scholarly journals Thermally Enhanced Cable Insulation for the Nb-Ti High Luminosity LHC Inner Triplet Model

2012 ◽  
Vol 22 (3) ◽  
pp. 7700404-7700404 ◽  
Author(s):  
P. P. Granieri ◽  
P. Fessia ◽  
D. Richter ◽  
D. Tommasini
1999 ◽  
Vol 524 (1) ◽  
pp. 379-393 ◽  
Author(s):  
Nancy Remage Evans ◽  
Kenneth Carpenter ◽  
Richard Robinson ◽  
Derck Massa ◽  
Glenn M. Wahlgren ◽  
...  
Keyword(s):  

Author(s):  
Xuefeng Zhao ◽  
Yincheng Gao ◽  
Futao Jin ◽  
Yuxin Lu ◽  
Wei Duan ◽  
...  
Keyword(s):  

Author(s):  
S. A. Antipov ◽  
N. Biancacci ◽  
J. Komppula ◽  
E. Métral ◽  
B. Salvant ◽  
...  

2021 ◽  
Vol 11 (11) ◽  
pp. 4722
Author(s):  
Botan Wang ◽  
Xiaolong Chen ◽  
Yi Wang ◽  
Dong Han ◽  
Baohong Guo ◽  
...  

This work reports the latest observations on the behavior of two Multigap Resistive Plate Chambers (MRPC) under wide high-luminosity exposures, which motivate the development and in-beam test of the sealed MRPC prototype assembled with low-resistive glass. The operation currently being monitored, together with previous simulation results, shows the impact of gas pollution caused by avalanches in gas gaps, and the necessity to shrink the gas-streaming volume. With the lateral edge of the detector sealed by a 3D-printed frame, a reduced gas-streaming volume of ~170 mL has been achieved for a direct gas flow to the active area. A high-rate test of the sealed MRPC prototype shows that, ensuring a 97% efficiency and 70 ps time resolution, the sealed design results in a stable operation current behavior at a counting rate of 3–5 kHz/cm2. The sealed MRPC will become a potential solution for future high luminosity applications.


1983 ◽  
Vol 6 ◽  
pp. 648-648
Author(s):  
J.B. Hutchings

IUE has been used to study 11 high luminosity X-ray binaries, of which 3 are in the Magellanic Clouds. In the supergiant systems, X-ray ionisation bubbles have been found in most cases, leading to a greater understanding of the winds and accretion processes. Further studies of precessing objects such as LMC X-4 with IUE and ST are clearly of considerable interest, relating to X-ray heating and blanketing. Detailed studies of the Cyg X-l ionisation bubble may resolve the long standing puzzle of its orbit inclination and masses. UV continua have furnished valuable information on extinction, temperatures and luminosities, and the presence of non-stellar (i.e. disk) luminosity. Here too, more detailed studies are clearly indicated for the future. A unique object of interest is the LMC transient 0538-66 whose UV spectrum has quasarlike lines and luminosity which varies oppositely to the visible. This may be a case of supercritical accretion generating an optically thick shell (“disk”) about the pulsar.


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