M Planck Quotes

You could give Aristotle a tutorial. And you could thrill him to the core of his being. Aristotle was an encyclopedic polymath, an all time intellect. Yet not only can you know more than him about the world. You also can have a deeper understanding of how everything works. Such is the privilege of living after Newton, Darwin, Einstein, Planck, Watson, Crick and their colleagues. I'm not saying you're more intelligent than Aristotle, or wiser. For all I know, Aristotle's the cleverest person who ever lived. That's not the point. The point is only that science is cumulative, and we live later.

Planck noted that although the Andromedans wouldn't have access to our rulers, scales, or clocks, they would have access to our physical laws, which are the same as theirs. They could measure, in particular, three universal constants: c: The speed of light. G: Newton's gravitational constant. In Newton's theory, this is a measure of the strength of gravity. To be precise, in Newton's law of gravity, the gravitational force between the bodies of masses m1, m2 separated by distance r is Gm1m2/r^2. h: Planck's constant.

Of course, I’ve only brought up two examples. Other universal laws of physics have been used as weapons as well, though we don’t know all of them. It’s very possible that every law of physics has been weaponized. It’s possible that in some parts of the universe, even … Forget it, I don’t even believe that.” “What were you going to say?” “The foundation of mathematics.” Cheng Xin tried to imagine it, but it was simply impossible. “That’s … madness.” Then she asked, “Will the universe turn into a war ruin? Or, maybe it’s more accurate to ask: Will the laws of physics turn into war ruins?” “Maybe they already are.… The physicists and cosmologists of the new world are focused on trying to recover the original appearance of the universe before the wars more than ten billion years ago. They’ve already constructed a fairly clear theoretical model describing the pre-war universe. That was a really lovely time, when the universe itself was a Garden of Eden. Of course, the beauty could only be described mathematically. We can’t picture it: Our brains don’t have enough dimensions.” Cheng Xin thought back to the conversation with the Ring again. Did you build this four-dimensional fragment? You told me that you came from the sea. Did you build the sea? “You are saying that the universe of the Edenic Age was four-dimensional, and that the speed of light was much higher?” “No, not at all. The universe of the Edenic Age was ten-dimensional. The speed of light back then wasn’t only much higher—rather, it was close to infinity. Light back then was capable of action at a distance, and could go from one end of the cosmos to the other within a Planck time.… If you had been to four-dimensional space, you would have some vague hint of how beautiful that ten-dimensional Garden must have been.” “You’re saying—” “I’m not saying anything.” Yifan seemed to have awakened from a dream. “We’ve only seen small hints; everything else is just guessing. You should treat it as a guess, just a dark myth we’ve made up.” But Cheng Xin continued to follow the course of the discussion taken so far. “—that during the wars after the Edenic Age, one dimension after another was imprisoned from the macroscopic into the microscopic, and the speed of light was reduced again and again.…” “As I said, I’m not saying anything, just guessing.” Yifan’s voice grew softer. “But no one knows if the truth is even darker than our guesses.… We are certain of only one thing: The universe is dying.” The

The great German physicist Max Planck had been advised by his lecturer, the marvellously named Philipp von Jolly, not to pursue the study of physics because “almost everything is already discovered, and all that remains is to fill a few unimportant holes.” Planck replied that he had no wish to discover new things, only to understand the known fundamentals of the field better. Perhaps unaware of the old maxim that if you want to make God laugh you tell him your plans, he went on to become a founding father of quantum physics. Scientists

