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torsdag 28 augusti 2025

Temperature as Absolute Control of Radiative Heat Transfer

This is a follow up of this post recalling the Faustian deal made by Max Planck in 1900 when presenting his law of black body radiation as an icon of modern physics named Planck's Law.  

Continuing the discussion with chatGPT we come to an agreement that temperature difference, positive or negative, is Natures control mechanism to keep a system stable over time under radiative heat transfer with an environment, like your house and the Earth's climate system. The temperature is measured on an absolute Kelvin scale available to all bodies allowing detection of positive or negative temperature difference to steer the exchange of heat energy. Equal temperature then gives zero exchange as radiative equilibrium. 

Unfortunately there is a different view sold by climate scientists as reason for climate alarm, which suggests the opposite control mechanism, namely that the temperature of the Earth is controled by differences in incoming and outgoing radiation with in particular small differences in incoming/outgoing radiation generating big differences in temperature possibly in a run-away greenhouse effect. Very alarming.

But physical bodies do not carry an absolute scale allowing comparison of incoming and outgoing radiation, like the absolute scale for temperature, more precisely they carry no counter for incoming and outgoing photons as proclaimed carriers of heat energy. 

In particular, there is no absolute Planck-Stefan-Boltzmann Law $R=\sigma T^4$ stating outgoing radiation from a body of temperature $T$ independent of environment as version 1. in the earlier post. Not physics!

Nevertheless such a law is used in models (Schwarzschild) of radiative heat transfer in the atmosphere playing with gross quantities of incoming/outgoing radiative heat transfer prone to instability. The accuracy of these models is no better than say $2-3$ Watts per m2, while alarming global heating is connected to variations of incoming/outgoing radiation of the same size. The result is alarm as a result of unphysical unstable control. This is like a hen from a feather.

If temperature is allowed to carry out its physical control to stabilise climate, here is no reason for alarm. Puh!

This analysis shows that temperature is measured via Wien's Displacement Law expressed as a high-frequency-cut-off scaling with temperature giving a body of higher temperature access to higher-frequencies aloowing transfer of heat to a body of lower temperature. The cut-off can be connected to the precision available in the underlying atomic wave physics of different frequencies.


onsdag 24 april 2024

How to Measure Temperature

Measuring temperature accurately is a delicate procedure.

This is a comment to the discussion in recent posts of the proclaimed perfect blackbody spectrum of Cosmic Microwave Background CMB radiation with temperature 2.725 K.  

You can measure your body temperature by body contact with a quicksilver thermometer or at distance by an infrared thermometer. Both work on a principle of thermal equilibrium between source and thermometer sensor as a stable state over time. Your body is assigned the temperature recorded by the thermometer. 

Temperature can be seen as a measure of energy in the form of heat energy or vibrational energy of a vibrating system like an atomic lattice as the generator of radiation as radiative heat transfer.

Computational Blackbody Radiation offers a new analysis of radiative heat transfer using classical wave mechanics as a deterministic form of Planck's analysis based on statistics of quanta. The basic element of the analysis is a radiation spectrum from a vibrating atomic lattice: 

  • $E(\nu ,T)=\gamma T\nu^2$ for $\nu \le \frac{T}{h}$        (1a)
  • $E(\nu ,T)= 0$ for $\nu >\frac{T}{h}$                               (1b)
where $\nu$ is frequency on an absolute time scale, $T$ is temperature on a lattice specific energy scale, $\gamma$ and $h$ are lattice specific parameters and $\frac{T}{h}$ is a corresponding high-frequency cut-off frequency setting a upper limit to frequencies being radiated. Here a common temperature $T$ for all frequencies expresses thermal equilibrium between frequencies. 

It is natural to define a blackbody BB to have radiation spectrum of the form (1) with maximal $\gamma$ and high-frequency cut-off and to use this as a universal thermometer measuring the temperature of different bodies by thermal equilibrium. 

Consider then a vibrating atomic lattice A with spectrum according (1)-(2) with different parameters $\bar\gamma <\gamma$ and $\bar h >h$ and different temperature scale $\bar T$ to be in equilibrium with the universal thermometer. The radiation law (1) then implies assuming that A is perfectly reflecting for frequencies above its own cut-off:
  • $\bar\gamma \bar T = \gamma T$                                         (2)
to serve as the connection between the temperature scales of BB and A. This gives (1) a form of universality with a universal $\gamma$ reflecting the use of a BB as a universal thermometer.

In reality the abrupt cut-off after at radiation maximum is replaced by a gradual decrease to zero over some frequency range as a case-specific post-max part of the spectrum.  A further case-specific element is non-perfect reflectivity above cut-off. Thermal equilibrium according to (2) is thus an ideal case.  

In particular, different bodies at the same distance to the Sun can take on different temperatures in thermal equilibrium with the Sun. Here the high-frequency part of the spectrum comes in as well as the route from non-equilibrium to equilibrium. 

Why CMB can have a perfect blackbody spectrum is hidden in the intricacies of the sensing. It may well reflect man-made universality.