Quantum Theory and Bohr's Theory of the Hydrogen Atom

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Vocabulary flashcards covering quantum theory equations, photon energy calculations, atomic emission spectra, and Bohr's model of the hydrogen atom.

Last updated 11:58 PM on 9/16/26
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13 Terms

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Planck's Constant (hh)

A fundamental physical constant equal to 6.626×10−34 J⋅s6.626 \times 10^{-34}\,\text{J}\cdot\text{s} that relates the energy of a photon to its frequency (Ephoton=hνE_{\text{photon}} = h\nu).

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Speed of Light (cc)

A constant equal to 2.998×108 m/s2.998 \times 10^8\,\text{m/s}, related to wavelength and frequency by the formula c=λνc = \lambda\nu.

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Continuous Spectrum

A spectrum containing all wavelengths of visible light, such as the spectrum produced by white light.

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Atomic Emission Spectrum

A spectrum created when gas-phase atoms absorb energy and re-emit light at specific wavelengths, which are separated by a prism.

<p>A spectrum created when gas-phase atoms absorb energy and re-emit light at specific wavelengths, which are separated by a prism.</p>
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<p>Bright-Line Spectrum</p>

Bright-Line Spectrum

A series of discrete line wavelengths emitted by energized atoms of an element, unique to each individual element.

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Ground State

The lowest energy, most stable energy state of an atom, corresponding to n=1n = 1 in the hydrogen atom model.

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Excited State

Any energy state of an atom in which the principal quantum number n>1n > 1, possessing higher potential energy than the ground state.

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Bohr Hydrogen Energy Equation

An equation applying exclusively to hydrogen atoms, defined as En=−2.18×10−18 J(1n2)E_n = -2.18 \times 10^{-18}\,\text{J} \left(\frac{1}{n^2}\right), which calculates the energy of an electron in orbit nn.

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Quantized Energy Transition

The movement of an electron between specific, discrete energy levels in an atom, analogous to a ball moving up and down steps.

<p>The movement of an electron between specific, discrete energy levels in an atom, analogous to a ball moving up and down steps.</p>
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Change in Energy (ΔE\Delta E)

The difference in potential energy between the final and initial states of an atom, calculated as ΔE=Ef−Ei\Delta E = E_f - E_i.

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Photon Emission

The release of a photon when an electron drops from a higher to a lower energy level (ni>nfn_i > n_f), resulting in a negative energy change (ΔE<0\Delta E < 0) for the atom.

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Photon Absorption

The uptake of a photon when an electron moves from a lower to a higher energy level (nf>nin_f > n_i), resulting in a positive energy change (ΔE>0\Delta E > 0) for the atom.

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Steel

An alloy composed of iron and carbon, to which metals like vanadium can be added to increase overall strength.