You do not have permission to edit this page, for the following reasons:

This IP address has been blocked from editing Wikipedia.
This does not affect your ability to read Wikipedia pages.
Most people who see this message have done nothing wrong. Some kinds of blocks restrict editing from specific service providers or telecom companies in response to recent abuse or vandalism, and can sometimes affect other users who are unrelated to that abuse. Review the information below for assistance if you do not believe that you have done anything wrong.

The IP address or range 3.238.0.0/16 has been blocked by ‪ST47‬ for the following reason(s):

The IP address that you are currently using has been blocked because it is believed to be a web host provider. To prevent abuse, web hosts may be blocked from editing Wikipedia.
You will not be able to edit Wikipedia using a web host provider because it hides your IP address, much like a proxy or VPN.
We recommend that you attempt to use another connection to edit. For example, if you use a proxy or VPN to connect to the internet, turn it off when editing Wikipedia. If you edit using a mobile connection, try using a Wi-Fi connection, and vice versa. If you are using a corporate internet connection, switch to a different Wi-Fi network. If you have a Wikipedia account, please log in.
If you do not have any other way to edit Wikipedia, you will need to request an IP block exemption.

How to appeal if you are confident that your connection does not use a web host's IP address:
If you are confident that you are not using a web host, you may appeal this block by adding the following text on your talk page: ((unblock|reason=Caught by a web host block but this host or IP is not a web host. My IP address is _______. Place any further information here. ~~~~)). You must fill in the blank with your IP address for this block to be investigated. Your IP address can be determined here. Alternatively, if you wish to keep your IP address private you can use the unblock ticket request system. There are several reasons you might be editing using the IP address of a web host (such as if you are using VPN software or a business network); please use this method of appeal only if you think your IP address is in fact not a web host.

Administrators: The IP block exemption user right should only be applied to allow users to edit using web host in exceptional circumstances, and they should usually be directed to the functionaries team via email. If you intend to give the IPBE user right, a CheckUser needs to take a look at the account. This can be requested most easily at SPI Quick Checkuser Requests. Unblocking an IP or IP range with this template is highly discouraged without at least contacting the blocking administrator.

This block will expire on 05:34, 21 January 2026. Your current IP address is 3.238.27.177.

Even when blocked, you will usually still be able to edit your user talk page, as well as email administrators and other editors.

For information on how to proceed, please read the FAQ for blocked users and the guideline on block appeals. The guide to appealing blocks may also be helpful.

Other useful links: Blocking policy · Help:I have been blocked
This IP address range has been globally blocked.
This does not affect your ability to read Wikipedia pages.
Most people who see this message have done nothing wrong. Some kinds of blocks restrict editing from specific service providers or telecom companies in response to recent abuse or vandalism, and can sometimes affect other users who are unrelated to that abuse. Review the information below for assistance if you do not believe that you have done anything wrong.

This block affects editing on all Wikimedia wikis.
The IP address or range 3.238.0.0/16 has been globally blocked by ‪Jon Kolbert‬ for the following reason(s):

Open proxy/Webhost: See the help page if you are affected

This block will expire on 05:35, 21 February 2029. Your current IP address is 3.238.27.177.

Even while globally blocked, you will usually still be able to edit pages on Meta-Wiki.

If you believe you were blocked by mistake, you can find additional information and instructions in the No open proxies global policy. Otherwise, to discuss the block please post a request for review on Meta-Wiki. You could also send an email to the stewards VRT queue at stewards@wikimedia.org including all above details.

Other useful links: Global blocks · Help:I have been blocked

You can view and copy the source of this page:

((Short description|Independent parameter describing the state of a physical system))
((About|physics and chemistry|other fields|Degrees of freedom))
((More citations needed|date=November 2009))

In [[physics]] and [[chemistry]], a '''degree of freedom''' is an independent physical [[parameter]] in the formal description of the state of a [[physical system]]. The set of all states of a system is known as the system's [[phase space]], and the degrees of freedom of the system are the [[dimension]]s of the phase space.

The location of a [[particle]] in [[three-dimensional space]] requires three [[Coordinate system|position coordinates]]. Similarly, the direction and speed at which a particle moves can be described in terms of three velocity components, each in reference to the three dimensions of space.  So, if the [[time evolution]] of the system is [[Deterministic system|deterministic]] (where the state at one instant uniquely determines its past and future position and velocity as a function of time), such a system has six degrees of freedom.((citation needed|date=November 2015)) If the motion of the particle is constrained to a lower number of dimensions – for example, the particle must move along a wire or on a fixed surface – then the system has fewer than six degrees of freedom. On the other hand, a system with an extended object that can rotate or vibrate can have more than six degrees of freedom.