This was a golden age, in which we solved most of the major problems in black hole theory even before there was any observational evidence for black holes. In fact, we were so successful with the classical general theory of relativity that I was at a bit of a loose end in 1973 after the publication with George Ellis of our book The Large Scale Structure of Space–Time. My work with Penrose had shown that general relativity broke down at singularities, so the obvious next step would be to combine general relativity—the theory of the very large—with quantum theory—the theory of the very small. In particular, I wondered, can one have atoms in which the nucleus is a tiny primordial black hole, formed in the early universe? My investigations revealed a deep and previously unsuspected relationship between gravity and thermodynamics, the science of heat, and resolved a paradox that had been argued over for thirty years without much progress: how could the radiation left over from a shrinking black hole carry all of the information about what made the black hole? I discovered that information is not lost, but it is not returned in a useful way—like burning an encyclopedia but retaining the smoke and ashes. To answer this, I studied how quantum fields or particles would scatter off a black hole. I was expecting that part of an incident wave would be absorbed, and the remainder scattered. But to my great surprise I found there seemed to be emission from the black hole itself. At first, I thought this must be a mistake in my calculation. But what persuaded me that it was real was that the emission was exactly what was required to identify the area of the horizon with the entropy of a black hole. This entropy, a measure of the disorder of a system, is summed up in this simple formula which expresses the entropy in terms of the area of the horizon, and the three fundamental constants of nature, c, the speed of light, G, Newton’s constant of gravitation, and ħ, Planck’s constant. The emission of this thermal radiation from the black hole is now called Hawking radiation and I’m proud to have discovered it.

Walking in circles Dr. Jan Souman, of the Max Planck Institute for Biological Cybernetics, studied what happens to us when we have no map, no compass, no way to determine landmarks. I’m not talking about a metaphor—he researched what happens to people lost in the woods or stumbling around the Sahara, with no north star, no setting sun to guide them. It turns out we walk in circles. Try as we might to walk in a straight line, to get out of the forest or the desert, we end up back where we started. Our instincts aren’t enough. In the words of Dr. Souman, “Don’t trust your senses because even though you might think you are walking in a straight line when you’re not.” Human nature is to need a map. If you’re brave enough to draw one, people will follow.

Music of the Grid: A Poem in Two Equations _________________________ The masses of particles sound the frequencies with which space vibrates, when played. This Music of the Grid betters the old mystic mainstay, "Music of the Spheres," both in fantasy and in realism. LET US COMBINE Einstein's second law m=E/C^2 (1) with another fundamental equation, the Planck-Einstein-Schrodinger formula E = hv The Planck-Einstein-Schrodinger formula relates the energy E of a quantum-mechanical state to the frequency v at which its wave function vibrates. Here h is Planck's constant. Planck introduced it in his revolutionary hypothesis (1899) that launched quantum theory: that atoms emit or absorb light of frequency v only in packets of energy E = hv. Einstein went a big step further with his photon hypothesis (1905): that light of frequency v is always organized into packets with energy E = hv. Finally Schrodinger made it the basis of his basic equation for wave functions-the Schrodinger equation (1926). This gave birth to the modern, universal interpretation: the wave function of any state with energy E vibrates at a frequency v given by v = E/h. By combining Einstein with Schrodinger we arrive at a marvelous bit of poetry: (*) v = mc^2/h (*) The ancients had a concept called "Music of the Spheres" that inspired many scientists (notably Johannes Kepler) and even more mystics. Because periodic motion (vibration) of musical instruments causes their sustained tones, the idea goes, the periodic motions of the planets, as they fulfill their orbits, must be accompanied by a sort of music. Though picturesque and soundscape-esque, this inspiring anticipation of multimedia never became a very precise or fruitful scientific idea. It was never more than a vague metaphor, so it remains shrouded in equation marks: "Music of the Spheres." Our equation (*) is a more fantastic yet more realistic embodiment of the same inspiration. Rather than plucking a string, blowing through a reed, banging on a drumhead, or clanging a gong, we play the instrument that is empty space by plunking down different combinations of quarks, gluons, electrons, photons,... (that is, the Bits that represent these Its) and let them settle until they reach equilibrium with the spontaneous activity of Grid. Neither planets nor any material constructions compromise the pure ideality of our instrument. It settles into one of its possible vibratory motions, with different frequencies v, depending on how we do the plunking, and with what. These vibrations represent particles of different mass m, according to (*). The masses of particles sound the Music of the Grid.

