• Now I have lambdas associated with transitions between energy levels in atomic hydrogen.

    现在我把波长和,氢原子中的,能级跃迁联系起来。

    麻省理工公开课 - 固态化学导论课程节选

  • So, what we know is happening is that were having transitions from some excited states to a more relaxed lower, more stable state in the hydrogen atom.

    我们知道,这里所发生的是,氢原子从激发态到更低更稳定的态的跃迁,而我们用眼睛可以探测到的。

    麻省理工公开课 - 化学原理课程节选

  • Gee, I wonder if I could come up with a set of transitions occurring inside atomic hydrogen Just right match that what Angstrom measured back in 1853.

    嘿!我想知道我是否可以想出,发生在氢原子内的,一系列的跃迁,正好符合,阿姆斯特朗在1853年测得的东西。

    麻省理工公开课 - 固态化学导论课程节选

  • So this means that we can go directly from the energy between two levels to the frequency of the photon that's emitted when you go between those levels.

    这意味着我们可以直接,从两个能级的能量得到它们之间,跃迁发射出光子的频率。

    麻省理工公开课 - 化学原理课程节选

  • And what we predict as an energy difference between two levels, we know should correspond to the energy of light that's either emitted, if we're giving off a photon, or that's absorbed if we're going to take on a photon and jump from a lower to a higher energy level.

    我们预测,两个能级之间的能量差,我们知道,它要么和发出的光有关,如果它发出光子的话,要么它吸收光子,从低能级跃迁到,更高能级上去。

    麻省理工公开课 - 化学原理课程节选

  • We saw a similar thing as we saw electrons move from different levels.

    这与我们曾经见过的,不同能级之间的跃迁很类似。

    麻省理工公开课 - 化学原理课程节选

  • We're getting further away from the nucleus because we're jumping, for example, from the n equals 2 to the n equals 3 shell, or from the n equals 3 to the n equals 4 shell.

    我们将会离原子核越来越远,因为我们在跃迁,比如从,n,等于,2,的壳层到n等于,3,的壳层,或者从,n,等于,3,的壳层到n等于,4,的壳层。

    麻省理工公开课 - 化学原理课程节选

  • p So to jump from the 2 s to the 2 p, takes more energy than we can actually compensate with by increasing the pull from the nucleus.

    也就是,从,2,s,跃迁到,消耗的能量超过了,由于原子核的引力增强而补偿的能量。

    麻省理工公开课 - 化学原理课程节选

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