In [[classical mechanics]], the state of a [[point particle]] at any given time is often described with position and velocity coordinates in the [[Lagrangian mechanics|Lagrangian]] formalism, or with position and [[momentum]] coordinates in the [[Hamiltonian (quantum mechanics)|Hamiltonian]] formalism.

In [[statistical mechanics]], a degree of freedom is a single [[scalar (physics)|scalar]] number describing the [[microstate (statistical mechanics)|microstate]] of a system.<ref name=":0">((cite book |last=Reif |first=F. |title=Fundamentals of Statistical and Thermal Physics |year=2009 |publisher=Waveland Press, Inc. |location=Long Grove, IL |isbn=978-1-57766-612-7 |page=51))</ref> The specification of all microstates of a system is a point in the system's [[phase space]].

In the 3D [[ideal chain]] model in chemistry, two [[angle]]s are necessary to describe the orientation of each monomer.

It is often useful to specify quadratic degrees of freedom. These are degrees of freedom that contribute in a quadratic function to the energy of the system.

Depending on what one is counting, there are several different ways that degrees of freedom can be defined,
each with a different value.<ref>((Cite web|url=https://chemistry.stackexchange.com/questions/83840/does-a-diatomic-gas-have-one-or-two-vibrational-degrees-of-freedom|title = Physical chemistry - Does a diatomic gas have one or two vibrational degrees of freedom?))</ref>

==Thermodynamic degrees of freedom for gases==
((External image|Link=|image1=https://chem.libretexts.org/@api/deki/files/9669/h2ovibrations.gif?revision=1|image2=https://chem.libretexts.org/@api/deki/files/9668/co2vibrations.gif?revision=1))
By the [[equipartition theorem]], internal energy per mole of gas equals ((math|''c''<sub>v</sub> ''T'')), where ((mvar|T)) is [[absolute temperature]] and the specific heat at constant volume is c<sub>v</sub> = (f)(R/2).
R = 8.314 J/(K mol) is the universal gas constant, and "f" is the number of thermodynamic (quadratic) degrees of freedom,
counting the number of ways in which energy can occur.

Any atom or molecule has three degrees of freedom associated with translational motion (kinetic energy) of the [[center of mass]] with respect to the x, y, and z axes. These are the only degrees of freedom for a monoatomic species, such as [[noble gas]] atoms.

[[File:Rotations in water molecule.png|thumb|]]
For a structure consisting of two or more atoms, the whole structure also has rotational kinetic energy, where the whole structure turns about an axis.
A [[linear molecular geometry|linear molecule]], where all atoms lie along a single axis,
such as any [[diatomic molecule]] and some other molecules like [[carbon dioxide]] (CO<sub>2</sub>),
has two rotational degrees of freedom, because it can rotate about either of two axes perpendicular to the molecular axis.
A nonlinear molecule, where the atoms do not lie along a single axis, like [[Properties of water|water]] (H<sub>2</sub>O), has three rotational degrees of freedom, because it can rotate around any of three perpendicular axes.
In special cases, such as adsorbed large molecules, the rotational degrees of freedom can be limited to only one.<ref>((cite journal|doi=10.1002/cphc.201200531|pmid=23047526|title=Stabilization of Large Adsorbates by Rotational Entropy: A Time-Resolved Variable-Temperature STM Study|journal=ChemPhysChem|volume=14 |issue=1|pages=162–9|year=2013 | last1=Waldmann|first1=Thomas |last2=Klein|first2=Jens|last3=Hoster|first3=Harry E.|last4=Behm|first4=R. Jürgen|s2cid=36848079 ))</ref>

