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November 3, 2006 at 12:59 am #536073
SeanzaParticipantClick .
Not happy, why is it locked it was supposed to be fun, if you read a reply in that topic, 1 of the Mods CLEARLY explained the ability for a Mod to lock a topic should not be used for a non-business reason.
Therefore, anisina, you have been disqualified from the ‘Last post wins’ game. You made me do it, you made me!
AdSense 336x280November 3, 2006 at 12:59 am #601984
SeanzaParticipantClick .
Not happy, why is it locked it was supposed to be fun, if you read a reply in that topic, 1 of the Mods CLEARLY explained the ability for a Mod to lock a topic should not be used for a non-business reason.
Therefore, anisina, you have been disqualified from the ‘Last post wins’ game. You made me do it, you made me!
AdSense 336x280November 3, 2006 at 1:02 am #601986
anisinaParticipantIt called ‘Staff Fun’
AdSense 336x280November 3, 2006 at 1:07 am #601989
SeanzaParticipantNah it’s called cheating. Thought you would’ve known better anisina.
Am not angry, just disappointed.
AdSense 336x280November 3, 2006 at 1:14 am #601990
anisinaParticipantDon’t blame me, i’m only following a standard set by an higher person than myself.
and so feel duty bound to take part as the current climate is encouraging me in a way I cannot resist due to the forces of the zodiac. I have in no part signed or declared fully my intention to withold my right to use the powers that be to enable me to participate. I therefore reserve the right to participate.
I am part nuclear and part human, hence…
The discovery of the electron was the first indication that the atom had internal structure. At the turn of the 20th century the accepted model of the atom was J. J. Thomson’s "plum pudding" model in which the atom was a large positively charged ball with small negatively charged electrons embedded inside of it. By the turn of the century physicists had also discovered three types of radiation coming from atoms, which they named alpha, beta, and gamma radiation. Experiments in 1911 by Lise Meitner and Otto Hahn, and by James Chadwick in 1914 discovered that the beta decay spectrum was continuous rather than discrete. That is, electrons were ejected from the atom with a range of energies, rather than the discrete amounts of energies that were observed in gamma and alpha decays. This was a problem for nuclear physics at the time, because it indicated that energy was not conserved in these decays. The problem would later lead to the discovery of the neutrino (see below).
Around the same time that this was happening (1911) Ernest Rutherford performed a remarkable experiment in which Hans Geiger and Ernest Marsden under his supervision fired alpha particles (helium nuclei) at a thin film of gold foil. The plum pudding model predicted that the alpha particles should come out of the foil with their trajectories being at most slightly bent. He was shocked to discover that a few particles were scattered through large angles, even completely backwards in some cases. The discovery led to the Rutherford model of the atom, in which the atom has a very small, very dense nucleus consisting of heavy positively charged particles with embedded electrons in order to balance out the charge. As an example, in this model nitrogen-14 consisted of a nucleus with 14 protons and 7 electrons, and the nucleus was surrounded by 7 more orbiting electrons.
The Rutherford model worked quite well until studies of nuclear spin were carried out by Franco Rasetti at the California Institute of Technology in 1929. By 1925 it was known that protons and electrons had a spin of 1/2, and in the Rutherford model of nitrogen-14 the 14 protons and six of the electrons should have paired up to cancel each others spin, and the final electron should have left the nucleus with a spin of 1/2. Rasetti discovered, however, that nitrogen-14 has a spin of one.
In 1930 Wolfgang Pauli was unable to attend a meeting in Tübingen, and instead sent a famous letter with the classic introduction "Dear Radioactive Ladies and Gentlemen". In his letter Pauli suggested that perhaps there was a third particle in the nucleus which he named the "neutron". He suggested that it was very light (lighter than an electron), had no charge, and that it did not readily interact with matter (which is why it hadn’t yet been detected). This desperate way out solved both the problem of energy conservation and the spin of nitrogen-14, the first because Pauli’s "neutron" was carrying away the extra energy and the second because an extra "neutron" paired off with the electron in the nitrogen-14 nucleus giving it spin one. Pauli’s "neutron" was renamed the neutrino (Italian for little neutral one) by Enrico Fermi in 1931, and after about thirty years it was finally demonstrated that a neutrino really is emitted during beta decay.
