New polytropic model to predict the performance of beta and gamma type Stirling engine

Energy ◽  
2017 ◽  
Vol 128 ◽  
pp. 62-76 ◽  
Author(s):  
Ruijie Li ◽  
Lavinia Grosu ◽  
Wei Li
2021 ◽  
Vol 313 ◽  
pp. 08006
Author(s):  
Josef Frauscher ◽  
Franz Diermaier ◽  
Hans-Jürgen Brandt ◽  
Michael Gschwendtner

Since 2001, Frauscher Thermal Motors have been conducting research in the field of thermodynamic machines, in particular Stirling engines of various types. One important development step is the invention of a Stirling engine in an alphagamma® configuration. In this configuration, the expansion piston is designed as a differential piston with its ring surface connected to the cold volume. In this paper, the design advantages of the alphagamma® configuration in comparison with a traditional alpha configuration are shown analytically by using a polytropic model as a modification of the ideal adiabatic analysis. The findings were confirmed by also simulating the proposed alphagamma® configuration in a Sage model which was validated against experimental data with very good agreement. The results of both methods show that the counter-productive compression work can be reduced to almost zero – which makes the compression piston a displacer and explains the name alphagamma® – with the expansion work also reduced for the same net work output. As a consequence, the forces on the pistons, and thus, on the bearings can be significantly reduced, also leading to smaller piston side-loads, less friction and wear. The combination of all advantages allows the design of a mechanically sound and inexpensive machine.


Author(s):  
Daniele Menniti ◽  
Anna Pinnarelli ◽  
Nicola Sorrentino ◽  
Giuseppe Barone ◽  
Giovanni Brusco ◽  
...  

Author(s):  
T. Nomaguchi ◽  
T. Suganami ◽  
M. Fujiwara ◽  
M. Sakai ◽  
T. Koda ◽  
...  

Author(s):  
Felipe Pinheiro Maia ◽  
Nícolas M. F. T. S. Araújo ◽  
Gabriel Ivan Medina Tapia

2016 ◽  
Vol 15 (1) ◽  
pp. 133-141
Author(s):  
Ramla Gheith ◽  
Fethi Aloui ◽  
Sassi Ben Nasrallah

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