Questions Regarding Energy Generating Fusion

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SUMMARY

The discussion centers on the energy requirements and variables influencing nuclear fusion, particularly focusing on hydrogen isotopes. The temperature necessary to initiate fusion is contingent on the atomic numbers of the nuclei involved, with lower temperatures required for hydrogen isotopes. Key concepts include the reaction rate (RR), which is influenced by ion densities and the microscopic cross-section (<σv>), a function of temperature and species. Magnetic confinement is employed to maintain plasma pressure, with magnetic pressure being proportional to the square of the magnetic field strength.

PREREQUISITES
  • Understanding of nuclear fusion principles
  • Familiarity with atomic structure and isotopes
  • Knowledge of reaction rates in plasma physics
  • Basic comprehension of magnetic confinement techniques
NEXT STEPS
  • Study the equations governing nuclear fusion, particularly those involving reaction rates
  • Explore the concept of microscopic cross-section in fusion reactions
  • Research magnetic confinement methods and their applications in plasma physics
  • Investigate online courses or resources on the mathematics of cold fusion
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Students and professionals in nuclear physics, plasma physicists, and researchers interested in the principles and applications of nuclear fusion technology.

Denyven
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Hi All,
I was wondering about some equations/formulae related to Fusion. How much energy/what temperature does it take to initiate Fusion? And how is this amount of energy affected by the different element/isotopes used, pressure, magnetic attraction and other variables?

Thanks in advanced.
 
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Denyven said:
Hi All,
I was wondering about some equations/formulae related to Fusion. How much energy/what temperature does it take to initiate Fusion? And how is this amount of energy affected by the different element/isotopes used, pressure, magnetic attraction and other variables?

Thanks in advanced.
You're asking for a basic course in fusion. The temperature required for fusion depends on the atomic numbers of the nuclei used in the process, the lowest temperatures being for hydrogen isotopes.

One also needs to understand the concept of microscopic cross-section, which is dependent of the species reacting.

The reaction rate (RR) is proportional to n1n2 or n2/2, where n1 and n2 are the ion densities of reacting species 1 and 2 (e.g., d+t), n where there is one ion species (e.g. d+d).

RR = n1n2<σv>, where <σv> is more or less the integrated probability of reaction. <σv> is a complicated function of temperature and species.

There is no magnetic attraction involved. Magnetic confinement is used to 'confine' the plasma as well as maintaining pressure on the plasma. Magnetic pressure is proportional to the square of the magetic field strength.

Look at the bottom of this page
https://wiki.engr.illinois.edu/display/npre421/NPRE+421+Plasma+and+Fusion+Science+-+Spring+2009
Particularly Chapter 2.
https://wiki.engr.illinois.edu/download/attachments/19302090/Chapter+02.pdf
 
Is there online a basic course in the math behind cold fusion? Or the equations describing a deuteron impacting a deuteron trapped in a metal lattice?

Astronuc said:
You're asking for a basic course in fusion.
 

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