Newton's law of cooling

Newton's law of cooling states that the rate of heat loss of a body is proportional to the difference in temperatures between the body and its surroundings. As such, it is equivalent to a statement that the heat transfer coefficient, which mediates between heat losses and temperature differences, is a constant. This condition is generally true in thermal conduction (where it is guaranteed by Fourier's law), but it is often only approximately true in conditions of convective heat transfer, where a number of physical processes make effective heat transfer coefficients somewhat dependent on temperature differences. Finally, in the case of heat transfer by thermal radiation, Newton's law of cooling is not true.

Isaac Newton did not originally state his law in the above form in 1701, when it was originally formulated. Rather, using today's terms, Newton noted after some mathematical manipulation that the rate of temperature change of a body is proportional to the difference in temperatures between the body and its surroundings. This final simplest version of the law given by Newton himself, was partly due to confusion in Newton's time between the concepts of heat and temperature, which would not be fully disentangled until much later.^[1]

When stated in terms of temperature differences, Newton's law (with several further simplifying assumptions, such as a low Biot number and temperature-independent heat capacity) results in a simple differential equation for temperature-difference as a function of time. This equation has a solution that specifies a simple negative exponential rate of temperature-difference decrease, over time. This characteristic time function for temperature-difference behavior, is also associated with Newton's law of cooling.

Relationship to mechanism of cooling

Convection-cooling is sometimes called "Newton's law of cooling." This use is based on a work by Isaac Newton published anonymously as "Scala graduum Caloris. Calorum Descriptiones & signa." in Philosophical Transactions, 1701,^[2]

In cases where the heat transfer coefficient is independent, or relatively independent, of the temperature difference between object and environment, Newton's law is followed. This independence is sometimes the case, but is not guaranteed to be so. The heat transfer coefficient is often relatively independent of temperature in purely conduction-type cooling, but becomes a function of the temperature in classical natural convective heat transfer. In this case, Newton's law only approximates the result when the temperature changes are relatively small. Newton himself realized this limitation. A correction to Newton's law concerning larger temperature differentials was made in 1817 by Dulong and Petit.^[3] (These men are better-known for their formulation of the Dulong–Petit law concerning the molar specific heat capacity of a crystal.)

Another situation with temperature-dependent transfer coefficient is radiative heat transfer. Newton's law is not followed here.

Heat transfer version of the law

The heat-transfer version of Newton's law, which (as noted) requires a constant heat transfer coefficient, states that the rate of heat loss of a body is proportional to the difference in temperatures between the body and its surroundings.

The rate of heat transfer in such circumstances is derived below:^[4]

Newton's cooling law in conduction is a restatement of the differential equation given by Fourier's law:

{ \frac{d Q}{d t} = h \cdot A \cdot ( T(t)-T_{\text{env}}) = h \cdot A \Delta T(t)\quad }

where

Q

is the thermal energy in joules

h

is the heat transfer coefficient (assumed independent of T here) (W/(m² K))

A

is the heat transfer surface area (m²)

T

is the temperature of the object's surface and interior (since these are the same in this approximation)

T_{\text{env}}

is the temperature of the environment; i.e. the temperature suitably far from the surface

\Delta T(t)= T(t) - T_{\text{env}}

is the time-dependent thermal gradient between environment and object

The heat transfer coefficient h depends upon physical properties of the fluid and the physical situation in which convection occurs. Therefore, a single usable heat transfer coefficient (one that does not vary significantly across the temperature-difference ranges covered during cooling and heating) must be derived or found experimentally for every system that can be analyzed using the presumption that Newton's law will hold.

Formulas and correlations are available in many references to calculate heat transfer coefficients for typical configurations and fluids. For laminar flows, the heat transfer coefficient is rather low compared to turbulent flows; this is due to turbulent flows having a thinner stagnant fluid film layer on the heat transfer surface.^[5] However, note that Newton's law breaks down if the flows should transition between laminar or turbulent flow, since this will change the heat transfer coefficient h which is assumed constant in solving the equation.

The Biot number

Main article: Biot number

The Biot number, a dimensionless quantity, is defined for a body as:

\mathrm{Bi} = \frac{h L_C}{\ k_b}

where:

h = film coefficient or heat transfer coefficient or convective heat transfer coefficient
L_C = characteristic length, which is commonly defined as the volume of the body divided by the surface area of the body, such that $\mathit{L_C} = \frac{V_{\rm body}}{A_{\rm surface}}$
k_b = Thermal conductivity of the body

The physical significance of Biot number can be understood by imagining the heat flow from a hot metal sphere suddenly immersed in a pool, to the surrounding fluid. The heat flow experiences two resistances: the first at the surface of the sphere, and the second within the solid metal (which is influenced by both the size and composition of the sphere). The ratio of these resistances is the dimensionless Biot number.