A structure consisting of two or more atoms also has vibrational energy, where the individual atoms move with respect to one another. A diatomic molecule has one [[molecular vibration]] mode: the two atoms oscillate back and forth with the chemical bond between them acting as a spring. A molecule with ((mvar|N)) atoms has more complicated modes of [[molecular vibration]], with ((math|3''N'' − 5)) vibrational modes for a linear molecule and ((math|3''N'' − 6)) modes for a nonlinear molecule.<ref>[[Molecular vibration]]((User-generated source|date=January 2021))</ref>
As specific examples, the linear CO<sub>2</sub> molecule has 4 modes of oscillation,<ref>For drawings, see http://www.colby.edu/chemistry/PChem/notes/NormalModesText.pdf</ref> and the nonlinear water molecule has 3 modes of oscillation<ref>For drawings, see https://sites.cns.utexas.edu/jones_ch431/normal-modes-vibration</ref>
Each vibrational mode has two energy terms: the [[kinetic energy]] of the moving atoms and the [[potential energy]] of the spring-like chemical bond(s).
Therefore, the number of vibrational energy terms is ((math|2(3''N'' − 5))) modes for a linear molecule and is ((math|2(3''N'' − 6))) modes for a nonlinear molecule.

Both the rotational and vibrational modes are quantized, requiring a minimum temperature to be activated.<ref>Section 12-7 (pp. 376-379) of Sears and Salinger, 1975: Thermodynamics, Kinetic Theory, and Statistical Thermodynamics. Third edition. Addison-Wesley Publishing Co.</ref> The "[[rotational temperature]]" to activate the rotational degrees of freedom is less than 100 K for many gases. For N<sub>2</sub> and O<sub>2</sub>, it is less than 3 K.<ref name=":0" />
The "[[vibrational temperature]]" necessary for substantial vibration is between 10<sup>3</sup> K and 10<sup>4</sup> K, 3521 K for N<sub>2</sub> and 2156 K for O<sub>2</sub>.<ref name=":0" /> Typical atmospheric temperatures are not high enough to activate vibration in N<sub>2</sub> and O<sub>2</sub>, which comprise most of the atmosphere. (See the next figure.) However, the much less abundant [[greenhouse gas]]es keep the [[troposphere]] warm by absorbing [[infrared]] from the Earth's surface, which excites their vibrational modes.<ref>((Cite web|last=|first=|date=|title=Molecules Vibrate|url=https://scied.ucar.edu/molecular-vibration-modes|url-status=live|archive-url=https://web.archive.org/web/20141010161149/http://scied.ucar.edu:80/molecular-vibration-modes |archive-date=2014-10-10 |access-date=2021-01-19|website=UCAR Center for Science Education))</ref>
Much of this energy is reradiated back to the surface in the infrared through the "[[greenhouse effect]]."

Because room temperature (≈298 K) is over the typical rotational temperature but lower than the typical vibrational temperature, only the translational and rotational degrees of freedom contribute, in equal amounts, to the [[heat capacity ratio]]. This is why ((mvar|γ))≈((math|((sfrac|5|3)))) for [[monatomic]] gases and ((mvar|γ))≈((math|((sfrac|7|5)))) for [[diatomic]] gases at room temperature.<ref name=":0" />
[[File:Specific heat at constant volume for dry air vs T.png|thumb|Graph of the specific heat of dry air at constant volume, c<sub>v</sub>, as a function of temperature numerical values are taken from the table at Air - Specific Heat at Constant Pressure and Varying Temperature.<ref>((Cite web|url=https://www.engineeringtoolbox.com/air-specific-heat-capacity-d_705.html|title=Air - Specific Heat vs. Temperature at Constant Pressure))</ref> Those values have units of J/(K kg), so reference lines at plotted (5/2) ((mvar|R))<sub>d</sub> and (7/2) ((mvar|R))<sub>d</sub>, where ((mvar|R))<sub>d</sub> = ((sfrac|((mvar|R<sub>d</sub>))|((mvar|M)))) is the gas constant for dry air, ((mvar|R)) = 8.314 J/(K mol) is the universal gas constant, and M<sub>d</sub> =  28.965369 g/mol is the molar mass of dry air.<ref>Gatley, D. P., S. Herrmann, H.-J. Kretzshmar, 2008: A twenty-first century molar mass for dry air. HVAC&R Research, vol. 14, pp. 655-662.</ref>
At T = 140, 160, 200, 220, 320, 340, 360, 380 K, c<sub>v</sub> = 718.4, 717.2, 716.3, 716.3, 719.2, 720.6, 722.3, 724.3 J/(K kg). Thus, for 140 K < T < 360 K, c<sub>v</sub> differs from (5/2) R<sub>d</sub> by less than 1%.]]
Since the [[Atmosphere_of_Earth|air]] is dominated by diatomic gases (with [[nitrogen]] and [[oxygen]] contributing about 99%), its molar internal energy is close to ((math|c<sub>v</sub> T)) = (5/2)((mvar|R))((mvar|T)), determined by the 5 degrees of freedom exhibited by diatomic gases.((cn|date=October 2022))<ref>[[Equipartition theorem#Diatomic gases]]</ref>((circular ref|date=January 2021))
See the graph at right. For 140 K < ((mvar|T)) < 380 K, c<sub>v</sub> differs from (5/2) ((mvar|R))<sub>d</sub> by less than 1%.
Only at temperatures well above temperatures in the [[troposphere]] and [[stratosphere]] do some molecules have enough energy to activate the vibrational modes of N<sub>2</sub> and O<sub>2</sub>. The specific heat at constant volume, c<sub>v</sub>, increases slowly toward (7/2) ((mvar|R)) as temperature increases above T = 400 K, where c<sub>v</sub> is 1.3% above (5/2) ((mvar|R))<sub>d</sub> = 717.5 J/(K kg).
{| class="wikitable"
|+Component degrees of freedom for ((Mvar|N)) atoms (3((Mvar|N)) total coordinate motions)
|-
!
! [[Monatomic]]
! [[Linear molecule]]s
! [[molecular geometry|Non-linear molecules]]
|-
| Translation (((mvar|x)), ((mvar|y)), and ((mvar|z)))
| align="center" | 3
| align="center" | 3
| align="center" | 3
|-
| Rotation (((mvar|x)), ((mvar|y)), and ((mvar|z)))
| align="center" | 0
| align="center" | 2
| align="center" | 3
|-
| Vibration (high temperature)
| align="center" | 0
| align="center" | ((math|2 (3''N'' − 5)))
| align="center" | ((math|2 (3''N'' − 6)))
|}

