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SCIENCE · INVESTIGATE AND EXPLAIN

Match photon energy, transition direction and preparation

Connect wavelength to energy units and separate energy compatibility from allowed transitions and population.

Learning outcome: Convert photon wavelength/frequency/energy, balance absorption/emission signs and explain why a matching gap does not establish intensity.

Starting recap

A photon carries positive energy E=hν=hc/λ. Matter gains that energy in absorption and loses it in emission; frequency is inversely proportional to vacuum wavelength.

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Try

A photon with 4 eV is not automatically suitable for a selected 2.5 eV bound-level transition simply because it has more energy.

Open the experiment

Predict

Predict which wavelength matches the selected gap, whether reversal changes the photon energy, and whether a matching energy guarantees an observable transition.

Experiment

Repair the initial electronic mismatch using the 495.936794 nm option, reverse the transition, then match the vibrational and rotational packets. Keep the rotational photon while changing the supplied transition condition; inspect the unpopulated emission case. Capture the independent checks and explain the differences.

Match photon energy to a selected transition

Stipulated level packets · exact SI constant conversions · Original simplified rotational/vibrational/electronic level gaps, not measured species spectra. One-photon selected transitions; initial population and allowed/forbidden condition supplied, not derived. Exact SI defining constants; wavelength labels rounded but calculations retain full stored values. No line width, intensity, rate, ionization or population-equilibrium calculation.

Reset keeps your prediction, captures and practice history.

Convert wavelength before judging the selected transition

Proposed vacuum wavelength: 619.9209922 nm = 6.1992099e-7 m. Frequency ν=c/λ = 4.8359785e+14 Hz; photon energy E=hν = 3.2043533e-19 J = 2 eV = 192.970664 kJ per mole of these photons. This offered wavelength lies in the visible region.

electronic packet: energy axis in eV · scale changes between level families0Level 02.5Level 15Level 2Filled marker: initial level is supplied as populated.Arrow shows the proposed matter transition, not proof that it occurs. Level 2 is contextual.

The selected matter change is 2.5 eV. In absorption, radiation changes by -2 eV for the proposed photon. Their signed sum is 0.5 eV. Photon energy itself is positive in both absorption and emission; the matter/radiation changes have opposite signs.

CheckResultWhat it establishes
Photon matches selected gapDoes not matchOne-photon energy balance for this pair of levels
Supplied transition conditionAllowedPacket assumption, not derived from an actual molecule here
Selected initial populationPresentSupplied preparation, not a calculated thermal population

The selected proposal fails at least one condition. Matching energy alone does not calculate intensity, transition probability or rate. A higher-energy photon is not automatically suitable for this particular bound-level gap; other transitions and ionization are not tested here.

For the same gap, reversing absorption into emission preserves photon frequency and wavelength while reversing the matter change. The smaller rotational and vibrational gaps illustrate microwave and infrared associations; the electronic packet illustrates a visible transition. These examples are not exhaustive wavelength boundaries or unique species signatures.

Constants, precision and scope

Exact SI defining values: h=6.62607015e-34 J s; c=299792458 m/s; elementary charge magnitude e=1.602176634e-19 C, so 1 eV has that numerical value in joules; Nₐ=6.02214076e+23 mol⁻¹. Divide J by e to get eV, and multiply J per photon by Nₐ/1000 to get kJ/mol photons.

Options are stored as full-precision wavelengths derived from stipulated photon energies; labels are rounded. The 10⁻¹² relative matching tolerance only handles numerical roundoff. It is not a measured uncertainty, physical linewidth or permission for energy nonconservation. Packet levels are invented; allowed/forbidden flags are supplied rather than calculated quantum selection rules.

NIST exact SI defining constants

At least one selected-transition condition fails.

Energy match: no; supplied transition allowed: yes; initial level populated: yes. These are compatibility checks, not a predicted spectral intensity or unique identity.

Captures retain the stipulated level/preparation packet and proposed photon wavelength. Replay reconstructs unit conversions and independent compatibility checks; it does not measure a spectrum or predict intensity.

