How dipole concentration and charge separation disrupt atomic processes. Part one
the discovery of the Oklo natural nuclear reactor This post will explore the subject of naturally-occurring nuclear fission reactions, focusing on the reactors of Gabon, Africa, which were operational approximately two billion years ago. This post will emphasize the implication of the reactors' operation on the possible variance of the fine-structure constant (α) over time. Background In 1972, a researcher analyzing uranium from the Oklo deposit in Gabon, Africa discovered that the samples contained a U-235 content of only 0.717 percent, significantly less than the 0.720 percent typical of modern uranium ore. Further, researchers found that at least one portion of the Oklo deposit was depleted, with approximately 200 kg of U-235 missing. In addition, the depleted region of the deposit was found to be rich in nuclear fission products. This suggested that the uranium deposit had undergone a self-sustaining fission reaction that consumed the missing U-235 and generated fission products. The idea of a naturally-occurring fission reaction had been postulated in 1953 by Wetherwill and Inghram and further studied in 1956 by Kuroda. As discussed elsewhere, the Gabon sites (16 in total, between the Oklo mine and the neighboring Okelobondo uranium mine) satisfied the conditions (e.g., appropriate size, presence of a moderator, and absence of neutron poisons) that had been proposed for natural fission reactors. One criterion is particularly of note - while a modern, natural uranium deposit could not become a reactor due to its decreased U-235 content (0.720 percent), at the time that the Gabon reactors were operational, natural uranium contained approximately 3 percent U-235. This higher concentration enabled the self-sustaining fission reactors; in fact, it is comparable to the level of U-235 enrichment of the uranium fuel used in most modern nuclear power stations. Interpreting Xenon Isotopes Meshik and co-workers studied (via mass spectrometry) the isotopic composition of xenon from Oklo rock, in order to probe the nature of the Gabon reactors. The researchers initially made two surprising discoveries. First, they observed that the xenon was not largely located in uranium-rich mineral grains as they had anticipated but instead was found in aluminum phosphate minerals. Second, they observed that the isotopic distribution differed from that of modern nuclear reactors. Of the nine stable isotopes of xenon, the material from Oklo was depleted in Xe-136 and Xe-134. [2] Meshik and co-workers recognized that none of the xenon isotopes were produced directly by the fission of uranium itself but, instead, were formed by the decay of other fission products (specifically, radioactive iodine and tellurium). Thus, they recognized that the formation of the various xenon isotopes would be dependent upon the lifespans of their precursors. This would result in Xe-136 forming within one minute of the initiation of the self-sustained fission reaction, with Xe-134 forming after one hour, with Xe-132 and Xe-131 forming within days, and with Xe-129 only forming after millions of years. These key insights led Meshik and co-workers to propose that the Gabon reactors likely operated through a series of "on/off" cycles. Essential to this conclusion was the proposal (by Meshik and others) that the reactors were moderated by water. In the presence of water, neutrons are slowed to thermal energies, and a fission chain reaction can occur. However, the heat generated by the reaction would eventually boil the water away, halting fission until groundwater returned. This cycle explains the xenon isotope distribution: when the reactor was operating, the rapidly-formed Xe-134 and Xe-136 gases were driven off, but the precursors that would ultimately yield Xe-132, Xe-131, and Xe-129 were incorporated into aluminum phosphate minerals as the reactor cooled, during an "off" cycle. This explains the absence of Xe-134 and Xe-136 from these aluminum phosphate minerals. Moreover, this dependence on a water moderator could also explain the absence of xenon from the uranium-rich mineral grains: the water would have washed away the water-soluble tellurium and iodine isotopes that would have led to xenon. >From the Xe-131 / Xe-134 and Xe-132 / Xe-134 ratios of the aluminum phosphate from the Oklo site, Meshik and co-workers calculated the operating schedule for the Oklo reactors. Their calculations indicated a 30-minute "on" period of fission (with concomitant boiling of the water moderator) followed by a 2-hour, 30-minute "off" cooling period before water returned and the reactor again became self-sustaining. The Time Variation of the Fine-Structure Constant α The fine-structure constant (α) is a fundamental physical constant which affects a multitude of