# quantum

Ask AI3: What is quantum?

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## Sentences

The photochemical exchange occurs with a

**quantum**yield of the order of unity in the liquid phase at 65-degrees using light absorbed only by the Af.
In the gas phase, with Af of Af and Af of Af,

**quantum**yields of the order of Af have been observed at 85-degrees.
It was possible to make estimates of the

**quantum**yield by observing the extent of reduction of a uranyl oxalate actinometer solution illuminated for a known time in a typical reaction cell and making appropriate conversions based on the differences in the absorption spectra of uranyl oxalate and of chlorine, and considering the spectral distribution of the light source.
These estimates indicated that the

**quantum**yield for the exchange of chlorine with liquid carbon tetrachloride at 65-degrees is of the order of magnitude of unity.
The standard ampere is most accurately realized using a watt balance, but is in practice maintained via Ohm's Law from the units of electromotive force and resistance, the volt and the ohm, since the latter two can be tied to physical phenomena that are relatively easy to reproduce, the Josephson junction and the

**quantum**Hall effect, respectively.
Atomic orbitals are typically categorized by n, l, and m

**quantum**numbers, which correspond to the electron's energy, angular momentum, and an angular momentum vector component, respectively.
Each orbital is defined by a different set of

**quantum**numbers ( n, l, and m ), and contains a maximum of two electrons each with their own spin**quantum**number.
The simple names s orbital, p orbital, d orbital and f orbital refer to orbitals with angular momentum

**quantum**number l = 0, 1, 2 and 3 respectively.
With the development of

**quantum**mechanics, it was found that the orbiting electrons around a nucleus could not be fully described as particles, but needed to be explained by the wave-particle duality.
Specifically, in

**quantum**mechanics, the state of an atom, i. e. an eigenstate of the atomic Hamiltonian, is approximated by an expansion ( see configuration interaction expansion and basis set ) into linear combinations of anti-symmetrized products ( Slater determinants ) of one-electron functions.
In atomic physics, the atomic spectral lines correspond to transitions (

**quantum**leaps ) between**quantum**states of an atom.
These states are labeled by a set of

**quantum**numbers summarized in the term symbol and usually associated with particular electron configurations, i. e., by occupation schemes of atomic orbitals ( e. g., 1s < sup > 2 </ sup > 2s < sup > 2 </ sup > 2p < sup > 6 </ sup > for the ground state of neon -- term symbol: < sup > 1 </ sup > S < sub > 0 </ sub >).
functions as real combinations of spherical harmonics Y < sub > lm </ sub >( θ, φ ) ( where l and m are

**quantum**numbers ).
Explaining the behavior of these electron " orbits " was one of the driving forces behind the development of

**quantum**mechanics.
Still, the Bohr model's use of quantized angular momenta and therefore quantized energy levels was a significant step towards the understanding of electrons in atoms, and also a significant step towards the development of

**quantum**mechanics in suggesting that quantized restraints must account for all discontinuous energy levels and spectra in atoms.
In the end, this was solved by the discovery of modern

**quantum**mechanics and the Pauli Exclusion Principle.
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