Understand

More photon energy is not automatically the right energy

The first packet selects a hypothetical electronic absorption from 0 to 2.5 eV. The initial photon option carries 2.0 eV and does not balance that transition. Try a shorter wavelength, then compare the 4.0 eV option. More energy does not automatically match this particular bound-level difference.

The packets are original simplified level schemes, not measured spectra of named substances. Other transitions and ionization could exist in a real species; this activity checks only the selected pair. It does not claim that a rejected photon cannot interact in any other way.

Convert units in a traceable chain

For vacuum wavelength λ, frequency ν and photon energy E:

ν=c/λ; E=hν=hc/λ.

Use wavelength in metres, frequency in Hz and h in J s to obtain energy in joules. One nm is 10⁻⁹ m. A frequency in Hz means cycles per second. For the offered wavelength near 495.936794 nm, the energy is 2.5 eV, approximately 4.00544×10⁻¹⁹ J per photon and 241.213 kJ per mole of those photons.

One electronvolt is 1.602176634×10⁻¹⁹ J. It is an energy unit, not a charge or voltage. To convert energy per photon to energy per mole of photons, multiply by the Avogadro constant and divide by 1000 for kJ. Do not mix a single-photon value with a molar value in the same energy ledger.

The options are stored at full precision and their wavelength labels are rounded. The matching tolerance only handles floating-point roundoff; it is not a physical linewidth or measurement uncertainty. Exact numerical constants do not turn the invented level gaps into measured reference data.

Reverse the direction without changing the photon’s energy

Select electronic emission with the upper level populated. For the same 2.5 eV gap, the emitted photon has the same positive energy, frequency and wavelength. Matter changes by −2.5 eV while radiation gains +2.5 eV. In absorption, matter gains +2.5 eV while radiation loses −2.5 eV.

The signed sum must be zero for the selected exchange. The arrow in the diagram follows matter’s proposed change; it does not assert that the transition occurs. The marked initial population and supplied transition condition are checked separately.

Compare rotational, vibrational and electronic gaps

Match the 0.2 eV vibrational packet with the wavelength near 6199.20992 nm, in the infrared. Match the 0.0001 eV rotational packet near 12,398,419.8 nm, or about 12.4 mm, in the microwave region. The 2.5 eV electronic example lies in the visible region; ultraviolet/visible radiation is commonly associated with electronic transitions.

Smaller gaps require lower frequencies and longer wavelengths. The diagram rescales the vertical energy axis between these families and prints the numerical eV labels; equal drawn heights do not mean equal physical energy gaps. The examples illustrate associations, not a rule that every species absorbs all radiation in a named region or that one wavelength uniquely identifies a molecule.

Energy balance is necessary, not a rate prediction

Keep the rotational wavelength selected and switch to the packet whose transition is supplied as forbidden. Energy still matches, but the independent transition condition fails. The activity does not derive a molecule’s quantum selection rules; the flag is part of the stated hypothetical evidence.

Now select the electronic emission proposal whose upper level is unpopulated. A matching photon and an allowed transition still do not supply an emitting particle in that level. Population is a preparation assumption here, not a calculated thermal distribution.

Even when all three checks pass, no line intensity, transition rate or probability is calculated. Capture a matched case and a case that fails only the transition or population condition, then explain which additional evidence would be required to predict an observed spectrum.

Connections and sources

The existing reference-line spectrum comparison addresses pattern matching, not these unit conversions or transition conditions. This lesson adds that mechanism-level reasoning without claiming empirical transition assignment, a full spectroscopy course or independently assessed experimental work.

Apply

A new selected transition changes matter energy by −3.0 eV. If it emits one photon, what must be true?

Public practice checks a specific claim. It does not establish independent mastery.

Use units and signed energy accounting to distinguish per-photon energy from per-mole energy. Explain spectral-region associations and what missing transition/population/rate information prevents you from concluding.

Continue

Completion requires a saved prediction, at least one capture and a reflection. Presence checks do not grade your reasoning.

Skipping retains experiments and awards no mastery.

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