===Counting the minimum number of co-ordinates to specify a position===

One can also count degrees of freedom using the minimum number of coordinates required to specify a position. This is done as follows:
# For a single particle we need 2 coordinates in a 2-D plane to specify its position and 3 coordinates in 3-D space. Thus its degree of freedom in a 3-D space is 3.
# For a body consisting of 2 particles (ex. a diatomic molecule) in a 3-D space with constant distance between them (let's say d) we can show (below) its degrees of freedom to be 5.
Let's say one particle in this body has coordinate ((math|(''x''<sub>1</sub>, ''y''<sub>1</sub>, ''z''<sub>1</sub>))) and the other has coordinate ((math|(''x''<sub>2</sub>, ''y''<sub>2</sub>, ''z''<sub>2</sub>))) with ((math| ''z''<sub>2</sub>)) unknown. Application of the formula for distance between two coordinates
:<math>d=\sqrt{(x_2-x_1)^2+(y_2-y_1)^2+(z_2-z_1)^2}</math>
results in one equation with one unknown, in which we can solve for ((math|''z''<sub>2</sub>)).
One of ((math|''x''<sub>1</sub>)), ((math|''x''<sub>2</sub>)), ((math|''y''<sub>1</sub>)), ((math|''y''<sub>2</sub>)), ((math|''z''<sub>1</sub>)), or ((math|''z''<sub>2</sub>)) can be unknown.

Contrary to the classical [[equipartition theorem]], at room temperature, the vibrational motion of molecules typically makes negligible contributions to the [[heat capacity]]. This is because these degrees of freedom are ''frozen'' because the spacing between the energy [[eigenvalue]]s exceeds the energy corresponding to ambient [[temperature]]s (((math|''k''<sub>B</sub>''T''))).<ref name=":0" />

==Independent degrees of freedom==
The set of degrees of freedom ((math|''X''<sub>1</sub>, ... , ''X''<sub>''N''</sub>)) of a system is independent if the energy associated with the set can be written in the following form:
:<math>E = \sum_{i=1}^N E_i(X_i),</math>

where ((mvar|E<sub>i</sub>)) is a function of the sole variable ((mvar|X<sub>i</sub>)).

example: if ((math|''X''<sub>1</sub>)) and ((math|''X''<sub>2</sub>)) are two degrees of freedom, and ((mvar|E)) is the associated energy:
* If <math>E = X_1^4 + X_2^4</math>, then the two degrees of freedom are independent.
* If <math>E = X_1^4 + X_1 X_2 + X_2^4</math>, then the two degrees of freedom are ''not'' independent. The term involving the product of ((math|''X''<sub>1</sub>)) and ((math|''X''<sub>2</sub>)) is a coupling term that describes an interaction between the two degrees of freedom.

