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  • https://en.wikipedia.org/wiki/Tricastin_Nuclear_Power_Plant
    Tricastin Nuclear Power Plant
    The Tricastin Nuclear Power Plant (French: Centrale Nucléaire du Tricastin) is a nuclear power plant consisting of 4 pressurized water reactors (PWRs) of CP1 type with 915 MW electrical power output each. The power plant is located in the south of France (Drôme and Vaucluse Department) at the Canal de Donzère-Mondragon near the Donzère-Mondragon Dam and the commune Pierrelatte. The power plant is part of the widespread Tricastin Nuclear Site (see below), which was named after the historic Tricastin region. Three out of the four reactors on the site had been used until 2012 to power the Eurodif Uranium enrichment plant, which had been located on the site. Tricastin Nuclear Site The Tricastin Nuclear Site (Site Nucléaire du Tricastin) is a collection of facilities run by Areva and EDF located on right bank of the Channel of Donzère-Mondragon (diversion canal of the Rhône River) south of the city of Valence (70 km upstream) and north of Avignon (65 km downstream). The site straddles the border between the departments Drôme (26) and Vaucluse (84), not far from the...
    EN.WIKIPEDIA.ORG
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  • https://www.indiatoday.in/programme/short-video/challenges-and-consequences-of-targeting-irans-nuclear-facilities-india-today-2611563-2024-10-04
    Challenges and Consequences of Targeting Iran's Nuclear Facilities | India Today
    Recent discussions have revolved around the targeting of Iran's nuclear facilities in light of missile attacks. These nuclear facilities, scattered across the vast expanse of the country, pose as substantial targets. The feasibility of such actions, however, have been put into question due its inherent challenges. Equally important is the analysis of the numerous hurdles and obstacles associated with such actions, as contemplated by experts.
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  • https://www.indiatoday.in/programme/first-up/video/us-against-israel-over-reported-plan-to-strike-irans-nuclear-facilities-2610442-2024-10-03
    US against Israel over reported plan to strike Iran's nuclear facilities
    US President Joe Biden expressed opposition to Israel's reported plan to strike Iran's nuclear facilities in retaliation for Tehran's missile attacks on the Jewish nation.
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  • https://en.wikipedia.org/wiki/Nuclear_fusion#Thermonuclear_fusion
    Nuclear fusion
    Nuclear fusion is a reaction in which two or more atomic nuclei are combined to form one or more different atomic nuclei and subatomic particles (neutrons or protons). The difference in mass between the reactants and products is manifested as either the release or absorption of energy. This difference in mass arises due to the difference in nuclear binding energy between the atomic nuclei before and after the reaction. Nuclear fusion is the process that powers active or main-sequence stars and other high-magnitude stars, where large amounts of energy are released. A nuclear fusion process that produces atomic nuclei lighter than iron-56 or nickel-62 will generally release energy. These elements have a relatively small mass and a relatively large binding energy per nucleon. Fusion of nuclei lighter than these releases energy (an exothermic process), while the fusion of heavier nuclei results in energy retained by the product nucleons, and the resulting reaction is endothermic...
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  • https://ui.adsabs.harvard.edu/abs/2002ApJ...576..323R
    Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics
    We present the first calculations to follow the evolution of all stable nuclei and their radioactive progenitors in stellar models computed from the onset of central hydrogen burning through explosion as Type II supernovae. Calculations are performed for Population I stars of 15, 19, 20, 21, and 25 Msolar using the most recently available experimental and theoretical nuclear data, revised opacity tables, neutrino losses, and weak interaction rates and taking into account mass loss due to stellar winds. A novel ``adaptive'' reaction network is employed with a variable number of nuclei (adjusted each time step) ranging from ~700 on the main sequence to >~2200 during the explosion. The network includes, at any given time, all relevant isotopes from hydrogen through polonium (Z=84). Even the limited grid of stellar masses studied suggests that overall good agreement can be achieved with the solar abundances of nuclei between 16O and 90Zr. Interesting discrepancies are seen in the 20 Msolar model and (so far, only in that model) are a consequence of the merging of the oxygen, neon, and carbon shells about a day prior to core collapse. We find that, in some stars, most of the ``p-process'' nuclei can be produced in the convective oxygen-burning shell moments prior to collapse; in others, they are made only in the explosion. Serious deficiencies still exist in all cases for the p-process isotopes of Ru and Mo.
    UI.ADSABS.HARVARD.EDU
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  • https://arxiv.org/abs/astro-ph/0112478
    Nucleosynthesis in Massive Stars With Improved Nuclear and Stellar Physics
