Hydrogen atom

A hydrogen atom is an atom of the chemical element hydrogen. The electrically neutral hydrogen atom contains a single positively charged proton in the nucleus, and a single negatively charged electron bound to the nucleus by the Coulomb force. Atomic hydrogen constitutes about 75% of the baryonic mass of the universe.
In everyday life on Earth, isolated hydrogen atoms (called "atomic hydrogen") are extremely rare. Instead, a hydrogen atom tends to combine with other atoms in compounds, or with another hydrogen atom to form ordinary (diatomic) hydrogen gas, H2. "Atomic hydrogen" and "hydrogen atom" in ordinary English use have overlapping, yet distinct, meanings. For example, a water molecule contains two hydrogen atoms, but does not contain atomic hydrogen (which would refer to isolated hydrogen atoms).
Atomic spectroscopy shows that there is a discrete infinite set of states in which a hydrogen (or any) atom can exist, contrary to the predictions of classical physics. Attempts to develop a theoretical understanding of the states of the hydrogen atom have been important to the history of quantum mechanics, since all other atoms can be roughly understood by knowing in detail about this simplest atomic structure.
The most abundant isotope, protium (H), or light hydrogen, contains no neutrons and is simply a proton and an electron. Protium is stable and makes up 99.985% of naturally occurring hydrogen atoms.
Deuterium (H) contains one neutron and one proton in its nucleus. Deuterium is stable, makes up 0.0156% of naturally occurring hydrogen, and is used in industrial processes like nuclear reactors and Nuclear Magnetic Resonance.
Tritium (H) contains two neutrons and one proton in its nucleus and is not stable, decaying with a half-life of 12.32 years. Because of its short half-life, tritium does not exist in nature except in trace amounts.
Heavier isotopes of hydrogen are only created artificially in particle accelerators and have half-lives on the order of 10 seconds. They are unbound resonances located beyond the neutron drip line; this results in prompt emission of a neutron.
The formulas below are valid for all three isotopes of hydrogen, but slightly different values of the Rydberg constant (correction formula given below) must be used for each hydrogen isotope.
Lone neutral hydrogen atoms are rare under normal conditions. However, neutral hydrogen is common when it is covalently bound to another atom, and hydrogen atoms can also exist in cationic and anionic forms.
If a neutral hydrogen atom loses its electron, it becomes a cation. The resulting ion, which consists solely of a proton for the usual isotope, is written as "H" and sometimes called hydron. Free protons are common in the interstellar medium, and solar wind. In the context of aqueous solutions of classical Brønsted–Lowry acids, such as hydrochloric acid, it is actually hydronium, H3O, that is meant. Instead of a literal ionized single hydrogen atom being formed, the acid transfers the hydrogen to H2O, forming H3O.
If instead a hydrogen atom gains a second electron, it becomes an anion. The hydrogen anion is written as "H" and called hydride.
The hydrogen atom has special significance in quantum mechanics and quantum field theory as a simple two-body problem physical system which has yielded many simple analytical solutions in closed-form.
Experiments by Ernest Rutherford in 1909 showed the structure of the atom to be a dense, positive nucleus with a tenuous negative charge cloud around it. This immediately raised questions about how such a system could be stable. Classical electromagnetism had shown that any accelerating charge radiates energy, as shown by the Larmor formula. If the electron is assumed to orbit in a perfect circle and radiates energy continuously, the electron would rapidly spiral into the nucleus with a fall time of: t fall ≈ a 0 3 4 r 0 2 c ≈ 1.6 × 10 − 11 s , {\displaystyle t_{\text{fall}}\approx {\frac {a_{0}^{3}}{4r_{0}^{2}c}}\approx 1.6\times 10^{-11}{\text{ s}},} where a 0 {\displaystyle a_{0}} is the Bohr radius and r 0 {\displaystyle r_{0}} is the classical electron radius. If this were true, all atoms would instantly collapse. However, atoms seem to be stable. Furthermore, the spiral inward would release a smear of electromagnetic frequencies as the orbit got smaller. Instead, atoms were observed to emit only discrete frequencies of radiation. The resolution would lie in the development of quantum mechanics.
In 1913, Niels Bohr obtained the energy levels and spectral frequencies of the hydrogen atom after making a number of simple assumptions in order to correct the failed classical model. The assumptions included:
Bohr supposed that the electron's angular momentum is quantized with possible values: L = n ℏ {\displaystyle L=n\hbar } where n = 1 , 2 , 3 , … {\displaystyle n=1,2,3,\ldots } and ℏ {\displaystyle \hbar } is Planck constant over 2 π {\displaystyle 2\pi } . He also supposed that the centripetal force which keeps the electron in its orbit is provided by the Coulomb force, and that energy is conserved. Bohr derived the energy of each orbit of the hydrogen atom to be: E n = − m e e 4 2 ( 4 π ε 0 ) 2 ℏ 2 1 n 2 , {\displaystyle E_{n}=-{\frac {m_{e}e^{4}}{2(4\pi \varepsilon _{0})^{2}\hbar ^{2}}}{\frac {1}{n^{2}}},} where m e {\displaystyle m_{e}} is the electron mass, e {\displaystyle e} is the electron charge, ε 0 {\displaystyle \varepsilon _{0}} is the vacuum permittivity, and n {\displaystyle n} is the quantum number (now known as the principal quantum number). Bohr's predictions matched experiments measuring the hydrogen spectral series to the first order, giving more confidence to a theory that used quantized values.
For n = 1 {\displaystyle n=1} , the value m e e 4 2 ( 4 π ε 0 ) 2 ℏ 2 = m e e 4 8 h 2 ε 0 2 = 1 Ry = 13.605 693 122 994 ( 26 ) eV {\displaystyle {\frac {m_{e}e^{4}}{2(4\pi \varepsilon _{0})^{2}\hbar ^{2}}}={\frac {m_{\text{e}}e^{4}}{8h^{2}\varepsilon _{0}^{2}}}=1\,{\text{Ry}}=13.605\;693\;122\;994(26)\,{\text{eV}}} is called the Rydberg unit of energy. It is related to the Rydberg constant R ∞ {\displaystyle R_{\infty }} of atomic physics by 1 Ry ≡ h c R ∞ . {\displaystyle 1\,{\text{Ry}}\equiv hcR_{\infty }.}
The exact value of the Rydberg constant assumes that the nucleus is infinitely massive with respect to the electron. For hydrogen-1, hydrogen-2 (deuterium), and hydrogen-3 (tritium) which have finite mass, the constant must be slightly modified to use the reduced mass of the system, rather than simply the mass of the electron. This includes the kinetic energy of the nucleus in the problem, because the total (electron plus nuclear) kinetic energy is equivalent to the kinetic energy of the reduced mass moving with a velocity equal to the electron velocity relative to the nucleus. However, since the nucleus is much heavier than the electron, the electron mass and reduced mass are nearly the same. The Rydberg constant RM for a hydrogen atom (one electron), R is given by R M = R ∞ 1 + m e / M , {\displaystyle R_{M}={\frac {R_{\infty }}{1+m_{\text{e}}/M}},} where M {\displaystyle M} is the mass of the atomic nucleus. For hydrogen-1, the quantity m e / M , {\displaystyle m_{\text{e}}/M,} is about 1/1836 (i.e. the electron-to-proton mass ratio). For deuterium and tritium, the ratios are about 1/3670 and 1/5497 respectively. These figures, when added to 1 in the denominator, represent very small corrections in the value of R, and thus only small corrections to all energy levels in corresponding hydrogen isotopes.
There were still problems with Bohr's model:
Most of these shortcomings were resolved by Arnold Sommerfeld's modification of the Bohr model. Sommerfeld introduced two additional degrees of freedom, allowing an electron to move on an elliptical orbit characterized by its eccentricity and declination with respect to a chosen axis. This introduced two additional quantum numbers, which correspond to the orbital angular momentum and its projection on the chosen axis. Thus the correct multiplicity of states (except for the factor 2 accounting for the yet unknown electron spin) was found. Further, by applying special relativity to the elliptic orbits, Sommerfeld succeeded in deriving the correct expression for the fine structure of hydrogen spectra (which happens to be exactly the same as in the most elaborate Dirac theory). However, some observed phenomena, such as the anomalous Zeeman effect, remained unexplained. These issues were resolved with the full development of quantum mechanics and the Dirac equation. It is often alleged that the Schrödinger equation is superior to the Bohr–Sommerfeld theory in describing hydrogen atom. This is not the case, as most of the results of both approaches coincide or are very close (a remarkable exception is the problem of hydrogen atom in crossed electric and magnetic fields, which cannot be self-consistently solved in the framework of the Bohr–Sommerfeld theory), and in both theories the main shortcomings result from the absence of the electron spin. It was the complete failure of the Bohr–Sommerfeld theory to explain many-electron systems (such as helium atom or hydrogen molecule) which demonstrated its inadequacy in describing quantum phenomena.
The Schrödinger equation is the standard quantum-mechanics model; it allows one to calculate the stationary states and also the time evolution of quantum systems. Exact analytical answers are available for the nonrelativistic hydrogen atom. Before we go to present a formal account, here we give an elementary overview.
Given that the hydrogen atom contains a nucleus and an electron, quantum mechanics allows one to predict the probability of finding the electron at any given radial distance r {\displaystyle r} . It is given by the square of a mathematical function known as the "wavefunction", which is a solution of the Schrödinger equation. The lowest energy equilibrium state of the hydrogen atom is known as the ground state. The ground state wave function is known as the 1 s {\displaystyle 1\mathrm {s} } wavefunction. It is written as: ψ 1 s ( r ) = 1 π a 0 3 / 2 e − r / a 0 . {\displaystyle \psi _{1\mathrm {s} }(r)={\frac {1}{{\sqrt {\pi }}a_{0}^{3/2}}}\mathrm {e} ^{-r/a_{0}}.}
Here, a 0 {\displaystyle a_{0}} is the numerical value of the Bohr radius. The probability density of finding the electron at a distance r {\displaystyle r} in any radial direction is the squared value of the wavefunction: | ψ 1 s ( r ) | 2 = 1 π a 0 3 e − 2 r / a 0 . {\displaystyle |\psi _{1\mathrm {s} }(r)|^{2}={\frac {1}{\pi a_{0}^{3}}}\mathrm {e} ^{-2r/a_{0}}.}
The 1 s {\displaystyle 1\mathrm {s} } wavefunction is spherically symmetric, and the surface area of a shell at distance r {\displaystyle r} is 4 π r 2 {\displaystyle 4\pi r^{2}} , so the total probability P ( r ) d r {\displaystyle P(r)\,dr} of the electron being in a shell at a distance r {\displaystyle r} and thickness d r {\displaystyle dr} is P ( r ) d r = 4 π r 2 | ψ 1 s ( r ) | 2 d r . {\displaystyle P(r)\,\mathrm {d} r=4\pi r^{2}|\psi _{1\mathrm {s} }(r)|^{2}\,\mathrm {d} r.}
It turns out that this is a maximum at r = a 0 {\displaystyle r=a_{0}} . That is, the Bohr picture of an electron orbiting the nucleus at radius a 0 {\displaystyle a_{0}} corresponds to the most probable radius. Actually, there is a finite probability that the electron may be found at any place r {\displaystyle r} , with the probability indicated by the square of the wavefunction. Since the probability of finding the electron somewhere in the whole volume is unity, the integral of P ( r ) d r {\displaystyle P(r)\,\mathrm {d} r} is unity. Then we say that the wavefunction is properly normalized.
As discussed below, the ground state 1 s {\displaystyle 1\mathrm {s} } is also indicated by the quantum numbers ( n = 1 , ℓ = 0 , m = 0 ) {\displaystyle (n=1,\ell =0,m=0)} . The second lowest energy states, just above the ground state, are given by the quantum numbers ( 2 , 0 , 0 ) {\displaystyle (2,0,0)} , ( 2 , 1 , 0 ) {\displaystyle (2,1,0)} , and ( 2 , 1 , ± 1 ) {\displaystyle (2,1,\pm 1)} . These n = 2 {\displaystyle n=2} states all have the same energy and are known as the 2 s {\displaystyle 2\mathrm {s} } and 2 p {\displaystyle 2\mathrm {p} } states. There is one 2 s {\displaystyle 2\mathrm {s} } state: ψ 2 , 0 , 0 = 1 4 2 π a 0 3 / 2 ( 2 − r a 0 ) e − r / 2 a 0 , {\displaystyle \psi _{2,0,0}={\frac {1}{4{\sqrt {2\pi }}a_{0}^{3/2}}}\left(2-{\frac {r}{a_{0}}}\right)\mathrm {e} ^{-r/2a_{0}},} and there are three 2 p {\displaystyle 2\mathrm {p} } states: ψ 2 , 1 , 0 = 1 4 2 π a 0 3 / 2 r a 0 e − r / 2 a 0 cos ⁡ θ , {\displaystyle \psi _{2,1,0}={\frac {1}{4{\sqrt {2\pi }}a_{0}^{3/2}}}{\frac {r}{a_{0}}}\mathrm {e} ^{-r/2a_{0}}\cos \theta ,} ψ 2 , 1 , ± 1 = ∓ 1 8 π a 0 3 / 2 r a 0 e − r / 2 a 0 sin ⁡ θ e ± i φ . {\displaystyle \psi _{2,1,\pm 1}=\mp {\frac {1}{8{\sqrt {\pi }}a_{0}^{3/2}}}{\frac {r}{a_{0}}}\mathrm {e} ^{-r/2a_{0}}\sin \theta ~e^{\pm i\varphi }.}
An electron in the 2 s {\displaystyle 2\mathrm {s} } or 2 p {\displaystyle 2\mathrm {p} } state is most likely to be found in the second Bohr orbit with energy given by the Bohr formula.
The Hamiltonian of the hydrogen atom is the radial kinetic energy operator plus the Coulomb electrostatic potential energy between the positive proton and the negative electron. Using the time-independent Schrödinger equation, ignoring all spin-coupling interactions and using the reduced mass μ = m e M / ( m e + M ) {\displaystyle \mu =m_{e}M/(m_{e}+M)} , the equation is written as: ( − ℏ 2 2 μ ∇ 2 − e 2 4 π ε 0 r ) ψ ( r , θ , φ ) = E ψ ( r , θ , φ ) {\displaystyle \left(-{\frac {\hbar ^{2}}{2\mu }}\nabla ^{2}-{\frac {e^{2}}{4\pi \varepsilon _{0}r}}\right)\psi (r,\theta ,\varphi )=E\psi (r,\theta ,\varphi )}
Expanding the Laplacian in spherical coordinates: − ℏ 2 2 μ [ 1 r 2 ∂ ∂ r ( r 2 ∂ ψ ∂ r ) + 1 r 2 sin ⁡ θ ∂ ∂ θ ( sin ⁡ θ ∂ ψ ∂ θ ) + 1 r 2 sin 2 ⁡ θ ∂ 2 ψ ∂ φ 2 ] − e 2 4 π ε 0 r ψ = E ψ {\displaystyle -{\frac {\hbar ^{2}}{2\mu }}\left[{\frac {1}{r^{2}}}{\frac {\partial }{\partial r}}\left(r^{2}{\frac {\partial \psi }{\partial r}}\right)+{\frac {1}{r^{2}\sin \theta }}{\frac {\partial }{\partial \theta }}\left(\sin \theta {\frac {\partial \psi }{\partial \theta }}\right)+{\frac {1}{r^{2}\sin ^{2}\theta }}{\frac {\partial ^{2}\psi }{\partial \varphi ^{2}}}\right]-{\frac {e^{2}}{4\pi \varepsilon _{0}r}}\psi =E\psi }
