A Note on Shock Model Justification for IFR Distributions

1981 ◽  
pp. 319-325
Author(s):  
Purushottam Laud ◽  
Roy Saunders
Keyword(s):  
Shock Model

Percutaneous transtracheal ventilation in a canine shock model with an open thorax

1984 ◽  
Vol 13 (1) ◽  
pp. 22-25 ◽  
Author(s):  
Robert C Jorden ◽  
Ernest E Moore ◽  
John A Marx ◽  
Benjamin Honigman ◽  
Barry Simon
Keyword(s):  
Shock Model ◽  
Transtracheal Ventilation

Adequacy of posthypertonic shock model to real cryopreservation conditions during deglycerolization of erythrocytes

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

Oxidative stress may be involved in distant organ failure in tourniquet shock model mice

2014 ◽  
Vol 16 (2) ◽  
pp. 70-75 ◽  
Author(s):  
Rie Nishikata ◽  
Naho Kato ◽  
Kouichi Hiraiwa
Keyword(s):  
Oxidative Stress ◽  
Organ Failure ◽  
Shock Model ◽  
Tourniquet Shock ◽  
Distant Organ

New kinds of multidimensional IFR distribution

1990 ◽  
Vol 22 (1) ◽  
pp. 251-253 ◽  
Author(s):  
Yuedong Wang ◽  
Jinhua Cao
Keyword(s):  
Partial Order ◽  
Shock Model ◽  
Closure Properties ◽  
Increasing Function

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.

scholarly journals Increment of Plasma Soluble CD14 Level in Carrageenan-Primed Endotoxin Shock Model Mice

2006 ◽  
Vol 29 (5) ◽  
pp. 1015-1021 ◽  
Author(s):  
Hiroyasu Hozumi ◽  
Yoshiyuki Adachi ◽  
Taisuke Murakami ◽  
Noriko N. Miura ◽  
Naohito Ohno
Keyword(s):  
Endotoxin Shock ◽  
Shock Model ◽  
Soluble Cd14

scholarly journals Diverse Features of the Multiwavelength Afterglows of Gamma-Ray Bursts: Natural or Special?

2016 ◽  
Vol 2016 ◽  
pp. 1-10 ◽  
Author(s):  
J. J. Geng ◽  
Y. F. Huang
Keyword(s):  
Black Holes ◽  
Numerical Method ◽  
Gamma Ray ◽  
Gamma Ray Bursts ◽  
Shock Model ◽  
Reverse Shock ◽  
X Ray ◽  
Electron Positron ◽  
Forward Shock ◽  
Electron Positron Pair

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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