    We present the first calculations to follow the evolution of all stable nuclei and their radioactive progenitors in stellar models computed from the onset of central hydrogen burning through explosion as Type II supernovae. Calculations are performed for Pop I stars of 15, 19, 20, 21, and 25 M_sun using the most recently available experimental and theoretical nuclear data, revised opacity tables, neutrino losses, and weak interaction rates, and taking into account mass loss due to stellar winds. A novel ``adaptive'' reaction network is employed with a variable number of nuclei (adjusted each time step) ranging from about 700 on the main sequence to more than 2200 during the explosion. The network includes, at any given time, all relevant isotopes from hydrogen through polonium (Z=84). Even the limited grid of stellar masses studied suggests that overall good agreement can be achieved with the solar abundances of nuclei between 16O and 90Zr. Interesting discrepancies are seen in the 20 M_sun model and, so far, only in that model, that are a consequence of the merging of the oxygen, neon, and carbon shells about a day prior to core collapse. We find that, in some stars, most of the ``p-process'' nuclei can be produced in the convective oxygen burning shell moments prior to collapse; in others, they are made only in the explosion. Serious deficiencies still exist in all cases for the p-process isotopes of Ru and Mo.
    ARXIV.ORG
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  • https://en.wikipedia.org/wiki/Nuclear_physics
    Nuclear physics
    Nuclear physics is the field of physics that studies atomic nuclei and their constituents and interactions, in addition to the study of other forms of nuclear matter. Nuclear physics should not be confused with atomic physics, which studies the atom as a whole, including its electrons. Discoveries in nuclear physics have led to applications in many fields such as nuclear power, nuclear weapons, nuclear medicine and magnetic resonance imaging, industrial and agricultural isotopes, ion implantation in materials engineering, and radiocarbon dating in geology and archaeology. Such applications are studied in the field of nuclear engineering. Particle physics evolved out of nuclear physics and the two fields are typically taught in close association. Nuclear astrophysics, the application of nuclear physics to astrophysics, is crucial in explaining the inner workings of stars and the origin of the chemical elements. History The history of nuclear physics as a discipline distinct from atomic physics, starts with the discovery of radioactivity by Henri Becquerel in 1896, made while investigating phosphorescence in uranium...
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  • https://en.wikipedia.org/wiki/Nuclear_transmutation
    Nuclear transmutation
    Nuclear transmutation is the conversion of one chemical element or an isotope into another chemical element. Nuclear transmutation occurs in any process where the number of protons or neutrons in the nucleus of an atom is changed. A transmutation can be achieved either by nuclear reactions (in which an outside particle reacts with a nucleus) or by radioactive decay, where no outside cause is needed. Natural transmutation by stellar nucleosynthesis in the past created most of the heavier chemical elements in the known existing universe, and continues to take place to this day, creating the vast majority of the most common elements in the universe, including helium, oxygen and carbon. Most stars carry out transmutation through fusion reactions involving hydrogen and helium, while much larger stars are also capable of fusing heavier elements up to iron late in their evolution. Elements heavier than iron, such as gold or lead, are created through elemental transmutations that can naturally occur in supernovae. One goal of alchemy, the transmutation of base substances into gold, is now known to be impossible by chemical means but possible by physical means...
    EN.WIKIPEDIA.ORG
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  • https://ui.adsabs.harvard.edu/abs/2021bnpp.book.....B
    The Basics of Nuclear and Particle Physics
    This undergraduate textbook breaks down the basics of Nuclear Structure and modern Particle Physics. Based on a comprehensive set of course notes, it covers all the introductory material and latest research developments required by third- and fourth-year physics students. The textbook is divided into two parts. Part I deals with Nuclear Structure, while Part II delves into Particle Physics. Each section contains the most recent science in the field, including experimental data and research on the properties of the top quark and Higgs boson. Detailed mathematical derivations are provided where necessary to helps students grasp the physics at a deeper level. Many of these have been conveniently placed in the Appendices and can be omitted if desired. Each chapter ends with a brief summary and includes a number of practice problems, the answers to which are also provided.
    UI.ADSABS.HARVARD.EDU
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  • https://arxiv.org/abs/0808.3156
    Perturbation of Nuclear Decay Rates During the Solar Flare of 13 December 2006
    Recently, Jenkins, et al. have reported the detection of correlations between fluctuations in nuclear decay rates and Earth-Sun distance, which suggest that nuclear decay rates can be affected by solar activity. In this paper, we report the detection of a significant decrease in the decay of 54Mn during the solar flare of 13 December 2006, whose x-rays were first recorded at 02:37 UT (21:37 EST on 12 December). Our detector was a 1 uCi sample of 54Mn, whose decay rate exhibited a dip coincident in time with spikes in both the x-ray and proton fluxes recorded by the GOES-10 and 11 satellites. A secondary peak in the x-ray and proton fluxes on 17 December at 12:40 EST was also accompanied by a coincident dip in the 54Mn decay rate. These observations support the claim by Jenkins, et al. that nuclear decay rates vary with Earth-Sun distance.
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  • Nuclear energy is a form of energy that is generated by the splitting or fusing of atoms. This type of energy has been used for many purposes, including electricity generation, medical applications, and military applications. Nuclear energy can be generated in several different ways, including through nuclear fission and nuclear fusion. Nuclear fission involves splitting an atom's nucleus into two or more smaller nuclei, while nuclear fusion involves combining two or more nuclei to form a larger nucleus. Both processes release large amounts of energy in the form of heat and radiation.