In 1932 Chadwick realized that radiation that had been observed by Walther Bothe, Herbert Becker, Irène and Frédéric Joliot-Curie was actually due to a massive particle that he called the neutron. In the same year Dmitrij Iwanenko suggested that neutrons were in fact spin 1/2 particles and that the nucleus contained neutrons and that there were no electrons in it, and Francis Perrin suggested that neutrinos were not nuclear particles but were created during beta decay. To cap the year off, Fermi submitted a theory of the neutrino to Nature (which the editors rejected for being "too remote from reality"). Fermi continued working on his theory and published a paper in 1934 which placed the neutrino on solid theoretical footing. In the same year Hideki Yukawa proposed the first significant theory of the strong force to explain how the nucleus holds together.
With Fermi and Yukawa’s papers the modern model of the atom was complete. The center of the atom contains a tight ball of neutrons and protons, which is held together by the strong nuclear force. Unstable nuclei may undergo alpha decay, in which they emit an energetic helium nucleus, or beta decay, in which they eject an electron (or positron). After one of these decays the resultant nucleus may be left in an excited state, and in this case it decays to its ground state by emitting high energy photons (gamma decay).
The study of the strong and weak nuclear forces led physicists to collide nuclei and electrons at ever higher energies. This research became the science of particle physics, the crown jewel of which is the standard model of particle physics which unifies the strong, weak, and electromagnetic forces.
AdSense 336x280November 3, 2006 at 2:07 am #601991
The CutterParticipantWhile Boltzmann had sidestepped the issue of determinism in the debate on the recurrence paradox, maintaining a somewhat ambiguous "statistical" viewpoint, he had to face the issue more squarely in another debate that came to a head at almost the same time he faced the debate about the Poincare Recurrence Theorem. E. P. Culverwell in Dublin had raised, in 1890, what might be called the "reversibility objection to the H theorem," not to be confused with the "reversibility paradox" discussed by William Thomson, Loschmidt, and Boltzmann in the 1870s. Culverwell asked how the H-theorem could possibly be valid as long as it was based on the assumption that molecular motions and collisions are themselves reversible, and suggested that irreversibility might enter at the molecular level, perhaps as a result of interactions with the ether.
The ether was always available as a hypothetical source and sink for properties of matter and energy that didn’t quite fit into the framework of Newtonian physics, although some physicists were by this time quite suspicious of the tendency of their colleagues to resolve theoretical difficulties this way.
Culverwell’s objection was discussed at meetings of the British Association and in the columns of Nature during the next few years. It was S. H. Burbury in London who pointed out, in 1894, that the proof of the H-theorem depends on the Maxwell-Boltzmann assumption that colliding molecules are uncorrelated. While this would seem a plausible assumption to make before the collision, one might suppose that the collision itself introduces a correlation between the molecules that have just collided, so that the assumption would not be valid for later collisions. Burbury suggested that the assumption might be justified by invoking some kind of "disturbance from without [the system], coming at haphazard" [Burbury 1894, p. 78].
Boltzmann, who participated in the British discussions of the H theorem, accepted Burbury’s conclusion that an additional assumption was needed, and called it the hypothesis of "molecular disorder." He argued that it could be justified by assuming that the mean free path in a gas is large compared with the mean distance of two neighboring molecules, so that a given molecule would rarely encounter again a specific molecule with which it had collided, and thus become correlated (see Boltzmann 1896-1898, pp. 40-41).
"Molecular disorder" is not merely the hypothesis that states of individual molecules occur completely at random; rather it amounts to an exclusion of special ordered states of the gas that would lead to violations of the Second Law. In fact such ordered states would be generated by a random process, as Boltzmann noted in his discussion of the recurrence paradox.
