All‐aluminum‐alloy ultrahigh vacuum system for a large‐scale electron–positron collider

1984 ◽  
Vol 2 (2) ◽  
pp. 1170-1175 ◽  
Author(s):  
Hajime Ishimaru
1986 ◽  
Vol 4 (3) ◽  
pp. 1762-1764 ◽  
Author(s):  
H. Ishimaru ◽  
T. Momose ◽  
K. Narushima ◽  
H. Mizuno ◽  
K. Kanazawa ◽  
...  

1986 ◽  
Vol 4 (6) ◽  
pp. 2515-2519 ◽  
Author(s):  
M. Miyamoto ◽  
Y. Sumi ◽  
S. Komaki ◽  
K. Narushima ◽  
H. Ishimaru

Vacuum ◽  
1968 ◽  
Vol 18 (12) ◽  
pp. 641-644 ◽  
Author(s):  
JL Robins ◽  
VNE Robinson

2011 ◽  
Vol 121-126 ◽  
pp. 325-329
Author(s):  
Bin Feng He

The FDM numerical simulation software View Cast system was employed to the counter-pressure casting of aluminum alloy large-scale thin-section casting. By analyzing the mold filling and solidification, the distribution of liquid fraction, temperature field were studied. The potential shrinkage defects were predicted to be formed at the top of the casting. A solution towards reducing such defects has been presented. The feeding capacity of the riser was improved. Analysis on the shrinkage proved that the improved riser is an effective method for reduction of defects.


2019 ◽  
Vol 28 (13) ◽  
pp. 1941011 ◽  
Author(s):  
K. M. Belotsky ◽  
E. A. Esipova ◽  
A. Kh. Kamaletdinov ◽  
E. S. Shlepkina ◽  
M. L. Solovyov

Here, we briefly review possible indirect effects of dark matter (DM) of the universe. It includes effects in cosmic rays (CR): first of all, the positron excess at [Formula: see text]500[Formula: see text]GeV and possible electron–positron excess at 1–1.5[Formula: see text]TeV. We tell that the main and least model-dependent constraint on such possible interpretation of CR effects goes from gamma-ray background. Even ordinary [Formula: see text] mode of DM decay or annihilation produces prompt photons (FSR) so much that it leads to contradiction with data on cosmic gamma-rays. We present our attempts to possibly avoid gamma-ray constraint. They concern with peculiarities of both space distribution of DM and their physics. The latter involves complications of decay/annihilation modes of DM, modifications of Lagrangian of DM-ordinary matter interaction and inclusion of mode with identical fermions in final state. In this way, no possibilities to suppress were found except, possibly, the mode with identical fermions. While the case of spatial distribution variation allows achieving consistency between different data. Also, we consider stable form of DM which can interact with baryons. We show which constraint such DM candidate can get from the damping effect in plasma during large-scale structure (LSS) formation in comparison with other existing constraints.


1981 ◽  
Vol 28 (3) ◽  
pp. 3320-3322 ◽  
Author(s):  
Hajime Ishimaru ◽  
Gen'ichi Horikoshi ◽  
Yoshitaka Kimura
Keyword(s):  

Vacuum ◽  
1968 ◽  
Vol 18 (4) ◽  
pp. 232-232
Author(s):  
VARIANASSOCIATESVACUUMDIVISIO

Sign in / Sign up

Export Citation Format

Share Document