Effects of temperature in binary collision simulations of high-energy displacement cascades

1982 ◽  
Vol 108-109 ◽  
pp. 62-66 ◽  
Author(s):  
H.L. Heinisch
Author(s):  
Mohammad Abu-Shams ◽  
Jeffery Moran ◽  
Ishraq Shabib

Abstract The effects of radiation damage on bcc tungsten with preexisting helium and hydrogen clusters have been investigated in a high-energy environment via a comprehensive molecular dynamics simulation study. This research determines the interactions of displacement cascades with helium and hydrogen clusters integrated into a tungsten crystal generating point defect statistics. Helium or hydrogen clusters of atoms~0.1% of the total number of atoms have been randomly distributed within the simulation model and primary knock-on-atom (PKA) energies of 2.5, 5, 7.5 and 10 keV have been used to generate displacement cascades. The simulations quantify the extent of radiation damage during a simulated irradiation cycle using the Wigner-Seitz point defect identification technique. The generated point defects in crystals with and without pre-existing helium/hydrogen defects exhibit a power relationship with applied PKA energy. The point defects are classified by their atom type, defect type, and distribution within the irradiated model. The presence of pre-existing helium and hydrogen clusters significantly increases the defects (5 - 15 times versus pure tungsten models). The vacancy composition is primarily tungsten (e. g., ~70% at 2.5 keV) in models with pre-existing helium, but the interstitials are primarily He (e. g., ~89% at 10 keV). On the other hand, models with pre-existing hydrogen have a vacancy composition that is primarily tungsten (more than 90% irrespective of PKA energy), and the interstitial composition is more balanced between tungsten (average 46%) and hydrogen (average 54%) interstitials across the PKA range. The distribution of the atoms reveals that the tungsten point defects prefer to reside close to the position of cascade initiation, but helium or hydrogen defects reside close to the positions where clusters are built.


2015 ◽  
Vol 456 ◽  
pp. 1-6 ◽  
Author(s):  
Yinbin Miao ◽  
Benjamin Beeler ◽  
Chaitanya Deo ◽  
Michael I. Baskes ◽  
Maria A. Okuniewski ◽  
...  

2019 ◽  
Vol 206 ◽  
pp. 04001
Author(s):  
Thomas A. Trainor

The PYTHIA Monte Carlo (PMC) has been applied broadly to simulations of high-energy p-p and p- $ \bar p $ collisions. The PMC is based on several assumptions, such as that most hadrons result from jet production (multiple par-ton interactions or MPIs), that p-p centrality is relevant and that color reconnection (CR) strongly influences fragmentation to jets. An alternative description is provided by the two-component (soft + hard) model (TCM) of hadron production. TCM analysis of p-Pb ensemble-mean-pt data reveals centrality trends quite different from those estimated via a geometric Glauber model based on the eikonal approximation. Glauber estimates of binary-collision number are three times TCM estimates. Detailed study of p-Pb data conflicts with a basic Glauber assumption – that a projectile proton may interact simultaneously with multiple target nucleons. Instead, in both p-p and p-A collisions, a p-N collision once initiated is exclusive of other possible interactions (during that collision), and within the collision any pair of participant partons may interact –a p-N collision is thus “all or nothing.” In this presentation the PMC is challenged by an assortment of contradictory data, and evidence for p-N exclusivity is reviewed to make a case for the “preoccupied proton” of the title.


Author(s):  
Muhammad Uzair ◽  
Syed Umair Hassan Kazmi ◽  
Muhammad Uzair Yousuf ◽  
Syed Asad Ali Zaidi

To incorporate solar energy efficiently into a country, it is needed to know the optimal tilt and azimuth angle of the solar collectors' location. Also, to build a solar park, it is necessary to know the most suitable and high-energy generating place inside a country, thus saving time and money. This study analyzed collector geometry for Karachi in particular and Pakistan in general. Karachi has the potential of 339.36 kW-hr/m2/annum energy at an annually optimal fixed tilt of 26°. In case collector geometry had to be changed in Karachi, a range of 40° azimuth angle and 20° tilt angle from its maximum value is available. The power produced in this case would only have a difference of 1%. Optimal yearly and monthly tilt of most of the locations of Pakistan (300+) were calculated. Through them, it was revealed that the Optimal Tilt of Pakistan follows the value of latitude closely. Generally, changing the tilt angle monthly is recommended for areas that produce more energy, while fixed annual tilt could be suitable for low energy-producing regions. Effects of temperature were also incorporated while finding the energy produced by the photovoltaic (PV) panels.


1984 ◽  
Vol 122 (1) ◽  
pp. K17-K21 ◽  
Author(s):  
A. I. Melker ◽  
S. N. Romanov

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