Energy Generation: Nuclear Energy

Author(s):  
Dorothy Duffy
Author(s):  
Ja. Nowotny ◽  
T. Hoshino ◽  
J. Dodson ◽  
A. J. Atanacio ◽  
M. Ionescu ◽  
...  

2008 ◽  
Vol 49 (4) ◽  
pp. 1069-1072 ◽  
Author(s):  
Liu Hong-Lin ◽  
Luo Zhi-Quan ◽  
Liu Jing-Jing ◽  
Lai Xiang-Jun

2018 ◽  
pp. 31-50
Author(s):  
PETER D. MacD. PARKER ◽  
CLAUS E. ROLFS

2018 ◽  
Vol 68 (3) ◽  
pp. 167-182 ◽  
Author(s):  
Saha Sabhasachi ◽  
Roy Koushik ◽  
Roy Souvik ◽  
Rahman Md. Asfakur ◽  
Hasan Md. Zahid

AbstractIn the present world, nuclear energy is a must need for various purposes. The main cause of nuclear energy is because of the increasing energy demand, which is not possible to provide by using convenient energy generation. Bangladesh is a lower income country and the energy sector is not so developed here though there is a very high demand for energy. Rooppur Nuclear Power Plant is the only one nuclear generation plant which can provide this kind of huge energy within a very short time. This paper mainly depicts the ins and outs of this plant and discusses it’s feasibility in Bangladesh. It also focuses on the worlds various power generation methods and comprises it with nuclear energy generation. A detailed technical brief is presented in this paper along with advantages, location selection, financial and environmental impacts. This will help researchers to do further researches about nuclear energy in Bangladesh.


2020 ◽  
Vol 2020 (3) ◽  
Author(s):  
Akira Dohi ◽  
Masa-aki Hashimoto ◽  
Rio Yamada ◽  
Yasuhide Matsuo ◽  
Masayuki Y Fujimoto

Abstract We investigate X-ray bursts during the thermal evolution of an accreting neutron star that corresponds to the X-ray burster GS 1826$-$24. Physical quantities of the neutron star are included using an equation of state below and above the nuclear matter density. We adopt an equation of state and construct an approximate network that saves computational time and calculates nuclear energy generation rates accompanying the abundance evolutions. The mass and radius of the neutron star are found by solving the stellar evolution equations from the center to the surface; this involves necessary information such as the nuclear energy generation in accreting layers, heating from the crust, and neutrino emissions inside the stellar core. We reproduce the light curve and recurrence time of the X-ray burst from GS 1826$-$24 within the standard deviation of 1$\sigma$ for the assumed accretion rate, metallicity, and equation of state. It is concluded that the observed recurrence time is consistent with the theoretical model with metallicity of the initial CNO elements $Z_{\rm CNO} = 0.01$. We suggest that the nuclear reaction rates responsible for the $rp$-process should be examined in detail, because the rates may change the shape of the light curve and our conclusion.


1966 ◽  
Vol 20 (3) ◽  
pp. 227-234
Author(s):  
A. M. Petros'yants

Author(s):  
R.A. Ploc

Zirconium-based alloys, namely Zircaloy-2 and Zr-2½ wt% Nb are heavily used in the CANDU (Canadian Deuterium and Uranium) system of nuclear energy generation. Although corrosion in heavy water at about 573 K is not a design limiting concern, corrosion does produce hydrogen which can result in hydride formation that embrittles reactor components. About twenty years ago, an effort was initiated at the Chalk River Nuclear laboratories (CRNL) designed to develop an understanding of the physical structure of the oxide films first, on reactor-grade zirconium, then on dilute zirconium alloys, and finally, on reactor materials. A great deal of this investigative work has been performed in the TEM, SEM and in a SAM.


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