The Mass-5 Roadblock质量-5路障
![]() ![]() In order for us to exist, we had to have a star, the Sun, which is overwhelmingly composed of hydrogen and helium. But after the deuterons formed and subsequently formed helium nuclei (alpha particles), the "clumping" process to make more massive nuclei stopped. Why? Because there is no stable nucleus of mass 5. The energies involved are illustrated in the diagram above. The -2.2 MeV of energy associated with deuterium shows that it has a negative binding energy and is thus stable. But this is 2.2 MeV out of a total mass energy of about 1876 MeV for the deuteron, so it is a relatively thin margin of stability, and became stable only when the expanding universe cooled to near 109K. The deuterium in the early universe combined quickly to form helium which can be seen to be exceptionally stable. But the mass-5 nuclei are highly unstable, so no other nuclei formed except trace quantities of 7Li and 7Be. The formation of heavier elements had to await the operation of the nuclear fusion furnaces in the center of stars. 为了存在,我们不得不有一个恒星,即太阳,它主要由氢和氦组成。但当氘核形成并随后形成氦核(α粒子)后,形成更重核的“聚变合并”过程停止了。为什么?因为质量为5的核没有稳定的。涉及的能量如上图所示。氘核所关联的-2.2 MeV能量表明它具有负结合能,因此是稳定的。但这个能量是氘核总质量能约1876 MeV中的2.2 MeV,因此稳定性相对较弱,只有当宇宙膨胀并冷却到接近10⁹ K时,才变得稳定。早期宇宙中的氘核迅速结合形成氦,可以明显看出氦的稳定性很高。但质量为5的核高度不稳定,因此除了少量的7Li和7Be外,没有其他核形成。更重元素的形成必须等待恒星中心的核融合炉运行。
![]() The deuteron is stable because in experiencing the strong nuclear force between the neutron and proton, there is a mass reduction associated with the nuclear binding energy which makes the deuteron's mass smaller than the sum of the neutron and proton mass. It is then "uphill" in energy by 2.2 MeV for it to separate back into a proton and neutron. 氘核是稳定的,因为在中子和质子之间体验到强核力时,存在与核结合能相关的质量减少,使得氘核的质量小于中子和质子质量之和。它要重新分离成质子和中子则需要额外的2.2 MeV能量。
Once the deuterons are formed, they have a very strong tendency to combine into helium nuclei . The helium nucleus (alpha particle) is very tightly bound and the rapid process of combining deuterons into helium nuclei gives us the cosmic abundance of hydrogen and helium we have today. But with the helium nuclei a new factor comes into play - the balance between the repulsive electromagnetic force and the attractive nuclear strong force. This intense conflict between the two strongest forces determines the stability of all nuclei more massive than deuterium. In the case of the helium nucleus, the strong force is dominant and it forms a very stable nucleus. 一旦氘核形成,它们就有很强的倾向结合成氦核。氦核(α粒子)非常紧密地结合在一起,氘核迅速结合成氦核的过程使我们今天观察到的氢和氦的宇宙丰度成为可能。但当氦核形成时,一个新的因素开始起作用——电磁斥力与核强力之间的平衡。这两种最强力之间的激烈冲突决定了所有比氘核更重的核的稳定性。在氦核的情况下,强力占主导地位,形成了非常稳定的核。
But the next step brings a surprise. Adding a neutron to make helium-5 does not yield a stable nucleus. Adding a proton makes lithium-5 which is likewise unstable. Adding a deuteron to make lithium-6 might work, but it is less stable than the helium nucleus and its probability is extremely low. So the process of heavy element building is effectively roadblocked at some three minutes into the age of the universe! It is not until the universe has expanded and cooled sufficiently to allow atoms to form, and those atoms in sufficient concentrations to colllapse to form stars and kindle the fires of nuclear fusion, is the progression of heavy element building resumed. 但下一步却带来了意外。向氦-5中添加一个中子并不会形成稳定的原子核。添加一个质子会形成锂-5,同样不稳定。向锂-6中添加一个氘核可能有效,但其稳定性不如氦核,且概率极低。因此,重元素的合成过程在宇宙年龄约三分钟时几乎停滞!只有当宇宙膨胀并冷却到足以允许原子形成,且这些原子浓度足够高以坍缩形成恒星并点燃核聚变时,重元素的合成过程才得以恢复。
Consider the scenario where the strong nuclear force was relatively stronger compared to the electromagnetic force. Then the clumping into ever more massive nuclei would have continued and the universe would have been made of heavy elements instead of hydrogen and helium. Then there would have been no stars, and no "us". 考虑一个场景,其中强核力相对于电磁力更强。那么,原子核会不断聚合成更重的原子核,宇宙将由重元素而非氢和氦组成。届时将不会有恒星,也不会有‘我们’。
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