physical phenomena. Its relation to other physical values and its approximate value are as follows: α ≈ 1/137 As Barrow and Webb note, the precise value of this constant has a significant impact on physical events: the value affects the density of solid matter, the temperatures of chemical bond dissociations, and the stability of nuclei. If the value of α were to become greater than 0.1, nuclear fusion would be impossible. Furthermore, a shift of just four percent in the value of α would yield a change in the energy levels of carbon nuclei so dramatic that its production in stars would not occur. Given that α has such in importance to fundamental physical processes, there has been significant interest in studying how the value of α may have changed over time. With nuclear processes having such a strong dependence on even minute variations in α, the Gabon reactors play an important role in determining the degree to which α may have changed over a very long period of time. In 1976, Shlyakhter recognized that the operation of the Oklo reactors was dependent upon the ability of Sm-149 to undergo neutron capture. He also he recognized that, in order for this process to have occurred at Oklo, it was necessary for a value of a particular resonant energy level of the Oklo Sm-149 to be very similar to its present value. This resonant energy level is dependent upon α and, thus, is sensitive to changes in α. From the isotopic composition of samples from Oklo, the capture cross-section value (at the time that the reactors were operational), as well as the possible range of its variation, could be determined. From this, the upper boundaries for the range of variation in the resonance energy level and, therefore, in α, could be determined. Shlyakhter thus determined that the rate of change of α (specifically, [rate of change of α]/[α]) must be < 10-17 / year. In 2004, Lamoreaux and Torgerson analyzed the Oklo reactor data and its implications on the time variation of α. A key aspect of their analysis was the recognition that the uranium present in the Oklo reactor could act as a 1/v neutron absorber, a factor which alters the neutron energy spectrum of the reactor. Taking this into account, Lamoreaux and Torgerson calculated that the value of α has decreased over the past two billion years. Specifically, they calculated the |[rate of change of α]/[α]| to be < 3.8 x 10-17 / year (95% confidence). In 2006, Petrov and co-workers published a comprehensive analysis in which a complete computer model of one of the Oklo reactors (RZ2) was constructed. Using this model, the researchers determined the averaged cross section for Sm-149, which was then used to determine the limits on the variation of α. Petrov and co-workers determined these limits to be -3.7 x 10-17 / year < [rate of change of α]/[α] < 3.1 x 10 -17 / year. Thus, their analysis indicates that a distinct increase or decrease in α over the past two billion years is not a certainty. Conclusions Petrov and co-workers commented that "the discovery of the Oklo natural nuclear reactor in Gabon (West Africa) in 1972 was possibly one of the most momentous events in reactor physics since 1942, when Enrico Fermi and his team achieved an artificial self-sustained fission chain reaction." As discussed herein, the implications of this event have been significant and far-reaching. The discovery, geological distribution, and isotopic pattern of fission products (namely, xenon) led to significant insight into the operation of the Gabon reactors, which may find additional utility should evidence of other natural reactors be found in the future. The very fact that the reactors were operational at all has stimulated discussion regarding the time variation of a fundamental physical constant, leading to comprehensive analyses of the reactor data in an effort to answer this important question. Given the manifold consequences of these natural fission reactors, the statement by Petrov and co-workers rings true, with the story of natural nuclear fission being one of special interest within the realm of nuclear physics. The take away, if the fine structure constant can be changed, the reaction rate and the stability of the nucleus could be effected. On Fri, May 31, 2013 at 12:11 AM, Axil Axil <janap...@gmail.com> wrote: > http://arxiv.org/pdf/1301.3923v1.pdf > > > > A sum rule for charged elementary particles > > > > This paper draws a connection between charge and the behavior of the > vacuum in a region. > > > > Charge and dipoles shapes the vacuum and also the speed that light travels > through it. > > > > Increase the charge in a vacuum and the speed of light slows. Other > fundamental constants also change. The fine structure constant is a > function of the volume of particle-antiparticle pairs. > > > > This paper is a must read for the vacuum energy folks. >
