Two body applications of Newtons law of cooling.

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SUMMARY

The discussion focuses on deriving the temperature function for an enclosed body of water (T_a) immersed in another body of water (T_b) using Newton's Law of Cooling. The formula T(t) = T_s + (T_0 - T_s)e^{-kt} is deemed inadequate due to the changing temperature of the surrounding water. The correct approach involves using the equation dU_a/dt = -k(T_a - T_b) and integrating to find T_a as a function of time, ultimately leading to T_a = ((T_a0 - T_b0)e^{(-k(t)/(C_a + C_b))} + (C_aT_a + C_bT_b)/C_b)/(1 + C_a/C_b). The analysis confirms that the system reaches equilibrium based on the specific heat capacities of both bodies.

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Homework Statement



What's the formula that better describes the temperature as a function of time for an enclosed body of water with certain initial temperature T_a immersed in another body of water of initial temperature T_b?

More clearly, I performed an experiment in which I put a small body of nearly boiling water (enclosed in a metal cylinder) inside a somewhat bigger body of ice-cold water, and measured T for both bodies of water at 1 minute intervals during 40 minutes; what's the equations that best describes this situation and to which I can compare my results? I am reluctant to use T(t) = T_s + ( T_0 - T_s )e^{-kt} because the latter assumes that the environment's temperature remains more or less constant, while in my case I do measure a change of temperature (of about 10C) in it (the large body of cold water).

Sorry if my post was somewhat hard to read.


Homework Equations





The Attempt at a Solution



Thanks in advance for your help.
 
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I wondered about this myself and decided to sit down and do it today out of curiosity. Post is 2 years old but it's worth putting. Also it's my first time using Latex so forgive the inconsistency of lettering.

Start from Newton's law of cooling, with t as time, T temp, and k constant,

\frac{dT_{a}}{dt} = -ka(T_{a}-T_{b})

Which we picked the sign of to make sure if T_{a} >T_{b}, that T will decrease.

Now, we remember the definition of specific heat, C_{a}=\frac{dU_{a}}{dT}, then

\frac{dU_{a}}{dt}=\frac{dU_{a}}{dT}*\frac{dT_{a}}{dt}=C*\frac{dT_{a}}{dt},

So our new Newton's law is \frac{dU_{a}}{dt} = -\frac{k_{a}}{C_{a}}(T_{a}-T_{b})= -k(T_{a}-T_{b})

And now we have to choose a T dependence for U. For Newton's law, we implicitly assumed U proportional to T, as is true for both the ideal gas and for metals from Dulong-Petit rule, so then we can express U=C*T, and separate variables for integration;

∫\frac{dU_{a}}{\frac{U_{a}}{C_{a}}-\frac{U_{b}}{C_{b}}}=∫-k*dt

\frac{Ln[{\frac{U_{a}}{C_{a}}-\frac{U_{b}}{C_{b}}}]}{\frac{1}{C_{a}}-\frac{\frac{dU_{b}}{dU_{a}}}{C_{b}}}=-k*t+c,

c integration constant for later. Now we employ energy conservation, so that
U_{a}+U_{b}=E, E constant. therefore 1+\frac{dU_{b}}{dU_{a}}=0, so our equation becomes;

Ln[{\frac{U_{a}}{C_{a}}-\frac{U_{b}}{C_{b}}}]=(\frac{1}{C_{a}}+\frac{1}{C_{b}})(-k*t+c)=(\frac{1}{C_{a}}+\frac{1}{C_{b}})(-k*t)+d

Exponentiate, and absorb the d as multiplicative integration constant. Add over U_{b}, multiply by C_{a}, and you get;

U_{a}=C_{a}*A*e^{(\frac{1}{C_{a}}+\frac{1}{C_{b}})(-k*t)}+\frac{C_{a}}{C_{b}}U_{b}

And to separate the coupled equations, we again use conservation of energy, so
U_{b}=E-U_{a}, add over the U term, factor out U, divide by coefficient, and;

U_{a}=\frac{C_{a}*A*e^{(\frac{1}{C_{a}}+\frac{1}{C_{b}})(-k*t)}+\frac{C_{a}}{C_{b}}E}{1+\frac{C_{a}}{C_{b}}}

And sub in U_{a}=C_{a}T_{a}, so divide whole equation by Ca,


T_{a}=\frac{A*e^{(\frac{1}{C_{a}}+\frac{1}{C_{b}})(-k*t)}+\frac{E}{C_{b}}}{1+\frac{C_{a}}{C_{b}}},

With E=C_{a}T_{a}+C_{b}T_{b}=C_{a}T_{a0}+C_{b}T_{b0}, since E same at all times.

Then we apply initial conditions, at t=0 T_{a}=T_{a0}=\frac{A+\frac{C_{a}T_{a0}+C_{b}T_{b0}}{C_{b}}}{1+\frac{C_{a}}{C_{b}}},

So A=T_{a0}-T_{b0} and we have our final form;



T_{a}=\frac{(T_{a0}-T_{b0})e^{(\frac{1}{C_{a}}+\frac{1}{C_{b}})(-k*t)}+\frac{C_{a}T_{a}+C_{b}T_{b}}{C_{b}}}{1+\frac{C_{a}}{C_{b}}}


And we check some limits for sanity; at t→∞,
T_{a}=\frac{C_{a}T_{a0}+C_{b}T_{b0}}{C_{a}+C_{b}},

So if C_{b} goes to 0, ie you get no heat from changing it's temperature, then T_{a}=T_{a0} ; it doesn't change temperature since there is no energy in the other system

If C_{b} goes to ∞, it takes infinite energy to change it's temperature, and we see by l'hospital's rule that T_{a}=T_{b0}; it raises to the unmovable temperature

And finally if both C's are equal, T_{a}=\frac{T_{a0}+T_{b0}}{2}; it reaches equilibrium at the average of the initial temperatures.

Nonlinear U dependences on T will need to be solved differently from the step listed as such, but for first order and most common systems this should work. Hope it helps.
 

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