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15:5215:52, 18 March 2026 LNF: Evaluation of the impact of fast particles on refuelling with cryogenic pellets in stellarator reactors (PaRaPel) (hist | edit) [6,094 bytes] Belenlmiranda (talk | contribs) (Created page with "== LNF - Nationally funded project == '''Title''': '''Evaluation of the impact of fast particles on refuelling with cryogenic pellets in stellarator reactors (PaRaPel)''' '''Reference''': PID2024-162966OA-I00 '''Programme and date''': Proyectos de Generación de Conocimiento 2024 '''Programme type (Modalidad de proyecto)''': Proyectos Generación de Conocimiento - Investigación orientada '''Area/subarea (Área temática / subárea)''': Clima, Energía y Movilidad...")

22:4622:46, 9 February 2026 GENE (hist | edit) [10,660 bytes] Hasan Ghotme (talk | contribs) (Created page with "'''GENE''' ('''Gyrokinetic Electromagnetic Numerical Experiment''') is an open-source computer simulation code used to study plasma turbulence in magnetic confinement fusion devices. GENE solves the gyrokinetic equations to simulate electromagnetic turbulence in plasmas, which is critical for understanding energy confinement in fusion reactors like tokamaks and stellarators. ==Overview== GENE is a gyrokinetic turbulence code that simulates plasma behavior at very small...")
11:5311:53, 9 February 2026 Piecewise Omnigeneity (hist | edit) [250 bytes] Jlvelasco (talk | contribs) (Created page with "Piecewise omnigenity is a property of the magnetic field such that the mean radial collisionless guiding center magnetic drift is zero. It consists on the property of omnigenity being fulfilled piecewisely on the flux surface of the stellarator.")

22:3122:31, 27 January 2026 Neutronics in Fusion (hist | edit) [14,803 bytes] Hasan Ghotme (talk | contribs) (Created page with "= Nuclear Fusion Reactions = == Deuterium–Tritium (D–T) == <math>^2\mathrm{H} + ^3\mathrm{H} \longrightarrow ^4\mathrm{He} + n</math> Q = 17.6 MeV * Alpha particle: 3.5 MeV * Neutron: 14.1 MeV == Deuterium–Deuterium (D–D) == <math>^2\mathrm{H} + ^2\mathrm{H} \longrightarrow ^3\mathrm{He} + n</math> Q = 3.27 MeV <math>^2\mathrm{H} + ^2\mathrm{H} \longrightarrow ^3\mathrm{H} + p</math> Q = 4.03 MeV == Deuterium–Helium‑3 (D–³He) == <math>^2\math...")

09:3109:31, 16 January 2026 Tokamak and Stellarator Comparison (hist | edit) [7,374 bytes] Hasan Ghotme (talk | contribs) (Created page with "== Comparison of Tokamaks and Stellarators == The following table presents a comparative overview of tokamak and stellarator <ref name="Xu2016" />. The comparison highlights key physical properties, transport characteristics, stability behavior, and reactor-relevant challenges of both concepts. The aim is to provide a simplified and coherent picture of the main technical and physical challenges faced by each configuration, and to show how far current experiments...")

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