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"In large
suns when hydrogen is exhausted and gravity contraction ensures, and
such a body is not sufficiently opaque to retain the internal
pressure of support for the outer gas regions, then a sudden
collapse occurs. The gravity-electric changes give origin to vast
quantities of tiny particles devoid of electric potential, and such
particles readily escape from the solar interior thus bringing about
the collapse of a gigantic sun within a few days." (p.464)
For the
mid-thirties that was quite a statement. These tiny particles that
we now call neutrinos were entirely speculative in the early 1930's
and were required to account for the missing mass-energy of beta
radioactive decay.
Hypotheses on
the possible origins of the Urantia Paper's statement on solar
collapse.
In the early
1930's, the idea that supernova explosions could occur and result in
the formation of neutron stars was extensively publicized by Fritz
Zwicky of the California Institute of Technology (Caltec) who worked
in Professor Millikan's Dept. For a period during the mid-thirties,
Zwicky was also at the University of Chicago. Dr. Sadler is said to
have known Millikan. So alternative possibilities for the origin of
The Urantia Book quote above could be:
-
The
revelators followed their mandate and used a human source of
information about supernovae, possibly Zwicky.
-
Dr Sadler had
learned about the tiny particles devoid of electric potential
from either Zwicky, Millikan, or some other knowledgeable person
and incorporated it into The Urantia Book.
-
It is
information supplied to fill missing gaps in otherwise earned
knowledge as permitted in the mandate. (1110)
Zwicky had the
reputation of being a brilliant scientist but given to much wild
speculation, some of which turned out to be correct. A paper
published by Zwicky and Baade in 1934 proposed that neutron stars
would be formed in stellar collapse and that 10% of the mass would
be lost in the process (Phys. Reviews. Vol. 45)
In "Black
Holes and Time Warps. Einstein's 'v Outrageous Legacy"
(Picador, London, 1994), a book that covers the work and thought of
this period in detail, K. S . Thorne, Feynman Professor of
Theoretical Physics at Caltec, writes: In the early 1930's, Fritz
Zwicky and Walter Baade joined forces to study novae, stars that
suddenly flare up and shine 10,000 times more brightly than before.
Baade was aware of tentative evidence that, besides ordinary novae,
there existed superluminous novae. These were roughly of the same
brightness but since they were thought to occur in nebulae far out
beyond our Milky Way, they must signal events of extraordinary
magnitude. Baade collected data on six such novae that had occurred
during the current century.
As Baade and
Zwicky struggled to understand supernovae, James Chadwick, in 1932,
reported the discovery of the neutron. This was just what Zwicky
required to calculate that if a star could be made to implode until
it reached the density of the atomic nucleus, it might transform
into a gas of neutrons, reduce its radius to a shrunken core, and,
in the process, lose about 10 % of its mass. The energy equivalent
of the mass loss would then supply the explosive force to power a
supernova.
Zwicky
believed cosmic rays accounted for the mass energy loss in supernova
explosions.
Information,
extracted from Thorne's recent book, indicates that Zwicky knew
nothing about the possible role of "little neutral
particles" in the implosion of a neutron star, but rather
that he attributed the entire mass-energy loss to cosmic rays. So,
if not from Zwicky, what then is the human origin of The Urantia
Book's statement that the neutrinos escaping from its interior bring
about the collapse of the imploding star? (Current estimates
attribute about 99% of the energy of a supernova explosion to being
carried off by the neutrinos).
In his book,
Thorne further states: astronomers in the 1930's responded
enthusiastically to the Baade-Zwicky concept of a supernova, but
treated Zwicky's neutron star and cosmic ray ideas with disdain...In
fact it is clear to me from a detailed study of Zwicky's writings of
the era that he did not understand the laws of physics well enough
to be able to substantiate his ideas." This opinion was also
held by Robert Oppenheimer who published a set of papers with
collaborators Volkoff, Snyder, and Tolman, on Russian physicist Lev
Landau's ideas about stellar energy originating from a neutron core
at the heart of a star.
