Date of Award
1973
Document Type
Thesis
Publication Status
Version of Record
Submission Date
October 2026
Abstract
The time history of the abundances of 13 nuclei and the thermodynamic and hydrodynamic variables in the burning zone of a detonation wave were numerically followed in detail by coupling a nuclear reaction network to the Rankine-Hugoniot relations and accurate equations of state. A number of computations were performed for material with initial densities and temperatures in the range 10^9 < p < 10^11(g/cm^3) and 3 x 10^8 K, respectively, and compositions consisting of C^12 and O^16, and O^16, Mg^24, and Si^28. From such computations it is concluded that: (1) the nuclear rea-tion rate doubling timescale approximation gives an accurate nuclear burning timescale, (2) the propagation of a detonation wave fueled by O^16 at very high densities is virtually assured, (3) the correct energy release is obtained assuming nuclear statistical equilibrium behind the detonation wave, and this latter assumption is good, (4) the Chapman- Jouguet hypothesis is adequate in spite of the fact that the actual form of the detonation wave is more likely that of a weak detonation.
Extent
97 p.
Recommended Citation
MARROQUIN, ADRIAN, "SOME PROPERTIES OF DETONATION WAVES IN DENSE STELLAR MATERIAL" (1973). Electronic Theses and Dissertations 1970 - 1979. 228.
https://digitalcommons.fau.edu/etd_general_2/228
Identifier
FADT13559
Comments
Thesis (M.S.)--Florida Atlantic University, 1973.|Thesis (M.S.)--Florida Atlantic University, 1973.