Two observations take us across the finish line. The Second Law ensures that entropy increases throughout the entire process, and so the information hidden within the hard drives, Kindles, old-fashioned paper books, and everything else you packed into the region is less than that hidden in the black hole. From the results of Bekenstein and Hawking, we know that the black hole's hidden information content is given by the area of its event horizon. Moreover, because you were careful not to overspill the original region of space, the black hole's event horizon coincides with the region's boundary, so the black hole's entropy equals the area of this surrounding surface. We thus learn an important lesson. The amount of information contained within a region of space, stored in any objects of any design, is always less than the area of the surface that surrounds the region (measured in square Planck units). This is the conclusion we've been chasing. Notice that although black holes are central to the reasoning, the analysis applies to any region of space, whether or not a black hole is actually present. If you max out a region's storage capacity, you'll create a black hole, but as long as you stay under the limit, no black hole will form. I hasten to add that in any practical sense, the information storage limit is of no concern. Compared with today's rudimentary storage devices, the potential storage capacity on the surface of a spatial region is humongous. A stack of five off-the-shelf terabyte hard drives fits comfortable within a sphere of radius 50 centimeters, whose surface is covered by about 10^70 Planck cells. The surface's storage capacity is thus about 10^70 bits, which is about a billion, trillion, trillion, trillion, trillion terabytes, and so enormously exceeds anything you can buy. No one in Silicon Valley cares much about these theoretical constraints. Yet as a guide to how the universe works, the storage limitations are telling. Think of any region of space, such as the room in which I'm writing or the one in which you're reading. Take a Wheelerian perspective and imagine that whatever happens in the region amounts to information processing-information regarding how things are right now is transformed by the laws of physics into information regarding how they will be in a second or a minute or an hour. Since the physical processes we witness, as well as those by which we're governed, seemingly take place within the region, it's natural to expect that the information those processes carry is also found within the region. But the results just derived suggest an alternative view. For black holes, we found that the link between information and surface area goes beyond mere numerical accounting; there's a concrete sense in which information is stored on their surfaces. Susskind and 'tHooft stressed that the lesson should be general: since the information required to describe physical phenomena within any given region of space can be fully encoded by data on a surface that surrounds the region, then there's reason to think that the surface is where the fundamental physical processes actually happen. Our familiar three-dimensional reality, these bold thinkers suggested, would then be likened to a holographic projection of those distant two-dimensional physical processes. If this line of reasoning is correct, then there are physical processes taking place on some distant surface that, much like a puppeteer pulls strings, are fully linked to the processes taking place in my fingers, arms, and brain as I type these words at my desk. Our experiences here, and that distant reality there, would form the most interlocked of parallel worlds. Phenomena in the two-I'll call them Holographic Parallel Universes-would be so fully joined that their respective evolutions would be as connected as me and my shadow.

El patrón de la apertura a la experiencia ya había sido estudiado. (...) Una característica era la juventud asociada al proceso creativo. Algunas profesiones se construyen exclusivamente sobre los avances creativos de niños prodigio (como por ejemplo, las matemáticas). Otras son menos extremas del mismo patrón: el número de melodías anuales de un compositor, los poemas de un poeta, los descubrimientos nuevos de un científico marcan un declive general pasado cierto pico de relativa juventud. Las grandes mentes creativas no sólo suelen generar cada vez menos descubrimientos a medida que pasa el tiempo, sino que están menos abiertas a aceptar los inventos de otros. (...) Como señaló el físico Max Planck, generaciones enteras de científicos sólidamente establecidos nunca aceptan las teorías nuevas, se mueren antes. (...) La estrechez mental da como resultado a un revolucionario envejecido que rechaza precisamente lo que debería haber sido la extensión lógica de su propia revolución. Tenemos el surgimiento de una pauta consistente: a medida que envejecemos, la mayoría de nosotros (los científicos de más edad fustigando a sus discípulos descarriados, la persona que pasa el día en el coche para ir a trabajar tratando de sintonizar en la radio una emisora que ponga una canción familiar) estamos menos abiertos a las novedades que otros. (...) Como la neurobiología no era gran de ayuda en el tema (no existe una región específica de apertura, y la neurogénesis se produce a lo largo de toda la vida, en mayor o menor cantidad), recurrí a la psicología. La producción creativa y la apertura a los nuevos inventos de otros está distorsionda por un factor: no se puede predecir el declive por la edad de la persona, sino por cuánto tiempo haya trabajado en una determinada disciplina. (...) No se trata de edad cronológica, sino de edad "disciplinaria": los eruditos que cambian de disciplina parecen rejuvenecer su apertura mental ante lo novedoso.