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  • power

    Nuclear power is the use of nuclear reactions that release energy to generate heat, which most frequently is then used in steam turbines to produce electricity in a nuclear power plant. As of 2020, 14 countries worldwide are operating nuclear power plants, with a total of about 450 reactors. Nuclear power is controversial due to its environmental and safety concerns. Proponents of nuclear power argue that it is a reliable and relatively clean source of energy, while opponents contend that it poses numerous threats to people and the environment.

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  • elements are matrix elements of nuclear operators between nuclear states. These matrix elements are important for calculations of nuclear properties, such as nuclear decay rates and transition probabilities. They are also used in the study of nuclear structure and in the description of nuclear reactions. Nuclear matrix elements can be calculated using a variety of theoretical methods, including shell model, Hartree-Fock, and density functional theory.

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  • Nuclear fusion is the process by which two or more atomic nuclei join together to form a single, heavier nucleus. It is the process that powers the sun and other stars. It occurs when two nuclei, typically of hydrogen, collide at very high speeds and fuse together to form a heavier nucleus such as helium. This fusion releases a tremendous amount of energy in the form of heat and light.

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  • Russia warns of "real" nuclear war risk
    Russian Foreign Minister Sergei Lavrov said the threat of a nuclear conflict and the outbreak of World War III is "real" amid the war ...
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  • Russia Ukraine WAR LIVE: Russia Ukraine War day 65 LIVE Updates | China Taiwan News | Nuclear War
    Russia Ukraine WAR LIVE: Russia Ukraine War day 65 LIVE Updates | Putin vs Joe Biden | Nuclear War ...
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  • Russia says Ukraine war could go nuclear if West keeps sending weapons
    Ukraine's government called the latest dire warning from Moscow a sign that Putin's regime "senses defeat" as the fighting, and ...
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  • Dr. John Mullen
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