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Screening also significantly increases the probability of interaction between hot fuel and lattice nuclei increasing the likelilhood of Oppenheimer-Phillips processes opening a potential route to reaction multiplication. The effect of screening for enhancement of the total nuclear reaction rate is a function of multiple parameters including fuel temperature and the relative scattering probability between the fuel and lattice metal nuclei. Aspects of screening effects to enable calculation of nuclear reaction rates are also evaluated, including Coulomb scattering and localized heating of the cold fuel, primary D-D reactions, and subsequent reactions with both the fuel and the lattice nuclei. This probability is incorporated into the astrophysical factor S(E). Electron screening also significantly increases the probability of large vs small angle Coulomb scattering of the reacting nuclei to enable subsequent nuclear reactions via tunneling. It is well known that screening increases the probability of tunneling through the Coulomb barrier. We show that neutrons are far more efficient than energetic charged particles, such as light particles (e−,e+) or heavy particles (p,d,α) in transferring kinetic energy to fuel nuclei (D) to initiate fusion processes. Such an environment provides for enhanced screening of the Coulomb barrier due to conduction and shell electrons of the metal lattice, or by plasma induced by ionizing radiation (γ quanta). Nuclear fusion reactions of D-D are examined in an environment comprised of high density cold fuel embedded in metal lattices in which a small fuel portion is activated by hot neutrons. The data support the theoretical analysis in a companion paper, predicting fusion reactions and subsequent reactions in the highly screened environment. Neutron spectroscopy was conducted using calibrated lead-shielded liquid (EJ-309) and plastic (stilbene) scintillator detectors. Additionally, neutron energies of approximately 4 and 5 MeV for TiD2 and ErD3 were measured, consistent with either boosted neutrons from kinetically heated deuterons or Oppenheimer-Phillips stripping reactions in the highly screened environment. Exposure of deuterated materials (ErD3 and TiD2) to photon energies in the range of 2.5–2.9 MeV resulted in photodissociation neutrons that were below 400 keV and also the 2.45-MeV neutrons consistent with H2(d,n)He3 fusion.
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For more information, and details on how to receive longer term support for Oracle JDK 8, please see the Oracle Java SE Support Roadmap.D-D nuclear fusion events were observed in an electron-screened, deuterated metal lattice by reacting cold deuterons with hot deuterons (d*) produced by elastically scattered neutrons originating from bremsstrahlung photodissociation (where “d” and “D” denote H2). Customers who need continued access to critical bug fixes and security fixes as well as general maintenance for Java SE 8 or previous versions can get long term support through Oracle Java SE Subscription or Oracle Java SE Desktop Subscription. Oracle will not post further updates of Java SE 8 to its public download sites for commercial use after January 2019. Per Oracle’s website, they posted the following:
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I need to know this information ASAP just in case my company has to go out and purchase a license agreement from Oracle.
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We also using Oracle’s JDK 8 Update 192 JRE to keep ColdFusion JVM current with the latest java release.ĭue to Oracle posting the following information on their website (see below), we would like to know what is Adobe going to do in reference to the licensing issue.
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Currently we are utilizing ColdFusion 11 with the latest patch installed.