkers in this chamber. Sometimes I don’t even know if I believe it myself. Physicists have given up to trying to predict anything exactly, because experimental evidence tells us that we just can’t do it. The uncertainty principle, a built in law of nature, restricts what we might know at any given moment. If we know a particle’s position perfectly well, then we don’t know its speed, and vice-versa.
In general, until we make an observation, all we can determine about a system is a set of probabilities. Then after we measure one particular quantity, the mere fact that we have observed the system shakes it up and affects its other properties, altering the probabilities that they have certain values. In other words, the future state of a system depends upon the choices made by observers.”
Kepler and Pythagoras exchanged puzzled glances. “But surely the magnificent harmony of nature has little to do with the decisions made by mortals,” stated Pythagoras.
“One would think,” replied the great theorist. “But one would get the wrong answer. For instance, in the scattering example I just mentioned one cannot assume that the electrons and photons followed only one trajectory. Rather, in quantum theory, one must consider the likelihoods of all possible exchanges between the particles, including bizarre situations such as photons traveling backward in time to meet electrons. Only by summing up these probabilities, in a special manner that takes a bit of mathematical juggling, might one be able to estimate likely outcomes.”
Kepler was intrigued, "Ah, I see. What I think you are saying, my spirited companion, is that nature is like a safe. To unlock its riddles, you must try each of the possible combinations it presents."
Feynman smiled. "Well, I would only need to try a few combinations--but I've had plenty of practice cracking open document drawers in Los Alamos. Nature, on the other hand, probes an infinite range of possibilities. But remarkably, one often can add up these infinite sums and obtain finite solutions to physical problems."
Einstein, who had been listening to the conversation while tuning his violin, looked dismayed.
"Ach, mein Freund. Gott ist im Himmel, nicht in Monte Carlo. Do you mean that there is only a finite probability that we are here, and that our energies might simultaneously occupy other configurations as well. Then how do we know precisely where we are?"
"Well if an observer were around to take a measurement of our locations, our wave functions might collapse to a particular position value. We may find ourselves still here, or conversely, we might not be here at all."
"An observer? Why, who might be here to observe us? I don't think anyone is paying attention to our proceedings?"
At that point the chamber became strangely silent. The winds seemed to shift, a lamp blew out, and the remarkable acoustical and optical illusions were no more.
Saturday, April 10, 2010
Last year I was interviewed about the science of prediction on the Discovery Channel for a show called Nostradamus Decoded. The show aired in November 2009 and is now available online.
My short segment starts at about 3:06 into the episode.
More about the science of prediction is in my book: