Orthogonality of the associated Laguerre polynomials

The orthogonality of the associated Laguerre polynomials states that the integral of the product of two distinct associated Laguerre polynomials over a specified interval is zero.

It is defined mathematically as:

where is known as a weight function.

 

Question

Why is the weight function included? Can the orthogonality of the associated Laguerre polynomials be defined as , where ? Why are the limits of integration from 0 to ? Why are the polynomials and not ?

Answer

The weight function is an integral part of the orthogonality definition of associated Laguerre polynomials due to its role in ensuring convergence and its practical applications. It is often tied to specific problems, such as those in quantum mechanics. Omitting the weight function would sever this connection and could potentially alter the orthogonality properties of the polynomials. Therefore, defining orthogonality without the weight function would generally be invalid and would not reflect the intended use and properties of the associated Laguerre polynomials.

The weight function naturally defines the integration range because as , making the integral convergent over this range. This range is also connected to specific problems, such as the radial part of the wave functions in quantum mechanics. In the context of the hydrogen atom, represents a distance, which is always non-negative.

The eigenvalue of is a function of and not . Since the eigenfunctions of a Hermitian operator are orthogonal, two associated Laguerre polynomials with distinct values of  must be orthogonal. If we allow the values of to be different, we wouldn’t know if the result of the integral is solely due to the values of .

 

To prove eq453, we multiply the generating function for the associated Laguerre polynomials (see eq448) for and to give

Multiplying through by and integrating with respect to yields

 

Question

Show that , where is a non-negative integer.,

Answer

Let , and , and then and . Integrating by parts,

Let and , and then and . Integrating by parts

If we carry out integrations by parts, we have

 

Therefore, eq454 becomes

Expressing the LHS as a binomial series,

So,

Equating the coefficients of when  gives eq453.

 

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Normalisation constant of the associated Laguerre polynomials

The normalisation constant ensures that the associated Laguerre polynomials are properly scaled, thereby maintaining the probabilistic interpretation of quantum states.

To determine the normalisation constant , we equate the coefficients of eq455 when to give

Substituting and scaling the result of the integral to unity, we have or

Consider the integral of orthogonal associated Laguerre polynomials . Substituting eq450 and rearranging gives

Substituting eq456 yields

Eq457 is used to determine the normalisation constant of a hydrogenic radial wavefunction.

 

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Radial wavefunction

The radial wavefunction describes the probability distribution of the distance between an electron and the nucleus of a hydrogenic atom.

It is given by

where

are the associated Laguerre polynomials.
is the principal quantum number.
is the orbital angular momentum quantum number
is the Bohr radius.
is the distance between an electron and the nucleus of a hydrogenic atom.

 

Question

What is a hydrogenic atom?

Answer

It is an atom with only one electron, regardless of the number of protons in its nucleus, making it similar to a hydrogen atom in terms of its electronic structure. Examples of hydrogenic atoms include the hydrogen atom, He+, Li2+, and others.

 

To derive the un-normalised form of eq458, consider the Schrodinger equation of a hydrogenic atom, which is a two-particle problem. Utilising the concepts of center of mass and reduced mass, we have

where

is the kinetic energy operator of the translational motion of the system.
is the kinetic energy operator of the internal motion (rotational and vibrational motions) of the system.
is the combined masses of the electron and the nucleus.
is the reduced mass.
and are the laplacian operators acting on the centre of mass coordinates and the reduced mass coordinates, respectively.
is the ratio of the Planck constant and .
is the atomic number of the atom.
is the vacuum permittivity.
is the total wavefunction of the atom.
is the eigenvalue corresponding to .

Since translational motion is independent from rotational and vibrational motions, , where and are the translational energy of the system and the internal motion energy of the system respectively. This implies that . Noting that translational energy is purely kinetic, we can separate eq459 into two one-particle problems:

Eq460 is associated with the translational motion of the entire atom. Therefore, we are only concerned with eq461, which corresponds to the motion of the electron relative to the nucleus. Since (see this article for derivation), we can assume that , where  are the spherical harmonics. Multiplying eq461 through by and recognising that gives

where .

Substituting eq96 and eq133 yields the radial differential equation:

where .

Question

If , show that .

Answer

Substituting in the chain rule gives , which when substituted in yields . Substituting in the chain rule results in . Finally substituting in gives .

 

Letting , , and noting that  gives

To determine the solution to eq462, we analyse its asymptotes. As , eq462 approximates to , which has a possible solution of , where is a constant. When , the term dominates, giving , which has a solution of , where is a constant. Each solution on its own is not square-integrable over the interval . However, we can combine them to give a square-integrable form: .

 

Question

Verify that is a solution to eq462. Hence, show that , where , is also a solution to eq462.

Answer

Substituting the second derivative of  in eq462, we get , which when substituted in and then in yields the eigenvalue .

Consider , where . Substituting the second derivative of in eq462, we get and the eigenvalue , which implies that is a solution to eq462. Since eq462 is a linear differential equation, each term in , and hence the entire function, is a solution to eq462. We can simplify to , where because and .

is known as the principal quantum number. Since , we have

Consequently, the eigenvalue associated with eq462, and hence with the radial differential equation, is a function of :

where we have replaced with .

 

Substituting , and its second derivative in eq462 gives

To solve eq463, we transform it into an associated Laguerre differential equation, which has known solutions. This is accomplished by setting . Then, , and eq463 becomes

Eq464 is an associated Laguerre differential equation. Comparing eq464 and eq442, we have

where are the associated Laguerre polynomials.

The explicit expression of can then be found by carrying out the following substitutions:

    1. Substituting in yields , where is the Bohr radius.
    2. Substituting in gives .
    3. Substituting in  results in .
    4. Substituting in eq444, where and , gives

Substituting in yields . Substituting and noting that , we have

Eq466 is the un-normalised radial wavefunction for a hydrogenic atom. To derive its normalisation constant , we begin by substituting ,  and in eq457 to give

The expression for the normalisation of eq466 is or equivalently


Substituting eq467 yields

Therefore, the normalised radial wavefunction is

which can be easily rearranged to eq458.

 

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Degeneracy in hydrogenic atoms

Degeneracy in hydrogenic atoms refers to the number of possible states corresponding to a given energy value of a hydrogenic wavefunction.

The total wavefunction of a hydrogenic atom is characterised by three quantum numbers: , and . This implies that the state of the atom is defined by the set of quantum numbers . However, in a hydrogenic atom, the nucleus acts effectively as a point charge, and the electrostatic potential energy is spherically symmetric. This spherical symmetry means that the energy of the electron depends only on its distance from the nucleus. In other words, the energy of the electron is the eigenvalue associated with the radial component of the total wavefunction. As shown in eq462b, this eigenvalue is governed solely by the principal quantum number . Consequently, all the possible energy states defined by for a given must have the same energy and are therefore degenerate.

Since (see this article for explanation) and (see eq462a), the possible values of the orbital angular momentum quantum number range from 0 to for a given . Furthermore, for each value of , the magnetic quantum number can take on values (see this article for explanation). Therefore, the degeneracy for a given  is the sum of all the possible values of for each from 0 to :

 

Question

Show that .

Answer

The proof is in the 3rd Q&A of this article.

 

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Node

A node is a region in space where a wavefunction is zero. This implies that the probability of finding an electron at a node is zero. Since a wavefunction can have two components—radial and angular—it can have both radial and angular nodes.

A radial node is a spherical surface where the radial wavefunction of an atomic orbital is zero. The number of radial nodes in a hydrogenic wavefunction is given by the formula:

where is the principal quantum number and is the angular momentum quantum number.

 

Question

How is eq471 derived?

Answer

When , the associated Laguerre polynomial . Since the upper summation index of the explicit form of is , the polynomial will have roots if . In other words, will be zero (a node) as many times as .

 

An angular node is a flat plane or a cone where the angular wavefunction (also known as spherical harmonics) is zero. Using the same logic, the number of angular nodes  in corresponds to the number of roots when , where  are the associated Legendre polynomials. Since , the polynomial is of degree . Therefore,

The total number of nodes in is

The number of radial nodes helps define the spatial distribution of the electron density in orbitals. In other words, they influence the shape and energy of these orbitals, and therefore play a role in chemical bonding between orbitals.

 

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s-orbital

An s-orbital is a spherical region of space around the nucleus where an electron with zero orbital angular momentum is most likely to be found. The letter ”s” is of spectroscopic origin, standing for ‘sharp’.

One-electron s-orbital wavefunctions can be expressed using the total wavefunction of a hydrogenic atom:

where

, the radial wavefunction, is the radial component of .
, the spherical harmonics, is the angular component of .
are the associated Laguerre polynomials.
are the associated Legendre polynomials.
is the normalisation constant of the radial wavefunction.
is the normalisation constant of the spherical harmonics.
is the principal quantum number, where
is the orbital angular momentum quantum number (also known as azimuthal quantum number), where and .
is the magnetic quantum number, where .

The principal quantum number, , is also called a shell. Since the first shell is characterised by , the one-electron s-orbital wavefunction in the first shell, known as the 1s orbital, is defined by the set of quantum numbers . Substituting these values into the explicit formula for  yields:

Similarly, the one-electron s-orbital wavefunction in the second shell, known as the 2s orbital, is defined by the set of quantum numbers and has the formula:

Since  for all s-orbitals, their wavefunctions are independent of and . This implies that the values of an s-orbital wavefunction are the same in all directions in 3D space for a given . In other words, s-orbital wavefunctions are spherically symmetrical.

Finally, the 1s orbital and 2s orbital have 0 radial nodes and 1 radial node, respectively (see above diagram).

 

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Total wavefunction of a hydrogenic atom

The total wavefunction of a hydrogenic atom characterises the probability of locating an electron around the nucleus by incorporating both radial and angular components.

This spatial wavefunction is mathematically defined as:

where

, the radial wavefunction, is the radial component of .
, the spherical harmonics, is the angular component of .
are the associated Laguerre polynomials.
are the associated Legendre polynomials.
is the normalisation constant of the radial wavefunction.
is the normalisation constant of the spherical harmonics.
is the principal quantum number, where
is the orbital angular momentum quantum number (also known as azimuthal quantum number), where and .
is the magnetic quantum number, where .
is the distance between an electron and the nucleus of a hydrogenic atom.
is the polar angle.
is the azimuthal angle.
is the Bohr radius.
is the reduced mass of the atom.
is the ratio of the Planck constant and .
is the atomic number of the atom.
is the vacuum permittivity.

 

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p-orbital

A p-orbital, defined by the quantum number , is a dumbbell-shaped region of space around the nucleus where an electron is most likely to be found. The letter ”p” is of spectroscopic origin, standing for ‘principal’.

One-electron p-orbital wavefunctions can be expressed using the total wavefunction of a hydrogenic atom:

where

, the radial wavefunction, is the radial component of .
, the spherical harmonics, is the angular component of .
are the associated Laguerre polynomials.
are the associated Legendre polynomials.
is the normalisation constant of the radial wavefunction.
is the normalisation constant of the spherical harmonics.
is the principal quantum number, where
is the orbital angular momentum quantum number (also known as azimuthal quantum number), where and .
is the magnetic quantum number, where .

The principal quantum number, , is also called a shell. Since when , there are three p-orbitals that are characterised by the set of quantum numbers  of , and in each shell for . Each of the three p-orbitals has an angular node. Consider the set . Substituting these values into the explicit formula for  yields:

where .

Converting from spherical coordinates to Cartesian coordinates, where , gives

Eq474 is known as the orbital. When , the wavefunction is zero everywhere in the -plane, which is known as the nodal plane.

For the sets and , we have  and , respectively. These two wavefunctions include the factor , which may complicate calculations when they undergo symmetry operations. Therefore, we take linear combinations of these wavefunctions to form simpler wavefunctions. The first linear combination is , which normalises to , or equivalently in Cartesian coordinates:

since .

The second normalised linear combination is , or equivalently,

since .

and , like , each have an angular node.

 

Question

If and are already normalised, why do we need to normalise a linear combination of them? How do we normalise a linear combination of and ?

Answer

When forming a linear combination of normalised wavefunctions, the result is not necessarily normalised. Consider a general linear combination , where and are coefficients. The normalisation condition for requires that , where  represents the volume element in spherical coordinates. Expanding and noting that and are orthonormal, we have . If , which is the case for the two linear combinations of and , will not be normalised.

To normalise , we have  or

Using (see this article for proof) and some basic trigonometry identities yields

Setting and gives .

 

 

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d-orbital

A d-orbital, defined by the quantum number , is a region of space around the nucleus where an electron is most likely to be found. The letter ”d” is of spectroscopic origin, standing for ‘diffuse’.

One-electron d-orbital wavefunctions can be expressed using the total wavefunction of a hydrogenic atom:

where

, the radial wavefunction, is the radial component of .
, the spherical harmonics, is the angular component of .
are the associated Laguerre polynomials.
are the associated Legendre polynomials.
is the normalisation constant of the radial wavefunction.
is the normalisation constant of the spherical harmonics.
is the principal quantum number, where
is the orbital angular momentum quantum number (also known as azimuthal quantum number), where and .
is the magnetic quantum number, where .

The principal quantum number, , is also called a shell. Since when , there are five d-orbitals that are characterised by the set of quantum numbers  of , , , and in each shell for . Four of the five d-orbitals have cloverleaf shapes, while the fifth has a lobular structure along the -axis with a doughnut-shaped region around the equatorial plane. Each of the five d-orbitals has two angular nodes. Consider the set . Substituting these values into the explicit formula for  yields:

where .

Converting from spherical coordinates to Cartesian coordinates, where , gives

Eq478 is known as the wavefunction for the orbital. When or , . Therefore, the wavefunction is zero at in spherical coordinates. This implies that the angular nodes occur at two conical surfaces with their apices at the origin, extending at along the -axis.

For the sets and , we have  and , respectively. These two wavefunctions include the factor , which may complicate calculations when they undergo symmetry operations. Therefore, we take linear combinations of these wavefunctions to form simpler wavefunctions. The first linear combination is , which normalises to , or equivalently in Cartesian coordinates:

where and .

when or . This implies that has two nodal planes:  and .

 

Question

If and are already normalised, why do we need to normalise a linear combination of them? How do we normalise a linear combination of and ?

Answer

When forming a linear combination of normalised wavefunctions, the result is not necessarily normalised. Consider a general linear combination , where and are coefficients. The normalisation condition for requires that , where  represents the volume element in spherical coordinates. Expanding and noting that and are orthonormal, we have . If , which is the case for the two linear combinations of and , will not be normalised.

To normalise , we have  or

Since and ,

Using (see this article for proof) and setting and gives .

 

The second normalised linear combination is , or equivalently,

where and .

when or . This implies that has two nodal planes:  and .

For the remaining sets and , we apply the same logic to give and , where . when or , which implies two diagonal nodal planes. when or , which implies two nodes described by the planes and .

 

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f-orbital

An f-orbital, defined by the quantum number , is a region of space around the nucleus where an electron is most likely to be found. The letter ”f” is of spectroscopic origin, standing for ‘fundamental’. f-block elements have either hexagonal close pack, cubic close pack or body centred cubic structures. For non-cubic symmetry systems, we describe them using a general set of orbitals, which are derived in the same way as the d-orbitals. For cubic symmetry systems, they are better described by another set of f-orbitals known as the cubic set, which are derived by taking a different set of linear combinations. Both sets are eigenfunctions of the Schrödinger equation.

One-electron f-orbital wavefunctions can be expressed using the total wavefunction of a hydrogenic atom:

where

, the radial wavefunction, is the radial component of .
, the spherical harmonics, is the angular component of .
are the associated Laguerre polynomials.
are the associated Legendre polynomials.
is the normalisation constant of the radial wavefunction.
is the normalisation constant of the spherical harmonics.
is the principal quantum number, where
is the orbital angular momentum quantum number (also known as azimuthal quantum number), where and .
is the magnetic quantum number, where .

 

General set

The principal quantum number, , is also called a shell. Since when , there are seven f-orbitals that are characterised by the set of quantum numbers  of , , , , , and in each shell for . Each of the seven f-orbitals has three angular nodes. Consider the set . Substituting these values into the explicit formula for  yields:

where .

Converting from spherical coordinates to Cartesian coordinates, where , gives

Eq482 is known as the orbital. When or or , . represents the nodal plane, while implies that the angular nodes occur at two conical surfaces with their apices at the origin, extending at along the -axis.

For the sets and , we have  and , respectively. These two wavefunctions include the factor , which may complicate calculations when they undergo symmetry operations. Therefore, we take linear combinations of these wavefunctions to form simpler wavefunctions. The first linear combination is , which normalises to , or equivalently in Cartesian coordinates:

where , and .

One angular node occurs at  or when , which represents the -nodal-plane. The second and third angular nodes correspond to . These nodes are described by two conical surfaces with their apices at the origin, extending at along the -axis.

The second normalised linear combination is , or equivalently,

where .

One angular node occurs at , which represents the -nodal plane. The second and third angular nodes correspond to . These nodes are described by two conical surfaces with their apices at the origin, extending at along the -axis.

 

Question

If and are already normalised, why do we need to normalise a linear combination of them? How do we normalise a linear combination of and ?

Answer

When forming a linear combination of normalised wavefunctions, the result is not necessarily normalised. Consider a general linear combination , where and are coefficients. The normalisation condition for requires that , where  represents the volume element in spherical coordinates. Expanding and noting that and are orthonormal, we have . If , which is the case for the two linear combinations of and , will not be normalised.

To normalise , we have  or

Using (see this article for proof),  and setting and gives .

 

For the remaining sets , , and , we apply the same logic to give:

Wavefunction Angular nodes

-plane

-planes

-plane

-plane

-plane

-plane

-planes

-plane

-planes

 

Cubic set

Out of the seven cubic f-orbitals, three of them, ,  and are the same as the general set of f-orbitals. The other four derived by taking different linear combinations of general set of f -orbitals. They are:

Linear combination Normalised wavefunction Angular nodes

-plane

Conical surfaces with apices at the origin, extending along the -axis

-plane

Conical surfaces with apices at the origin, extending along the -axis

-plane

-planes

-plane

-planes

 

Question
    1. How do we know which set of linear combinations result in the cubic set of wavefunctions?
    2. How do we determine the angular nodes of ?
Answer
    1. The linear combinations that give the cubic set of wavefunctions must transform according to the point group.
    2. The angular nodes occur when , which implies that or . Obviously, corresponds to the -nodal-plane. , which states that increases as increases in spherical coordinates, represents two conical surfaces with their apices at the origin. Substituting gives . When (along the -axis), the angles that the conical surfaces make with the -axis are .

 

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