One possibility is that many of these universes are unstable and decay to our familiar universe. We recall that the vacuum, instead of being a boring, featureless thing, is actually teeming with bubble universes popping in and out of existence, like in a bubble bath. Hawking called this the space-time foam. Most of these tiny bubble universes are unstable, jumping out of the vacuum and then jumping back in. In the same way, once the final formulation of the theory is found, one might be able to show that most of these alternate universes are unstable and decay down to our universe. For example, the natural time scale for these bubble universes is the Planck time, which is 10−43 seconds, an incredibly short amount of time. Most universes only live for this brief instant. Yet the age of our universe, by comparison, is 13.8 billion years, which is astronomically longer than the lifespan of most universes in this formulation. In other words, perhaps our universe is special among the infinity of universes in the landscape. Ours has outlasted them all, and that is why we are here today to discuss this question. But what do we do if the final equation turns out to be so complex that it cannot be solved by hand? Then it seems impossible to show that our universe is special among the universes in the landscape. At that point I think we should put it in a computer. This is the path taken for the quark theory. We recall that the Yang-Mills particle acts like a glue to bind quarks into a proton. But after fifty years, no one has been able to rigorously prove this mathematically. In fact, many physicists have pretty much given up hope of ever accomplishing it. Instead, the Yang-Mills equations are solved on a computer. This is done by approximating space-time as a series of lattice points. Normally, we think of space-time being a smooth surface, with an infinite number of points. When objects move, they pass through this infinite sequence. But we can approximate this smooth surface with a grid or lattice, like a mesh. As we let the spacing between lattice points get smaller and smaller, it becomes ordinary space-time, and the final theory begins to emerge. Similarly, once we have the final equation for M-theory, we can put it on a lattice and do the computation on a computer. In this scenario, our universe emerges from the output of a supercomputer. (However, I am reminded of the Hitchhiker’s Guide to the Galaxy, when a gigantic supercomputer is built to find the meaning of life. After eons doing the calculation, the computer finally concluded that the meaning of the universe was “forty-two.”)

Of course, physics prevents us from dividing things beyond a certain limit, determined by what is called the Planck constant. This is because, according to physicists, it is actually impossible to measure a distance smaller than 10-34m without creating a black hole that would swallow up the measuring device.

The habit to get out of is the one (1) that goes, "I know what I'm doing, and every distraction is a bad thing that takes me further from my goals." Instead, if you get into the habit of accepting sometimes that distractions can be a path to your manifestations, then that's more neural matter your higher mind has access to, so it can give you it. In a word, it's called having 'grace.' But what it really is, is creating more bridges to your higher mind, increasing your blueshift while minimizing the pushback from the redshift.

After he won his prize, he was invited to lecture everywhere, and he had this chauffeur who drove him around to give public lectures all through Germany. And the chauffeur memorized the lecture, and so one day he said, "Gee, Professor Planck, why don't you let me try it by switching places?" And so he got up and gave the lecture. At the end of it. Some physicist stood up and posed a question of extreme difficulty. But the chauffeur was up to it. "Well," he said, "I'm surprised that a citizen of an advanced city like Munich is asking so elementary a question. So I'm going to ask my chauffeur to respond.

Expressed in Planck units, the temperature T of a black hole is inversely proportional to its mass, m. This is a third law, Hawking's law: T = k/m. The constant k is very small in normal units. As a result, astrophysical black holes have temperatures of a very small fractionnof a degree.

physicist Max Planck once observed, “A new scientific truth does not triumph by convincing its opponents and making them see the light, but rather because its opponents eventually die.

As physicist Max Planck once observed, “A new scientific truth does not triumph by convincing its opponents and making them see the light, but rather because its opponents eventually die.