This is a separable, partial differential equation which can be solved in terms of special functions. When the wavefunction is separated as product of functions R ( r ) {\displaystyle R(r)} , Θ ( θ ) {\displaystyle \Theta (\theta )} , and Φ ( φ ) {\displaystyle \Phi (\varphi )} three independent differential functions appears with A and B being the separation constants:
The normalized position wavefunctions, given in spherical coordinates are: ψ n ℓ m ( r , θ , φ ) = ( 2 n a 0 ∗ ) 3 ( n − ℓ − 1 ) ! 2 n ( n + ℓ ) ! e − ρ / 2 ρ ℓ L n − ℓ − 1 2 ℓ + 1 ( ρ ) Y ℓ m ( θ , φ ) {\displaystyle \psi _{n\ell m}(r,\theta ,\varphi )={\sqrt {{\left({\frac {2}{na_{0}^{*}}}\right)}^{3}{\frac {(n-\ell -1)!}{2n(n+\ell )!}}}}\mathrm {e} ^{-\rho /2}\rho ^{\ell }L_{n-\ell -1}^{2\ell +1}(\rho )Y_{\ell }^{m}(\theta ,\varphi )}
where:
Note that the generalized Laguerre polynomials are defined differently by different authors. The usage here is consistent with the definitions used by Messiah, and Mathematica. In other places, the Laguerre polynomial includes a factor of ( n + ℓ ) ! {\displaystyle (n+\ell )!} , or the generalized Laguerre polynomial appearing in the hydrogen wave function is L n + ℓ 2 ℓ + 1 ( ρ ) {\displaystyle L_{n+\ell }^{2\ell +1}(\rho )} instead.
The quantum numbers can take the following values:
Additionally, these wavefunctions are normalized (i.e., the integral of their modulus square equals 1) and orthogonal: ∫ 0 ∞ r 2 d r ∫ 0 π sin ⁡ θ d θ ∫ 0 2 π d φ ψ n ℓ m ∗ ( r , θ , φ ) ψ n ′ ℓ ′ m ′ ( r , θ , φ ) = ⟨ n , ℓ , m | n ′ , ℓ ′ , m ′ ⟩ = δ n n ′ δ ℓ ℓ ′ δ m m ′ , {\displaystyle \int _{0}^{\infty }r^{2}\,dr\int _{0}^{\pi }\sin \theta \,d\theta \int _{0}^{2\pi }d\varphi \,\psi _{n\ell m}^{*}(r,\theta ,\varphi )\psi _{n'\ell 'm'}(r,\theta ,\varphi )=\langle n,\ell ,m|n',\ell ',m'\rangle =\delta _{nn'}\delta _{\ell \ell '}\delta _{mm'},} where | n , ℓ , m ⟩ {\displaystyle |n,\ell ,m\rangle } is the state represented by the wavefunction ψ n ℓ m {\displaystyle \psi _{n\ell m}} in Dirac notation, and δ {\displaystyle \delta } is the Kronecker delta function.
The wavefunctions in momentum space are related to the wavefunctions in position space through a Fourier transform φ ( p , θ p , φ p ) = ( 2 π ℏ ) − 3 / 2 ∫ e − i p → ⋅ r → / ℏ ψ ( r , θ , φ ) d V , {\displaystyle \varphi (p,\theta _{p},\varphi _{p})=(2\pi \hbar )^{-3/2}\int \mathrm {e} ^{-i{\vec {p}}\cdot {\vec {r}}/\hbar }\psi (r,\theta ,\varphi )\,dV,} which, for the bound states, results in φ ( p , θ p , φ p ) = 2 π ( n − ℓ − 1 ) ! ( n + ℓ ) ! n 2 2 2 ℓ + 2 ℓ ! n ℓ p ℓ ( n 2 p 2 + 1 ) ℓ + 2 C n − ℓ − 1 ℓ + 1 ( n 2 p 2 − 1 n 2 p 2 + 1 ) Y ℓ m ( θ p , φ p ) , {\displaystyle \varphi (p,\theta _{p},\varphi _{p})={\sqrt {{\frac {2}{\pi }}{\frac {(n-\ell -1)!}{(n+\ell )!}}}}n^{2}2^{2\ell +2}\ell !{\frac {n^{\ell }p^{\ell }}{(n^{2}p^{2}+1)^{\ell +2}}}C_{n-\ell -1}^{\ell +1}\left({\frac {n^{2}p^{2}-1}{n^{2}p^{2}+1}}\right)Y_{\ell }^{m}(\theta _{p},\varphi _{p}),} where C N α ( x ) {\displaystyle C_{N}^{\alpha }(x)} denotes a Gegenbauer polynomial and p {\displaystyle p} is in units of ℏ / a 0 ∗ {\displaystyle \hbar /a_{0}^{*}} .
The solutions to the Schrödinger equation for hydrogen are analytical, giving a simple expression for the hydrogen energy levels and thus the frequencies of the hydrogen spectral lines and fully reproduced the Bohr model and went beyond it. It also yields two other quantum numbers and the shape of the electron's wave function ("orbital") for the various possible quantum-mechanical states, thus explaining the anisotropic character of atomic bonds.
The Schrödinger equation also applies to more complicated atoms and molecules. When there is more than one electron or nucleus the solution is not analytical and either computer calculations are necessary or simplifying assumptions must be made.
Since the Schrödinger equation is only valid for non-relativistic quantum mechanics, the solutions it yields for the hydrogen atom are not entirely correct. The Dirac equation of relativistic quantum theory improves these solutions (see below).
The solution of the Schrödinger equation (wave equation) for the hydrogen atom uses the fact that the Coulomb potential produced by the nucleus is isotropic (it is radially symmetric in space and only depends on the distance to the nucleus). Although the resulting energy eigenfunctions (the orbitals) are not necessarily isotropic themselves, their dependence on the angular coordinates follows completely generally from this isotropy of the underlying potential: the eigenstates of the Hamiltonian (that is, the energy eigenstates) can be chosen as simultaneous eigenstates of the angular momentum operator. This corresponds to the fact that angular momentum is conserved in the orbital motion of the electron around the nucleus. Therefore, the energy eigenstates may be classified by two angular momentum quantum numbers, ℓ {\displaystyle \ell } and m {\displaystyle m} (both are integers). The angular momentum quantum number ℓ = 0 , 1 , 2 , … {\displaystyle \ell =0,1,2,\ldots } determines the magnitude of the angular momentum. The magnetic quantum number m = − ℓ , … , + ℓ {\displaystyle m=-\ell ,\ldots ,+\ell } determines the projection of the angular momentum on the (arbitrarily chosen) z {\displaystyle z} -axis.
In addition to mathematical expressions for total angular momentum and angular momentum projection of wavefunctions, an expression for the radial dependence of the wave functions must be found. It is only here that the details of the 1 / r {\displaystyle 1/r} Coulomb potential enter (leading to Laguerre polynomials in r {\displaystyle r} ). This leads to a third quantum number, the principal quantum number n = 1 , 2 , 3 , … {\displaystyle n=1,2,3,\ldots } . The principal quantum number in hydrogen is related to the atom's total energy.