In modern terminology, one makes a distinction between "random numbers" and "numbers generated by a random process" — in preparing a table of random numbers for use in statistical studies, one rejects certain subsets, for example pages on which the frequencies of digits depart too greatly from 10%, because they are inconveniently-nonrandom products of a random process.
Boltzmann recognized that the hypothesis of molecular disorder was needed to derive irreversibility, yet at the same time he admitted that the hypothesis itself may not always be valid in real gases, especially at high densities, and that recurrence may actually occur.
In view of Boltzmann’s partial abandonment of determinism on the molecular level, we must reconsider the view that 19th-century physicists always assumed determinism and used statistical methods only for convenience.
There is no doubt that some 19th-century thinkers did see determinism as the essence of science. Thus W. Stanley Jevons, a philosopher of science, wrote in 1877:
"We may safely accept as a satisfactory scientific hypothesis the doctrine so grandly put forth by Laplace, who asserted that a perfect knowledge of the universe, as it existed at any given moment, would give a perfect knowledge of what was to happen thenceforth and for ever after. Scientific inference is impossible, unless we may regard the present as the outcome of what is past, and the cause of what is to come. To the view of perfect intelligence nothing is uncertain." [Jevons 1877, pp. 738-39]
Hence, as Laplace himself had remarked in 1783 (see Gillispie 1972, p. 10), there is really no such thing as "chance" in nature, regarded as a cause of events; it is merely an expression of our own ignorance, and "probability belongs wholly to the mind" [Jevons 1877, p. 198].
But was this view really held by scientists themselves? By the time Jevons wrote the words quoted above, support for absolute determinism was already beginning to collapse. In arguing for some degree of continuity between the 19th and 20th centuries, I do not want to overstate the case; 20th-century events (including the discovery of radioactive decay, though it actually occurred just before 19OO) accounted for most of the impetus toward atomic randomness, while the 19th-century background accounted for a significantly smaller amount. Nevertheless the discussion of randomness and irreversibility in connection with kinetic theory and the Second Law of Thermodynamics was quite familiar to physicists in the early decades of the 20th century.
The claim that 19th-century kinetic theory was based on molecular determinism must rely heavily on the evidence of the writings of James Clerk Maxwell and Ludwig Boltzmann; though in the absence of any explicit statements one might legitimately infer that they tacitly accepted the view of their contemporaries. In fact as we have already seen in the case of Boltzmann, the situation is a little more complicated: the words were ambiguous but the equations pushed physical theory very definitely in the direction of indeterminism. As in other transformations of physical science — the cases of Kepler, Fresnel, Planck, and Heisenberg might be adduced here — mathematical calculation led to results that forced the acceptance of qualitatively different concepts.
Maxwell’s earliest work in kinetic theory, in particular his introduction of the velocity-distribution law, seems to derive from the tradition of general probability theory and social statistics (as developed by Adolphe Quetelet) rather than from the mechanistic analysis of molecular motions. Maxwell’s law asserts that each component of the velocity of each molecule is a random variable, which is statistically independent of every other component of the same and every other molecule. Only in his later papers did Maxwell attempt to justify the law by relating it to molecular collisions, and even then he needed to assume that the velocities of two colliding molecules are statistically independent. On the other hand, the computation of gas properties such as viscosity and thermal conductivity, whose comparison with experimental data provided the essential confirmation of the theory, did involve the precise dynamical analysis of collisions of particles with specified velocities, positions, and force laws. Without determinism in this part of the theory Maxwell could not have achieved his most striking successes in relating macroscopic properties to molecular parameters.