Einstein and
Eddington opposed neutron star concept.
These Oppenheimer
papers concluding that either neutron stars or black holes could be
the outcome of massive star implosion were about as far as
physicists could go at that time.
However,
the most prominent physicist of the time, Albert Einstein, and the
doyen of astronomers, Sir Arthur Eddington, both vigorously opposed
the concepts involved in stellar collapse beyond the white dwarf
stage. Thus the subject appears to have been put on hold coincident
with the outbreak of war in 1939.
During
the 1940's, virtually all capable physicists were occupied with
tasks relating to the war effort. Apparently this was not so for
Russian-born astronomer-physicist, George Gamow, a professor at
Leningrad who had taken up a position at George Washington
University in 1934. Gamow conceived the beginning of the Hubble
expanding universe as a thermonuclear fireball in which the original
stuff of creation was a dense gas of protons, neutrons, electrons,
and gamma radiation which transmuted by a chain of nuclear reactions
into the variety of elements that make up the world of today.
Referring to this work, Overbye4 writes: "In the
forties, Gamow and a group of collaborators wrote a series of papers
spelling out the details of thermonucleogenesis. Unfortunately their
scheme didn't work. Some atomic nuclei were so unstable that they
fell apart before they could fuse again into something heavier, thus
breaking the element building chain. Gamow's team disbanded in the
late 40's, its work ignored and disdained." Among this work was
a paper by Gamow and Schoenfeld that proposed that energy loss from
aging stars would be mediated by an efflux of neutrinos. This
proposal appears to have been overlooked or ignored until the
1960's.
Conservation
of energy law under fire.
As time went by,
the need for the neutrino grew, firstly to save the law of
conservation of energy, but also laws of conservation of momentum,
angular momentum (spin), and lepton number. As knowledge of what it
ought to be like grew, plus the knowledge accruing from the intense
efforts to produce the atom bomb, possible means of detecting this
particle began to emerge. In 1953, experiments were begun by a team
led by C.L. Cowan and F. Reines.' Fission reactors were now in
existence in which the breakdown of uranium yielded free neutrons
that, outside of the atomic nucleus, were unstable and broke down
via beta decay to yield a proton, an electron, and, if it existed,
the missing particle.
Detection of
the elusive neutrino.
The Cowan and
Reines team devised an elaborate scheme to detect the antineutrinos
from a reactor. By 1956 their system was detecting 70 such events
per day, unequivocally ascribable to antineutrinos. It now remained
to prove that this particle was not its own antiparticle, as is the
case with the photon. This was done by R.R. Davis in 1956', using a
detection system designed specifically for what the properties of
the neutrino should be and testing it with an antineutrino source
from a fission reactor.
Renewal of the
search for the neutron star.
The subject of
the fate of imploding stars re- opened with vigor when both Robert
Oppenheimer and John Wheeler, two of the really great names of
physics, attended a conference in Brussels in 1958. Oppenheimer
believed that his 1939 papers said all that needed to be said about
such implosions. Wheeler disagreed, wanting to know what went on
beyond the well-established laws of physics.
When Oppenheimer
and Snyder did their work in 1939, it had been hopeless to compute
the details of the implosion. In the meantime, nuclear weapons
design had provided the necessary tools because, to design a bomb,
nuclear reactions, pressure effects, shock waves, heat, radiation,
and mass ejection had to be taken into account. Wheeler realized
that his team had only to rewrite their computer programs so as to
simulate implosion rather than explosion. However his hydrogen bomb
team had been disbanded and it fell to Stirling Colgate at
Livermore, in collaboration with Richard White and Michael May, to
do these simulations. Wheeler learned of the results and was largely
responsible for generating the enthusiasm to follow this line of
research. The term 'black hole' was coined by Wheeler.
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