Note that the maximum value of the angular momentum quantum number is limited by the principal quantum number: it can run only up to n − 1 {\displaystyle n-1} , i.e., ℓ = 0 , 1 , … , n − 1 {\displaystyle \ell =0,1,\ldots ,n-1} .
Due to angular momentum conservation, states of the same ℓ {\displaystyle \ell } but different m {\displaystyle m} have the same energy (this holds for all problems with rotational symmetry). In addition, for the hydrogen atom, states of the same n {\displaystyle n} but different ℓ {\displaystyle \ell } are also degenerate (i.e., they have the same energy). However, this is a specific property of hydrogen and is no longer true for more complicated atoms which have an (effective) potential differing from the form 1 / r {\displaystyle 1/r} (due to the presence of the inner electrons shielding the nucleus potential).
Taking into account the spin of the electron adds a last quantum number, the projection of the electron's spin angular momentum along the z {\displaystyle z} -axis, which can take on two values. Therefore, any eigenstate of the electron in the hydrogen atom is described fully by four quantum numbers. According to the usual rules of quantum mechanics, the actual state of the electron may be any superposition of these states. This explains also why the choice of z {\displaystyle z} -axis for the directional quantization of the angular momentum vector is immaterial: an orbital of given ℓ {\displaystyle \ell } and m ′ {\displaystyle m'} obtained for another preferred axis z ′ {\displaystyle z'} can always be represented as a suitable superposition of the various states of different m {\displaystyle m} (but same ℓ {\displaystyle \ell } ) that have been obtained for z {\displaystyle z} .
In 1928, Paul Dirac found an equation that was fully compatible with special relativity, and (as a consequence) made the wave function a 4-component "Dirac spinor" including "up" and "down" spin components, with both positive and "negative" energy (or matter and antimatter). The solution to this equation gave the following results, more accurate than the Schrödinger solution.
The energy levels of hydrogen, including fine structure (excluding Lamb shift and hyperfine structure), are given by the Sommerfeld fine-structure expression:
E j n = − μ c 2 [ 1 − ( 1 + [ α n − j − 1 2 + ( j + 1 2 ) 2 − α 2 ] 2 ) − 1 / 2 ] ≈ − μ c 2 α 2 2 n 2 [ 1 + α 2 n 2 ( n j + 1 2 − 3 4 ) ] , {\displaystyle {\begin{aligned}E_{j\,n}={}&-\mu c^{2}\left[1-\left(1+\left[{\frac {\alpha }{n-j-{\frac {1}{2}}+{\sqrt {\left(j+{\frac {1}{2}}\right)^{2}-\alpha ^{2}}}}}\right]^{2}\right)^{-1/2}\right]\\\approx {}&-{\frac {\mu c^{2}\alpha ^{2}}{2n^{2}}}\left[1+{\frac {\alpha ^{2}}{n^{2}}}\left({\frac {n}{j+{\frac {1}{2}}}}-{\frac {3}{4}}\right)\right],\end{aligned}}}
where α {\displaystyle \alpha } is the fine-structure constant and j {\displaystyle j} is the total angular momentum quantum number, which is equal to | ℓ ± 1 2 | {\displaystyle \left|\ell \pm {\tfrac {1}{2}}\right|} , depending on the orientation of the electron spin relative to the orbital angular momentum. This formula represents a small correction to the energy obtained by Bohr and Schrödinger as given above. The factor in square brackets in the last expression is nearly one; the extra term arises from relativistic effects (for details, see #Features going beyond the Schrödinger solution). It is worth noting that this expression was first obtained by A. Sommerfeld in 1916 based on the relativistic version of the old Bohr theory. Sommerfeld has however used different notation for the quantum numbers.
