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Classical physics appears as a limit of quantum physics if all "actions" (quantities of dimension energy * time, momentum * length, or angular momentum) are much larger than ħ. Conversely, you can also formally set ħ=0 to get classical results from quantum formulae. This means that effects that are proportional to some power of ħ cannot be explained classically, and instead are "a quantum thing".
 
Classical physics appears as a limit of quantum physics if all "actions" (quantities of dimension energy * time, momentum * length, or angular momentum) are much larger than ħ. Conversely, you can also formally set ħ=0 to get classical results from quantum formulae. This means that effects that are proportional to some power of ħ cannot be explained classically, and instead are "a quantum thing".
  
'''R<sub>e</sub>: Someone needs to do a lot of tedious numerical work; hopefully it's not you'''  The {{w|Reynolds number}} (which is usually denoted by "Re," not "R<sub>e</sub>" as it appears in the comic) is the most important dimensionless group in fluid mechanics. Named for Osborne Reynolds, Re characterizes the relative sizes of inertial and viscous effects in a moving fluid. Large values of Re are indicative of turbulent flow, which cannot usually be retrieved analytically, and so numerical modeling is necessary. Accurate numerical studies of high-Reynolds-number flows are notoriously difficult to create and program.
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'''Rₑ: Someone needs to do a lot of tedious numerical work; hopefully it's not you'''  The {{w|Reynolds number}} (which is usually denoted by "Re," not "R<sub>e</sub>" as it appears in the comic) is the most important dimensionless group in fluid mechanics. Named for Osborne Reynolds, Re characterizes the relative sizes of inertial and viscous effects in a moving fluid. Large values of Re are indicative of turbulent flow, which cannot usually be retrieved analytically, and so numerical modeling is necessary. Accurate numerical studies of high-Reynolds-number flows are notoriously difficult to create and program.
  
Alternatively, R<sub>e</sub> could stand for electronic {{w|transition dipole moment}} in a molecule. This appears in quantum-mechanical calculations of transition probabilities and also includes a lot of unpleasant numerical work. R<sub>e</sub> is also a term used for the radius of the Earth at mean sea level, though this is not necessarily a complex term in and of itself.
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Alternatively, Rₑ could stand for electronic {{w|transition dipole moment}} in a molecule. This appears in quantum-mechanical calculations of transition probabilities and also includes a lot of unpleasant numerical work. Rₑ is also a term used for the radius of the Earth at mean sea level, though this is not necessarily a complex term in and of itself.
  
Another alternative is that R<sub>e</sub> could refer to Relative Error, a measurement of precision or accuracy.  Used often in the analysis of scientific data and numerical analysis.
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Another alternative is that Rₑ could refer to Relative Error, a measurement of precision or accuracy.  Used often in the analysis of scientific data and numerical analysis.
  
'''(T<sub>a</sub><sup>4</sup> - T<sub>b</sub><sup>4</sup>): You are at risk of skin burns'''  The {{w|Stefan-Boltzmann law}} says that a perfectly absorbing ("black body") source emits electromagnetic radiation with a power per unit area of σT<sup>4</sup>, where σ is a known constant and T is the absolute temperature. The quantity (T<sub>a</sub><sup>4</sup> – T<sub>b</sub><sup>4</sup>) thus appears in any calculation of purely radiative energy transfer between two bodies, one at temperature T<sub>a</sub> and the other at T<sub>b</sub>. When the radiative transfer is large enough to be the most important form of heat interchange, it is normally also large enough to sear the skin with thermal or ultraviolet burns.
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'''(T<sub>a</sub>- T<sub>b</sub>): You are at risk of skin burns'''  The {{w|Stefan-Boltzmann law}} says that a perfectly absorbing ("black body") source emits electromagnetic radiation with a power per unit area of σT<sup>4</sup>, where σ is a known constant and T is the absolute temperature. The quantity (T<sub>a</sub><sup>4</sup> – T<sub>b</sub><sup>4</sup>) thus appears in any calculation of purely radiative energy transfer between two bodies, one at temperature T<sub>a</sub> and the other at T<sub>b</sub>. When the radiative transfer is large enough to be the most important form of heat interchange, it is normally also large enough to sear the skin with thermal or ultraviolet burns.
  
'''N<sub>A</sub>: You are probably about to make an incredibly dangerous arithmetic error'''  N<sub>A</sub>, or {{w|Avogadro's number}}, is the number of molecules in a mole of a substance, approximately the number of carbon atoms in exactly 12 grams of carbon-12. This is an enormous number, exactly 6.022 140 76 × 10<sup>23</sup>, or 602 214 076 000 000 000 000 000. Working with N<sub>A</sub>, it is easy to accidentally divide by it instead of multiplying or vice versa, leading to erroneous and nonsensical answers such as ~10<sup>-23</sup> molecules (even though you can't have less than 1 whole molecule) or ~10<sup>46</sup> moles (>10<sup>43</sup> to 10<sup>45</sup> kilograms, depending on the chemical) of a substance.
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'''N<sub>A</sub>: You are probably about to make an incredibly dangerous arithmetic error'''  N<sub>A</sub>, or {{w|Avogadro's number}}, is the number of molecules in a mole of a substance, approximately the number of carbon atoms in exactly 12 grams of carbon-12. This is an enormous number, exactly 6.022 140 76 × 10²³, or 602 214 076 000 000 000 000 000. Working with N<sub>A</sub>, it is easy to accidentally divide by it instead of multiplying or vice versa, leading to erroneous and nonsensical answers such as ~10<sup>-23</sup> molecules (even though you can't have less than 1 whole molecule) or ~10<sup>46</sup> moles (>10<sup>43</sup> to 10<sup>45</sup> kilograms, depending on the chemical) of a substance.
  
 
'''µm: Careful, that equipment is expensive'''  {{w|Micrometre|Micrometer}}s are a very small unit of distance. Micrometers are commonly used to measure wavelengths in the infrared, and infrared detectors are very expensive, compared with visible wavelength counterparts. Of course, micrometers are used as a measurement of distance in other contexts, but any distance-measuring device capable of accurately measuring micrometer distances would also be expensive. Similarly, tools used to create or calibrate items within micrometer tolerances can also be expensive.
 
'''µm: Careful, that equipment is expensive'''  {{w|Micrometre|Micrometer}}s are a very small unit of distance. Micrometers are commonly used to measure wavelengths in the infrared, and infrared detectors are very expensive, compared with visible wavelength counterparts. Of course, micrometers are used as a measurement of distance in other contexts, but any distance-measuring device capable of accurately measuring micrometer distances would also be expensive. Similarly, tools used to create or calibrate items within micrometer tolerances can also be expensive.

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