Difference between revisions of "User:Tohline/Appendix/Equation templates"
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I: §10.2<br /> (10.1) | |||
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§II.1<br /> (1) <br />[http://www.vistrails.org/index.php/User:Tohline/Appendix/Equation_templates#C67note01 Note] | |||
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I: §5.6<br /> (5.91) | |||
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Key Parallel | Key Parallel Reference Texts (spanning 5+ decades) | ||
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* [C67] Chandrasekhar, S. 1967 (originally, 1939) An Introduction to the Study of Stellar Structure (New York: Dover) | * [C67] Chandrasekhar, S. 1967 (originally, 1939) An Introduction to the Study of Stellar Structure (New York: Dover) | ||
** <span id="C67note01">EQ_EOSideal0A</span> — In C67, the ideal gas equation of state is written in terms of the specific volume {{User:Tohline/Math/VAR_SpecificVolume01}}, instead of the mass density {{User:Tohline/Math/VAR_Density01}}; also, it is assumed that {{User:Tohline/Math/MP_MeanMolecularWeight}} = 1. | |||
* [LL75] Laundau, L. D. & Lifshitz, E. M. 1975 (originally, 1959), Fluid Mechanics (New York: Pergamon Press) | * [LL75] Laundau, L. D. & Lifshitz, E. M. 1975 (originally, 1959), Fluid Mechanics (New York: Pergamon Press) | ||
* [BT87] Binney, J. & Tremaine, S. 1987, Galactic Dynamics (Princeton, NJ: Princeton University Press) | * [BT87] Binney, J. & Tremaine, S. 1987, Galactic Dynamics (Princeton, NJ: Princeton University Press) |
Revision as of 19:28, 24 January 2010
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Key Equations
To insert a given equation into any Wiki document, type ... |
Parallel References (Section & Eq. #) |
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Template_Name |
Resulting Equation |
C67 |
LL75 |
BT87 |
KW94 |
P00 |
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I: §8.5 |
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I: §8.5 |
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I: §8.5 |
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I: §10.2 |
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<math>~P = n_g k T</math> |
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§II.1 |
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I: §5.6 |
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<math>~P = (\gamma_\mathrm{g} - 1)\epsilon \rho </math> |
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Key Parallel Reference Texts (spanning 5+ decades)
- [C67] Chandrasekhar, S. 1967 (originally, 1939) An Introduction to the Study of Stellar Structure (New York: Dover)
- EQ_EOSideal0A — In C67, the ideal gas equation of state is written in terms of the specific volume <math>~V</math>, instead of the mass density <math>~\rho</math>; also, it is assumed that <math>~\bar{\mu}</math> = 1.
- [LL75] Laundau, L. D. & Lifshitz, E. M. 1975 (originally, 1959), Fluid Mechanics (New York: Pergamon Press)
- [BT87] Binney, J. & Tremaine, S. 1987, Galactic Dynamics (Princeton, NJ: Princeton University Press)
- [KW94] Kippenhahn, R. & Weigert, A. 1994, Stellar Structure and Evolution (New York: Springer-Verlag)
- [P00] Padmanabhan, T. 2000, Theoretical Astrophysics. Volume I: Astrophysical Processes (Cambridge: Cambridge University Press); and Padmanabhan, T. 2001, Theoretical Astrophysics. Volume II: Stars and Stellar Systems (Cambridge: Cambridge University Press)
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