If the thermal resistance of the fluid/sphere interface exceeds that thermal resistance offered by the interior of the metal sphere, the Biot number will be less than one. For systems where it is much less than one, the interior of the sphere may be presumed always to have the same temperature, although this temperature may be changing, as heat passes into the sphere from the surface. The equation to describe this change in (relatively uniform) temperature inside the object, is the simple exponential one described in Newton's law of cooling expressed in terms of temperature difference (see below).

In contrast, the metal sphere may be large, causing the characteristic length to increase to the point that the Biot number is larger than one. In this case, thermal gradients within the sphere become important, even though the sphere material is a good conductor. Equivalently, if the sphere is made of a thermally insulating (poorly conductive) material, such as wood or styrofoam, the interior resistance to heat flow will exceed that of the fluid/sphere boundary, even with a much smaller sphere. In this case, again, the Biot number will be greater than one.

Values of the Biot number smaller than 0.1 imply that the heat conduction inside the body is much faster than the heat convection away from its surface, and temperature gradients are negligible inside of it. This can indicate the applicability (or inapplicability) of certain methods of solving transient heat transfer problems. For example, a Biot number less than 0.1 typically indicates less than 5% error will be present when assuming a lumped-capacitance model of transient heat transfer (also called lumped system analysis).^[6] Typically this type of analysis leads to simple exponential heating or cooling behavior ("Newtonian" cooling or heating) since the amount of thermal energy (loosely, amount of "heat") in the body is directly proportional to its temperature, which in turn determines the rate of heat transfer into or out of it. This leads to a simple first-order differential equation which describes heat transfer in these systems.

Having a Biot number smaller than 0.1 labels a substance as "thermally thin," and temperature can be assumed to be constant throughout the material's volume. The opposite is also true: A Biot number greater than 0.1 (a "thermally thick" substance) indicates that one cannot make this assumption, and more complicated heat transfer equations for "transient heat conduction" will be required to describe the time-varying and non-spatially-uniform temperature field within the material body. Analytic methods for handling these problems, which may exist for simple geometric shapes and uniform material thermal conductivity, are described in the article on the heat equation.

Rate-of-change of temperature-difference version of the law

As noted in the section above, accurate formulation for temperatures may require analysis based on changing heat transfer coefficients at different temperatures, a situation frequently found in free-convection situations, and which precludes accurate use of Newton's law.

As noted above, Newton's law behavior when stated in terms of temperature change in the body, also requires that internal heat conduction within the object be large in comparison to the loss/gain of heat by surface transfer (conduction and/or convection), which is the condition where the Biot number is less than about 0.1. This allows the presumption of a single "temperature" inside the body (as a function of time) to make sense, as otherwise the body would have many different temperatures inside it, at any one time. This single temperature will generally change exponentially, as time progresses (see below).

Assumption of rapid internal conduction also allows use of the so-called lumped capacitance model. In this model, the amount of thermal energy in the body is calculated by assuming a constant heat capacity and thus thermal energy in the body is assumed to be a linear function of the body's temperature.

Temperature function-of-time solution in terms of object heat capacity

If the entire body is treated as lumped capacitance thermal energy reservoir, with a total thermal energy content which is proportional to simple total heat capacity $C$ , and $T$ , the temperature of the body, or $Q = C T$ , it is expected that the system will experience exponential decay in the temperature difference of body and surroundings, as a function of time. This is proven in the following sections:

From the definition of heat capacity $C$ comes the relation $C = dQ/dT$ . Differentiating this equation with regard to time gives the identity (valid so long as temperatures in the object are uniform at any given time): $dQ/dt = C (dT/dt)$ . This expression may be used to replace $dQ/dt$ in the first equation which begins this section, above. Then, if $T(t)$ is the temperature of such a body at time $t$ , and $T_{env}$ is the temperature of the environment around the body:

\frac{d T(t)}{d t} = - r (T(t) - T_{\mathrm{env}}) = - r \Delta T(t)\quad

where $r = hA/C$ is a positive constant characteristic of the system, which must be in units of $time^{-1}$ , and is therefore sometimes expressed in terms of a characteristic time constant $t_0$ given by: $r = 1/t_0 = - (dT(t)/dt)/\Delta T$ . Thus, in thermal systems, $t_0 = C/(hA)$ . (The total heat capacity $C$ of a system may be further represented by its mass-specific heat capacity $c_p$ multiplied by its mass $m$ , so that the time constant $t_0$ is also given by $mc_p/hA$ ).