Maxwell did not consistently maintain the assumption of determinism at the molecular level, though he occasionally supported that position, for example, in his lecture on "Molecules" at the British Association meeting in 1873. Yet in the same year, in private discussions and correspondence, he began to repudiate determinism as a philosophical doctrine. A detailed exposition of his views may be found in a paper titled "Does the progress of physical science tend to give any advantage to the opinion of necessity (or Determinism) over that of the contingency of events and the Freedom of the Will?" presented to an informal group at Cambridge University. The answer was no — based on arguments such as the existence of singular points in the trajectory of dynamical systems, where an infinitesimal force can produce a finite effect. (These arguments have led some contemporary scientists to list Maxwell as one of the precursors of "chaos theory.") The conclusion was that "the promotion of natural knowledge may tend to remove that prejudice in favor of determinism which seems to arise from assuming that the physical science of the future is a mere magnified image of that of the past" [Campbell & Garnett 1882, p. 434].
By 1875 Maxwell was asserting that molecular motion is "perfectly irregular; that is to say, that the direction and magnitude of the velocity of a molecule at a given time cannot be expressed as depending on the present position of the molecule and the time" [Maxwell 1875a, p. 235]. He also stated that this irregularity must be present in order for the system to behave irreversibly [Maxwell 1875b].
Two decades later, as noted above, Boltzmann seemed to have reached a similar conclusion. But he was not quite satisfied that his hypothesis of molecular disorder resolved the reversibility and recurrence paradoxes; in response to further criticisms by Zermelo he proposed a new hypothesis. Suppose we consider the curve of H as a function of time for the entire universe, or for a part of the universe isolated from the rest. A high value of H will correspond to a low-entropy highly-ordered state, where life can exist. If the recurrence theorem is correct then such a state can be regarded as one of an infinite number of maxima of an oscillating curve. If we follow H forward in time from one of these peaks, it will decrease in accordance with the H theorem; but it must eventually increase again to get to the next peak. Such an epoch of increasing H (decreasing entropy) would seem to violate the Second Law. But, Boltzmann suggested, if the irreversible processes in our environment and in our own bodies are "running backwards" then our own sense of the direction of time must also be reversed. Thus for any conscious beings who exist during this epoch, H must decrease when measured with respect to the time-changes of those beings, so for them the Second Law still holds.
Although Boltzmann did not regard this proposal as any more than a speculative hypothesis, he justified it as follows:
"One has the choice of two kinds of pictures. One can assume that the entire universe finds itself at present in a vry improbable state. However, one may suppose that the eons during which this improbable state lasts, and the distance from here to Sirius, are minute compared to the age and size of the universe. There must then be in the universe, which is in thermal equilibrium as a whole and therefore dead, here and there relatively small regions of the size of our galaxy (which we call worlds), which during the relatively short time of eons deviate significantly from thermal equilibrium. Among these worlds the state probability increases as often as it decreases. For the universe as a whole the two directions of time are indistinguishable, just as in space there is no up or down. However, just as at a certain place on the Earth’s surface we can call "down" the direction toward the centre of the Earth, so a living being that finds itself in such a world at a certain period of time can define the time direction as going from less probable to more probable states (the former will be the "past" and the latter the "future") and by virtue of this definition he will find that this small region, isolated from the rest of the universe, is "initially" always in an improbable state. This viewpoint seems to me to be the only way in which one can understand the validity of the Second Law and the Heat Death of each individual world without invoking a unidirectional change of the entire universe from a definite initial state to a final state."
[Boltzmnn 1897, p. 242]Boltzmann’s hypothesis asserts that irreversibility — the statement that "entropy increases with time" is not a law of nature but a tautology: the direction of time is determined by the direction of entropy increase. (Curiously this idea had recently been advanced by Ernst Mach, the most famous critic of Boltzmann’s kinetic-atomic theories.) Alternatively it could be seen as foreshadowing Einstein’s idea that time is not absolute but is somehow relative to the observer.
[url url=http://www.math.umd.edu/~lvrmr/History/MolecularChaos.html]Molecular Chaos and Determinism
(1890 – 1894)[/url]I just had to.
Mr. C.
AdSense 336x280November 3, 2006 at 11:29 pm #602018
anisinaParticipantI like the feel Mr. C.
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