Mixed shock model for multi-state weighted k-out-of-n: F systems with degraded resistance against shocks

Author(s):  
Xiaoyue Wang ◽  
Xian Zhao ◽  
Congshan Wu ◽  
Siqi Wang
Keyword(s):  
1984 ◽  
Vol 13 (1) ◽  
pp. 22-25 ◽  
Author(s):  
Robert C Jorden ◽  
Ernest E Moore ◽  
John A Marx ◽  
Benjamin Honigman ◽  
Barry Simon

Cryobiology ◽  
2020 ◽  
Vol 97 ◽  
pp. 276
Author(s):  
Olena Chabanenko ◽  
Natalya Yershova ◽  
Natalia Shpakova
Keyword(s):  

2014 ◽  
Vol 16 (2) ◽  
pp. 70-75 ◽  
Author(s):  
Rie Nishikata ◽  
Naho Kato ◽  
Kouichi Hiraiwa

1990 ◽  
Vol 22 (1) ◽  
pp. 251-253 ◽  
Author(s):  
Yuedong Wang ◽  
Jinhua Cao

Two kinds of multidimensional IFR distribution are defined by using a partial order in Rn+, which is derived from a non-negative, strictly increasing function in Rn+. Some closure properties under operations and an application to a shock model are discussed.


2006 ◽  
Vol 29 (5) ◽  
pp. 1015-1021 ◽  
Author(s):  
Hiroyasu Hozumi ◽  
Yoshiyuki Adachi ◽  
Taisuke Murakami ◽  
Noriko N. Miura ◽  
Naohito Ohno

2016 ◽  
Vol 2016 ◽  
pp. 1-10 ◽  
Author(s):  
J. J. Geng ◽  
Y. F. Huang

The detection of optical rebrightenings and X-ray plateaus in the afterglows of gamma-ray bursts (GRBs) challenges the generic external shock model. Recently, we have developed a numerical method to calculate the dynamics of the system consisting of a forward shock and a reverse shock. Here, we briefly review the applications of this method in the afterglow theory. By relating these diverse features to the central engines of GRBs, we find that the steep optical rebrightenings would be caused by the fall-back accretion of black holes, while the shallow optical rebrightenings are the consequence of the injection of the electron-positron-pair wind from the central magnetar. These studies provide useful ways to probe the characteristics of GRB central engines.


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