The work of Max Planck, Albert Einstein, Niels Bohr and others showed that light appeared to be both a wave and a stream of particles. Although it was convenient for many purposes to think of light as behaving like a wave, the particle idea explained more phenomena. As the great American physicist Richard Feynman would later put it: ‘It is very important to know that light behaves like particles, especially for those of you who have gone to school, where you were probably told about light behaving like waves. I’m telling you the way it does behave – like particles.

Emerging Possibilities for Space Propulsion Breakthroughs Originally published in the Interstellar Propulsion Society Newsletter, Vol. I, No. 1, July 1, 1995.  Marc. G. Millis, Space Propulsion Technology Division, NASA Lewis Research Center Cleveland, Ohio “New perspectives on the connection between gravity and electromagnetism have just emerged. A theory published in February 1994 (ref 11) suggests that inertia is nothing but an electromagnetic illusion. This theory builds on an earlier work (ref 12) that asserts that gravity is nothing other than an electromagnetic side-effect. Both of these works rely on the perspective that all matter is fundamentally made up of electrically charged particles, and they rely on the existence of Zero Point Energy. Zero Point Energy (ZPE) is the term used to describe the random electromagnetic oscillations that are left in a vacuum after all other energy has been removed (ref 13). This can be explained in terms of quantum theory, where there exists energy even in the absolute lowest state of a harmonic oscillator. The lowest state of an electromagnetic oscillation is equal to one-half the Planck constant times the frequency. If all the energy for all the possible frequencies is summed up, the result is an enormous energy density, ranging from 1036 to 1070 Joules/m3. In simplistic terms there is enough energy in a cubic centimeter of the empty vacuum to boil away Earth's oceans. First predicted in 1948, ZPE has been linked to a number of experimental observations. Examples include the Casimir effect (ref 14), Van der Waal forces (ref 15), the Lamb-Retherford Shift (ref 10, p. 427), explanations of the Planck blackbody radiation spectrum (ref 16), the stability of the ground state of the hydrogen atom from radiative collapse (ref 17), and the effect of cavities to inhibit or enhance the spontaneous emission from excited atoms (ref 18). Regarding the inertia and gravity theories mentioned earlier, they take the perspective that all matter is fundamentally constructed of electrically charged particles and that these particles are constantly interacting with this ZPE background. From this perspective the property of inertia, the resistance to change of a particle's velocity, is described as a high- frequency electromagnetic drag against the Zero Point Fluctuations. Gravity, the attraction between masses, is described as Van der Waals forces between oscillating dipoles, where these dipoles are the charged particles that have been set into oscillation by the ZPE background. It should be noted that these theories were not written in the context of propulsion and do not yet provide direct clues for how to electromagnetically manipulate inertia or gravity. Also, these theories are still too new to have either been confirmed or discounted. Despite these uncertainties, typical of any fledgling theory, these theories do provide new approaches to search for breakthrough propulsion physics.

The Marquis de Forestelle's monocle was minute and rimless, and, by enforcing an incessant and painful contraction of the eye over which it was incrusted like a superfluous cartilage, the presence of which there was inexplicable and its substance unimaginable, it gave to his face a melancholy refinement, and led women to suppose him capable of suffering terribly when in love. But that of M. de Saint-Candé, girdled, like Saturn, with an enormous ring, was the centre of gravity of a face which composed itself afresh every moment in relation to the glass, while his thrusting red nose and swollen sarcastic lips endeavoured by their grimaces to rise to the level of the steady flame of wit that sparkled in the polished disk, and saw itself preferred to the most ravishing eyes in the world by the smart, depraved young women whom it set dreaming of artificial charms and a refinement of sensual bliss; and then, behind him, M. de Planck, who with his huge carp's head and goggling eyes moved slowly up and down the stream of festive gatherings, unlocking his great mandibles at every moment as though in search of his orientation, had the air of carrying about upon his person only an accidental and perhaps purely symbolical fragment of the glass wall of his aquarium, a part intended to suggest the whole which recalled to Swann, a fervent admirer of Giotto's Vices and Virtues at Padua, that Injustice by whose side a leafy bough evokes the idea of the forests that enshroud his secret lair.