Isentropic relations: Difference between revisions
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{{NumEqn|<math> | {{NumEqn|<math> | ||
de=Tds-pd\left(\frac{1}{\rho}\right) | de=Tds-pd\left(\frac{1}{\rho}\right) | ||
</math>|eq-first-law-b}} | </math>|label=eq-first-law-b}} | ||
Enthalpy is defined as: <math>h=e+p/\rho</math> and thus | Enthalpy is defined as: <math>h=e+p/\rho</math> and thus | ||
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{{NumEqn|<math> | {{NumEqn|<math> | ||
dh=de+pd\left(\frac{1}{\rho}\right)+\left(\frac{1}{\rho}\right)dp | dh=de+pd\left(\frac{1}{\rho}\right)+\left(\frac{1}{\rho}\right)dp | ||
</math>|eq-dh}} | </math>|label=eq-dh}} | ||
Eliminate <math>de</math> in {{EquationNote|eq-first-law-b}} using {{EquationNote|eq-dh}} | Eliminate <math>de</math> in {{EquationNote|label=eq-first-law-b}} using {{EquationNote|label=eq-dh}} | ||
{{NumEqn|<math> | {{NumEqn|<math> | ||
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{{NumEqn|<math> | {{NumEqn|<math> | ||
ds=C_p\frac{dT}{T}-R\frac{dp}{p} | ds=C_p\frac{dT}{T}-R\frac{dp}{p} | ||
</math>|eq-ds}} | </math>|label=eq-ds}} | ||
Integrating {{EquationNote|eq-ds}} gives | Integrating {{EquationNote|eq-ds}} gives | ||
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{{NumEqn|<math> | {{NumEqn|<math> | ||
s_2-s_1=\int_1^2 C_p\frac{dT}{T}-R\ln\left(\frac{p_2}{p_1}\right) | s_2-s_1=\int_1^2 C_p\frac{dT}{T}-R\ln\left(\frac{p_2}{p_1}\right) | ||
</math>|eq-ds-b}} | </math>|label=eq-ds-b}} | ||
For a calorically perfect gas, <math>C_p</math> is constant (not a function of temperature) and can be moved out from the integral and thus | For a calorically perfect gas, <math>C_p</math> is constant (not a function of temperature) and can be moved out from the integral and thus | ||
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{{NumEqn|<math> | {{NumEqn|<math> | ||
s_2-s_1=C_p\ln\left(\frac{T_2}{T_1}\right)-R\ln\left(\frac{p_2}{p_1}\right) | s_2-s_1=C_p\ln\left(\frac{T_2}{T_1}\right)-R\ln\left(\frac{p_2}{p_1}\right) | ||
</math>|eq-ds-c}} | </math>|label=eq-ds-c}} | ||
An alternative form of {{EquationNote|eq-ds-c}} is obtained by using <math>de=C_v dT</math> in {{EquationNote|eq-first-law-b}}, which gives | An alternative form of {{EquationNote|label=eq-ds-c}} is obtained by using <math>de=C_v dT</math> in {{EquationNote|label=eq-first-law-b}}, which gives | ||
{{NumEqn|<math> | {{NumEqn|<math> | ||
s_2-s_1=\int_1^2 C_v\frac{dT}{T}-R\ln\left(\frac{\rho_2}{\rho_1}\right) | s_2-s_1=\int_1^2 C_v\frac{dT}{T}-R\ln\left(\frac{\rho_2}{\rho_1}\right) | ||
</math>|eq-ds-d}} | </math>|label=eq-ds-d}} | ||
Again, for a calorically perfect gas, we get | Again, for a calorically perfect gas, we get | ||
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{{NumEqn|<math> | {{NumEqn|<math> | ||
s_2-s_1=C_v\ln\left(\frac{T_2}{T_1}\right)-R\ln\left(\frac{\rho_2}{\rho_1}\right) | s_2-s_1=C_v\ln\left(\frac{T_2}{T_1}\right)-R\ln\left(\frac{\rho_2}{\rho_1}\right) | ||
</math>|eq-ds-e}} | </math>|label=eq-ds-e}} | ||
=== Isentropic Relations === | === Isentropic Relations === | ||
Adiabatic and reversible processes, i.e., isentropic processes implies <math>ds=0</math> and thus {{EquationNote|eq-ds-c}} reduces to | Adiabatic and reversible processes, i.e., isentropic processes implies <math>ds=0</math> and thus {{EquationNote|label=eq-ds-c}} reduces to | ||
{{NumEqn|<math> | {{NumEqn|<math> | ||
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{{NumEqn|<math> | {{NumEqn|<math> | ||
\frac{p_2}{p_1}=\left(\frac{T_2}{T_1}\right)^{\gamma/(\gamma-1)} | \frac{p_2}{p_1}=\left(\frac{T_2}{T_1}\right)^{\gamma/(\gamma-1)} | ||
</math>|eq-isentropic-a}} | </math>|label=eq-isentropic-a}} | ||
In the same way, {{EquationNote|eq-ds-e}} gives | In the same way, {{EquationNote|label=eq-ds-e}} gives | ||
{{NumEqn|<math> | {{NumEqn|<math> | ||
\frac{\rho_2}{\rho_1}=\left(\frac{T_2}{T_1}\right)^{1/(\gamma-1)} | \frac{\rho_2}{\rho_1}=\left(\frac{T_2}{T_1}\right)^{1/(\gamma-1)} | ||
</math>|eq-isentropic-b}} | </math>|label=eq-isentropic-b}} | ||
Revision as of 19:55, 29 March 2026
First law of thermodynamics
First law of thermodynamics:
| (Eq. 1.6) |
For a reversible process: and
| (Eq. 1.7) |
Enthalpy is defined as: and thus
| (Eq. 1.8) |
Eliminate in (Eq. 1.7) using (Eq. 1.8)
| (Eq. 1.9) |
| (Eq. 1.10) |
Using and the equation of state , we get
| (Eq. 1.11) |
Integrating (Eq. 1.11) gives
| (Eq. 1.12) |
For a calorically perfect gas, is constant (not a function of temperature) and can be moved out from the integral and thus
| (Eq. 1.13) |
An alternative form of (Eq. 1.13) is obtained by using in (Eq. 1.7), which gives
| (Eq. 1.14) |
Again, for a calorically perfect gas, we get
| (Eq. 1.15) |
Isentropic Relations
Adiabatic and reversible processes, i.e., isentropic processes implies and thus (Eq. 1.13) reduces to
| (Eq. 1.16) |
| (Eq. 1.17) |
In the same way, (Eq. 1.15) gives
| (Eq. 1.18) |
Eqn. (Eq. 1.17) and Eqn. (Eq. 1.18) constitutes the isentropic relations
| (Eq. 1.19) |