![]() ![]() Nuclear Fusion: Inside the Breakthrough That Could Change Our World.(1 min)Ī concise explanation of the December 2022 advancement in inertial confinement fusion energy generation. The Fusion Breakthrough, Explained in 60 Seconds.(8 pages)Ī current overview of the state of fusion energy research, the investment landscape, and the near-term R&D benchmarks necessary to ascertain the viability of using fusion energy to decarbonize power systems. Will Fusion Energy Help Decarbonize the Power System?.(6 min)Īn easy-to-understand introduction to the thermonuclear process and approaches involved in building a fusion reactor. Fusion Power Explained – Future or Failure.Introduces fusion energy generation concepts and ways scientists are attempting to achieve fusion energy. Include selections from the Optional and Useful list based on your interests and available time. We strongly encourage you to review the Essential videos and readings before watching our lecture on Fusion Energy. We assign videos and readings to our Stanford students as pre-work for each lecture to help contextualize the lecture content. * The Coulomb barrier is the amount of energy needed to overcome the electrostatic forces between nuclei so they can get close enough to fuse. Currently, fusion is in the research phase and is not currently commercially viable, though billions of dollars from both the public and private sectors are being invested in the fusion space. The most commonly used fuels for nuclear fusion are deuterium and tritium (isotopes of hydrogen), which combine to form helium. However, while nuclear fusion happens continuously in (and even powers) the sun, making nuclear fusion happen on earth is extremely challenging (think about putting the sun in a box). Nuclear fusion has the potential to be an extremely energy dense and carbon-free energy resource that does not produce air pollution or radioactive waste. The energy of the neutrons can then be captured (usually by converting to heat) and used to generate electricity. Nuclear fusion occurs when nuclei from two or more atoms are forced together (overcoming the Coulomb barrier*) and fuse to form a single larger nucleus, releasing lots of energy (by E = mc 2), usually in the form of fast moving neutrons. Tools to Manage and Sustain Energy Systemsįusion reactions power the sun and the stars.The Grid: Electricity Transmission, Industry, and Markets.Drilling, Completing, and Producing from Oil and Natural Gas Wells.
0 Comments
Leave a Reply. |
AuthorWrite something about yourself. No need to be fancy, just an overview. ArchivesCategories |