For ((mvar|i)) from 1 to ((mvar|N)), the value of the ((mvar|i))th degree of freedom ((mvar|X<sub>i</sub>)) is distributed according to the [[Boltzmann distribution]]. Its [[probability density function]] is the following:
: <math>p_i(X_i) = \frac{e^{-\frac{E_i}{k_B T))}{\int dX_i \, e^{-\frac{E_i}{k_B T))}</math>,

In this section, and throughout the article the brackets <math>\langle \rangle</math> denote the [[mean]] of the quantity they enclose.

The [[internal energy]] of the system is the sum of the average energies associated with each of the degrees of freedom:
:<math>\langle E \rangle = \sum_{i=1}^N \langle E_i \rangle.</math>

==Quadratic degrees of freedom==
A degree of freedom ((mvar|X<sub>i</sub>)) is quadratic if the energy terms associated with this degree of freedom can be written as
:<math>E = \alpha_i\,\,X_i^2 + \beta_i \,\, X_i Y </math>,

where ((mvar|Y)) is a [[linear combination]] of other quadratic degrees of freedom.

example: if ((math|''X''<sub>1</sub>)) and ((math|''X''<sub>2</sub>)) are two degrees of freedom, and ((mvar|E)) is the associated energy:
* If <math>E = X_1^4 + X_1^3 X_2 + X_2^4</math>, then the two degrees of freedom are not independent and non-quadratic.
* If <math>E = X_1^4 + X_2^4</math>, then the two degrees of freedom are independent and non-quadratic.
* If <math>E = X_1^2 + X_1 X_2 + 2X_2^2</math>, then the two degrees of freedom are not independent but are quadratic.
* If <math>E = X_1^2 + 2X_2^2</math>, then the two degrees of freedom are independent and quadratic.

For example, in [[Newtonian mechanics]], the [[Dynamics (mechanics)|dynamics]] of a system of quadratic degrees of freedom are controlled by a set of homogeneous [[linear differential equation]]s with [[constant coefficients]].

===Quadratic and independent degree of freedom===
((math|''X''<sub>1</sub>, ... , ''X''<sub>''N''</sub>)) are quadratic and independent degrees of freedom if the energy associated with a microstate of the system they represent can be written as:
:<math>E = \sum_{i=1}^N \alpha_i X_i^2</math>

===Equipartition theorem===
((main|Equipartition theorem))
In the classical limit of [[statistical mechanics]], at [[thermodynamic equilibrium]], the [[internal energy]] of a system of ((mvar|N)) quadratic and independent degrees of freedom is:
: <math>U = \langle E \rangle = N\,\frac{k_B T}{2}</math>

Here, the [[mean]] energy associated with a degree of freedom is:
:<math>\langle E_i \rangle = \int dX_i\,\,\alpha_i X_i^2\,\, p_i(X_i) = \frac{\int dX_i\,\,\alpha_i X_i^2\,\, e^{-\frac{\alpha_i X_i^2}{k_B T))}{\int dX_i\,\, e^{-\frac{\alpha_i X_i^2}{k_B T))} </math>
:<math>\langle E_i \rangle = \frac{k_B T}{2}\frac{\int dx\,\,x^2\,\, e^{-\frac{x^2}{2))}{\int dx\,\, e^{-\frac{x^2}{2))} = \frac{k_B T}{2} </math>

Since the degrees of freedom are independent, the [[internal energy]] of the system is equal to the sum of the [[mean]] energy associated with each degree of freedom, which demonstrates the result.

==Generalizations==
The description of a system's state as a [[point (geometry)|point]] in its phase space, although mathematically convenient, is thought to be fundamentally inaccurate. In [[quantum mechanics]], the motion degrees of freedom are superseded with the concept of [[wave function]], and [[operator (physics)|operators]] which correspond to other degrees of freedom have [[point spectrum|discrete spectra]]. For example, [[angular momentum operator#Spin, orbital, and total angular momentum|intrinsic angular momentum]] operator (which corresponds to the rotational freedom) for an [[electron]] or [[photon]] has only two [[eigenvalue]]s. This discreteness becomes apparent when [[action (physics)|action]] has an [[order of magnitude]] of the [[Planck constant]], and individual degrees of freedom can be distinguished.