The solution of this differential equation, by standard methods of integration and substitution of boundary conditions, gives:

T(t) = T_{\mathrm{env}} + (T(0) - T_{\mathrm{env}}) \ e^{-r t}. \quad

If:

\Delta T(t) \quad

is defined as :

T(t) - T_{\mathrm{env}} \ , \quad

where

\Delta T(0)\quad

is the initial temperature difference at time 0,

then the Newtonian solution is written as:

\Delta T(t) = \Delta T(0) \ e^{-r t} = \Delta T(0) \ e^{-t/t_0}. \quad

This same solution is more immediately apparent if the initial differential equation is written in terms of $\Delta T(t)$ , as a single function of time to be found, or "solved for."

\frac{d T(t)}{d t} = \frac{d\Delta T(t)}{d t} = - \frac{1}{t_0} \Delta T(t)\quad

References

↑ History of Newton's cooling law
↑ 824–829; ed. Joannes Nichols, Isaaci Newtoni Opera quae exstant omnia, vol. 4 (1782), 403–407.
↑ Whewell, William (1866). History of the Inductive Sciences from the Earliest to the Present Times.
↑ Louis C. Burmeister, (1993) “Convective Heat Transfer”, 2nd ed. Publisher Wiley-Interscience, p 107 ISBN 0-471-57709-X, 9780471577096, Google Book Search. Accessed 20-03-09
↑ http://www.engineersedge.com/heat_transfer/convection.htm Engineers Edge, 2009, “Convection Heat Transfer”,Accessed 20/03/09
↑ Incropera; DeWitt, Bergman, Lavine (2007). Fundamentals of Heat and Mass Transfer (6th ed.). John Wiley & Sons. pp. 260–261. ISBN 978-0-471-45728-2. Cite uses deprecated parameter |coauthors= (help)

External links

Heat conduction - Thermal-FluidsPedia
Newton's Law of Cooling by Jeff Bryant based on a program by Stephen Wolfram, Wolfram Demonstrations Project.

Isaac Newton

Publications	De analysi per aequationes numero terminorum infinitas (1669, published 1711) Method of Fluxions (1671) De motu corporum in gyrum (1684) Philosophiæ Naturalis Principia Mathematica (1687) General Scholium (1713) Opticks (1704) The Queries (1704) Arithmetica Universalis (1707)

Other writings	Notes on the Jewish Temple Quaestiones quaedam philosophicae The Chronology of Ancient Kingdoms Amended (1728) An Historical Account of Two Notable Corruptions of Scripture (1754)

Newtonianism	Bucket argument Newton's inequalities Newton's law of cooling Newton's law of universal gravitation Post-Newtonian expansion Parameterized post-Newtonian formalism Newton–Cartan theory Schrödinger–Newton equation Gravitational constant Newton's laws of motion Newtonian dynamics Newton's method in optimization Gauss–Newton algorithm Truncated Newton method Newton's rings Newton's theorem about ovals Newton–Pepys problem Newtonian potential Newtonian fluid Classical mechanics Newtonian fluid Corpuscular theory of light Leibniz–Newton calculus controversy Rotating spheres Newton's cannonball Newton–Cotes formulas Newton's method Newton fractal Generalized Gauss–Newton method Newton's identities Newton polynomial Newton's theorem of revolving orbits Newton–Euler equations Newton number Kissing number problem Power number Solar mass Dynamics Absolute time and space Finite difference Table of Newtonian series Impact depth Structural coloration Inertia

Life	Cranbury Park Woolsthorpe Manor Early life of Isaac Newton Later life of Isaac Newton Religious views of Isaac Newton Isaac Newton's occult studies The Mysteryes of Nature and Art Scientific revolution Copernican Revolution

Friends and family	Catherine Barton John Conduitt William Clarke Benjamin Pulleyn William Stukeley William Jones Isaac Barrow Abraham de Moivre John Keill

Discoveries and inventions	Calculus Newton disc Newton polygon Newton–Okounkov body Newton's reflector Newtonian telescope Newton scale Newton's metal Newton's cradle Sextant

Phrases	Hypotheses non fingo Standing on the shoulders of giants

Theory expansions	Kepler's laws of planetary motion Problem of Apollonius

Related	Writing of Principia Mathematica Newton (Blake) List of things named after Isaac Newton Isaac Newton in popular culture Elements of the Philosophy of Newton Isaac Newton S/O Philipose Newton (unit)

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