“Ground state”的意思、由来-开放百科全书

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Ground state

释义

Ground state has no nodes in one-dimension
Examples
Notes
Bibliography

{{For|articles related to the ground state|Quantum vacuum (disambiguation)}}

The ground state of a quantum-mechanical system is its lowest-energy state; the energy of the ground state is known as the zero-point energy of the system. An excited state is any state with energy greater than the ground state. In the quantum field theory, the ground state is usually called the vacuum state or the vacuum.

If more than one ground state exists, they are said to be degenerate. Many systems have degenerate ground states. Degeneracy occurs whenever there exists a unitary operator that acts non-trivially on a ground state and commutes with the Hamiltonian of the system.

According to the third law of thermodynamics, a system at absolute zero temperature exists in its ground state; thus, its entropy is determined by the degeneracy of the ground state. Many systems, such as a perfect crystal lattice, have a unique ground state and therefore have zero entropy at absolute zero. It is also possible for the highest excited state to have absolute zero temperature for systems that exhibit negative temperature.

Ground state has no nodes in one-dimension

In one dimension, the ground state of the Schrödinger equation can be proven to have no nodes.^[1]

Consider the average energy of a state with a node at {{mvar|x}} = 0; i.e., {{math|ψ(0)}} = 0. The average energy in this state would be

where {{math|V(x)}} is the potential.

Now, consider a small interval around ; i.e., . Take a new (deformed) wave function {{math|ψ{{'}}(x)}} to be defined as , for ; and , for ; and constant for . If is small enough, this is always possible to do, so that {{math|ψ{{'}}(x)}} is continuous.

Assuming around , one may write

where is the norm.

Note that the kinetic-energy density everywhere because of the normalization. More significantly, the average kinetic energy is lowered by by the deformation to {{math|ψ{{'}}}}.

Now, consider the potential energy. For definiteness, let us choose . Then it is clear that, outside the interval , the potential energy density is smaller for the {{math|ψ{{'}}}} because there.

On the other hand, in the interval we have

which holds to order .

However, the contribution to the potential energy from this region for the state {{math|ψ}} with a node is

lower, but still of the same lower order as for the deformed state {{math|ψ{{'}}}}, and subdominant to the lowering of the average kinetic energy.

Therefore, the potential energy is unchanged up to order , if we deform the state with a node into a state {{math|ψ{{'}}}} without a node, and the change can be ignored.

We can therefore remove all nodes and reduce the energy by , which implies that {{math|ψ{{'}}}} cannot be the ground state. Thus the ground-state wave function cannot have a node. This completes the proof. (The average energy may then be further lowered by eliminating undulations, to the variational absolute minimum.)

Examples

The wave function of the ground state of a particle in a one-dimensional box is a half-period sine wave, which goes to zero at the two edges of the well. The energy of the particle is given by , where h is the Planck constant, m is the mass of the particle, n is the energy state (n = 1 corresponds to the ground-state energy), and L is the width of the well.
The wave function of the ground state of a hydrogen atom is a spherically symmetric distribution centred on the nucleus, which is largest at the center and reduces exponentially at larger distances. The electron is most likely to be found at a distance from the nucleus equal to the Bohr radius. This function is known as the 1s atomic orbital. For hydrogen (H), an electron in the ground state has energy {{val|-13.6|u=eV}}, relative to the ionization threshold. In other words, 13.6 eV is the energy input required for the electron to no longer be bound to the atom.
The exact definition of one second of time since 1997 has been the duration of {{val|9,192,631,770}} periods of the radiation corresponding to the transition between the two hyperfine levels of the ground state of the caesium-133 atom at rest at a temperature of 0 K.^[2]

Notes

1. ^ See, for example, {{cite thesis |last= Cohen|first= M. |date=1956 |title=The energy spectrum of the excitations in liquid helium |type= Ph.D. |publisher=California Institute of Technology |url=http://thesis.library.caltech.edu/1007/1/Cohen_m_1956.pdf |chapter=Appendix A: Proof of non-degeneracy of the ground state}} Published as {{cite journal |doi=10.1103/PhysRev.102.1189 |title=Energy Spectrum of the Excitations in Liquid Helium |journal=Physical Review |volume=102 |issue=5 |pages=1189 |year=1956 |last1=Feynman |first1=R. P. |last2=Cohen |first2=Michael |bibcode=1956PhRv..102.1189F}}
2. ^{{cite web |title=Unit of time (second) |work=SI Brochure |url=http://www.bipm.org/en/si/si_brochure/chapter2/2-1/second.html |publisher=International Bureau of Weights and Measures |accessdate=2013-12-22}}

Bibliography

{{cite book|title=The Feynman Lectures on Physics|volume=3| first1=Richard |last1=Feynman|author1-link=Richard Feynman|first2=Robert |last2=Leighton|first3=Matthew|last3= Sands|year=1965|chapter=see section 2-5 for energy levels, 19 for the hydrogen atom|url=http://www.feynmanlectures.caltech.edu/III_toc.html}}

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