==References==
((Reflist))

((Authority control))

[[Category:Physical quantities]]
[[Category:Dimension]]

Pages transcluded onto the current version of this page (help):

Degrees of freedom (physics and chemistry) (edit)
Template:About (view source) (template editor protected)
Template:Ambox (view source) (template editor protected)
Template:Authority control (view source) (template editor protected)
Template:Category handler (view source) (protected)
Template:Circular ref (edit)
Template:Circular reference (view source) (template editor protected)
Template:Citation needed (view source) (protected)
Template:Cite book (view source) (protected)
Template:Cite journal (view source) (protected)
Template:Cite web (view source) (protected)
Template:Cn (view source) (template editor protected)
Template:Delink (view source) (protected)
Template:External image (edit)
Template:External media (view source) (template editor protected)
Template:Find sources mainspace (view source) (template editor protected)
Template:Fix (view source) (protected)
Template:Fix/category (view source) (protected)
Template:Hlist/styles.css (view source) (protected)
Template:Infobox (view source) (template editor protected)
Template:Main (view source) (template editor protected)
Template:Main other (view source) (protected)
Template:Math (view source) (template editor protected)
Template:More citations needed (view source) (template editor protected)
Template:Mvar (view source) (template editor protected)
Template:Pagetype (view source) (protected)
Template:Reflist (view source) (protected)
Template:Reflist/styles.css (view source) (protected)
Template:SDcat (view source) (protected)
Template:Sfrac (view source) (extended confirmed protected)
Template:Sfrac/styles.css (view source) (extended confirmed protected)
Template:Short description (view source) (protected)
Template:Short description/lowercasecheck (view source) (protected)
Template:Template other (view source) (protected)
Template:User-generated source (view source) (template editor protected)
Module:About (view source) (template editor protected)
Module:Arguments (view source) (protected)
Module:Authority control (view source) (template editor protected)
Module:Authority control/config (view source) (template editor protected)
Module:Category handler (view source) (protected)
Module:Category handler/blacklist (view source) (protected)
Module:Category handler/config (view source) (protected)
Module:Category handler/data (view source) (protected)
Module:Category handler/shared (view source) (protected)
Module:Check for unknown parameters (view source) (protected)
Module:Citation/CS1 (view source) (protected)
Module:Citation/CS1/COinS (view source) (protected)
Module:Citation/CS1/Configuration (view source) (protected)
Module:Citation/CS1/Date validation (view source) (protected)
Module:Citation/CS1/Identifiers (view source) (protected)
Module:Citation/CS1/Utilities (view source) (protected)
Module:Citation/CS1/Whitelist (view source) (protected)
Module:Citation/CS1/styles.css (view source) (protected)
Module:Delink (view source) (protected)
Module:Disambiguation/templates (view source) (protected)
Module:EditAtWikidata (view source) (protected)
Module:Find sources (view source) (template editor protected)
Module:Find sources/config (view source) (template editor protected)
Module:Find sources/links (view source) (template editor protected)
Module:Find sources/templates/Find sources mainspace (view source) (template editor protected)
Module:Format link (view source) (template editor protected)
Module:Hatnote (view source) (template editor protected)
Module:Hatnote/styles.css (view source) (template editor protected)
Module:Hatnote list (view source) (template editor protected)
Module:Infobox (view source) (template editor protected)
Module:Infobox/styles.css (view source) (template editor protected)
Module:Labelled list hatnote (view source) (template editor protected)
Module:Message box (view source) (protected)
Module:Message box/ambox.css (view source) (protected)
Module:Message box/configuration (view source) (protected)
Module:Namespace detect/config (view source) (protected)
Module:Namespace detect/data (view source) (protected)
Module:Navbar (view source) (protected)
Module:Navbar/configuration (view source) (protected)
Module:Navbox (view source) (template editor protected)
Module:Navbox/configuration (view source) (template editor protected)
Module:Navbox/styles.css (view source) (template editor protected)
Module:Pagetype (view source) (protected)
Module:Pagetype/config (view source) (protected)
Module:Pagetype/disambiguation (view source) (protected)
Module:Pagetype/rfd (view source) (template editor protected)
Module:Pagetype/setindex (view source) (protected)
Module:Pagetype/softredirect (view source) (protected)
Module:SDcat (view source) (protected)
Module:String (view source) (protected)
Module:Unsubst (view source) (protected)
Module:Wikitext Parsing (view source) (protected)
Module:Yesno (view source) (protected)

Return to Degrees of freedom (physics and chemistry).

Retrieved from "https://en.wikipedia.org/wiki/Degrees_of_freedom_(physics_and_chemistry)"