全部书籍

专业

应用 关于 Coach 登录 开始阅读

书籍暂未推出简体中文版——当前显示英文版。

Physics · 术语表

什么是 The Coulomb barrier?

又称: Coulomb barrier · plasma

Definition 33.18 High School Physics · 第 33 章 — Nuclear Energy: Fission, Fusion, E=mc2

Two nuclei are both positive: to touch, they must first climb the hill of their electric repulsion (Chapter 14) — the Coulomb barrier. Only near 1×108 K1 \times 10^{8}\,\mathrm{K} do collisions carry the energy to cross it; the fuel is then a plasma of bare nuclei and electrons. Fission pays no such toll: its trigger, the neutron, is neutral, and works cold.

示例

Example 33.19 (The Sun runs on it)

The Sun’s core, at 1.5×107 K1.5 \times 10^{7}\,\mathrm{K}, fuses ordinary hydrogen step by step — the proton–proton chain, of net effect 4 11H→24He+2 +10e+radiation4\,{}^{1}_{1}\mathrm{H} \to {}^{4}_{2}\mathrm{He} + 2\,{}^{0}_{+1}\mathrm{e} + \text{radiation}, about 26 MeV26\,\mathrm{MeV} per helium: 0.7%0.7\% of the hydrogen’s mass leaves as energy. The sunlight whose spectrum we read in Chapter 2 is this mass, arriving eight minutes late; every star shines by walking the curve toward iron.

在原文中阅读 →