The image to the right shows the first few hydrogen atom orbitals (energy eigenfunctions). These are cross-sections of the probability density that are color-coded (black represents zero density and white represents the highest density). The angular momentum (orbital) quantum number ℓ is denoted in each column, using the usual spectroscopic letter code (s means ℓ = 0, p means ℓ = 1, d means ℓ = 2). The main (principal) quantum number n (= 1, 2, 3, ...) is marked to the right of each row. For all pictures the magnetic quantum number m has been set to 0, and the cross-sectional plane is the xz-plane (z is the vertical axis). The probability density in three-dimensional space is obtained by rotating the one shown here around the z-axis.
The "ground state", i.e. the state of lowest energy, in which the electron is usually found, is the first one, the 1s state (principal quantum level n = 1, ℓ = 0).
Black lines occur in each but the first orbital: these are the nodes of the wavefunction, i.e. where the probability density is zero. (More precisely, the nodes are spherical harmonics that appear as a result of solving the Schrödinger equation in spherical coordinates.)
The quantum numbers determine the layout of these nodes. There are:
The frequency of a state in level n is ω n = E n / ℏ {\displaystyle \omega _{n}=E_{n}/\hbar } , so in case of a superposition of multiple orbitals, they would oscillate due to the difference in frequency. For example two states, ψ1and ψ2: The wavefunction is given by ψ = ψ 1 e i ω 1 t + ψ 2 e i ω 2 t {\displaystyle \psi =\psi _{1}e^{i\omega _{1}t}+\psi _{2}e^{i\omega _{2}t}} and the probability function is P ( t ) = | ψ | 2 = ( ψ 1 e i ω 1 t + ψ 2 e i ω 2 t ) ( ψ 1 ∗ e − i ω 1 t + ψ 2 ∗ e − i ω 2 t ) {\displaystyle P(t)=|\psi |^{2}=(\psi _{1}e^{i\omega _{1}t}+\psi _{2}e^{i\omega _{2}t})(\psi _{1}^{*}e^{-i\omega _{1}t}+\psi _{2}^{*}e^{-i\omega _{2}t})} ∝ | ψ 1 ψ 2 | cos ⁡ [ ( ω 1 − ω 2 ) t ] {\displaystyle \propto |\psi _{1}\psi _{2}|\cos {[(\omega _{1}-\omega _{2})t]}}
The result is a rotating wavefunction. The movement of electrons and change of quantum states radiates light at a frequency of the cosine.
There are several important effects that are neglected by the Schrödinger equation and which are responsible for certain small but measurable deviations of the real spectral lines from the predicted ones:
Both of these features (and more) are incorporated in the relativistic Dirac equation, with predictions that come still closer to experiment. Again the Dirac equation may be solved analytically in the special case of a two-body system, such as the hydrogen atom. The resulting solution quantum states now must be classified by the total angular momentum number j (arising through the coupling between electron spin and orbital angular momentum). States of the same j and the same n are still degenerate. Thus, direct analytical solution of Dirac equation predicts 2S(⁠1/2⁠) and 2P(⁠1/2⁠) levels of hydrogen to have exactly the same energy, which is in a contradiction with observations (Lamb–Retherford experiment).
For these developments, it was essential that the solution of the Dirac equation for the hydrogen atom could be worked out exactly, such that any experimentally observed deviation had to be taken seriously as a signal of failure of the theory.
In the language of Heisenberg's matrix mechanics, the hydrogen atom was first solved by Wolfgang Pauli using a rotational symmetry in four dimensions [O(4)-symmetry] generated by the angular momentum and the Laplace–Runge–Lenz vector. By extending the symmetry group O(4) to the dynamical group O(4,2), the entire spectrum and all transitions were embedded in a single irreducible group representation.
In 1979 the (non-relativistic) hydrogen atom was solved for the first time within Feynman's path integral formulation of quantum mechanics by Duru and Kleinert. This work greatly extended the range of applicability of Feynman's method.
Further alternative models are Bohm mechanics and the complex Hamilton-Jacobi formulation of quantum mechanics.