Inertia and damping effects on the damage-dependent burst size distribution of fiber bundles

2001 ◽  
Vol 290 (5-6) ◽  
pp. 261-269 ◽  
Author(s):  
Etienne L Bonnaud ◽  
Jonas M Neumeister
Keyword(s):  
Size Distribution ◽  
Burst Size ◽  
Fiber Bundles ◽  
Damping Effects

Burst-size distribution in fiber-bundles with local load-sharing

1994 ◽  
Vol 193 (5-6) ◽  
pp. 425-430 ◽  
Author(s):  
S.D. Zhang ◽  
E.J. Ding
Keyword(s):  
Size Distribution ◽  
Burst Size ◽  
Load Sharing ◽  
Local Load ◽  
Fiber Bundles

Molecular Shot Noise, Burst Size Distribution, and Single-Molecule Detection in Fluid Flow:  Effects of Multiple Occupancy

1998 ◽  
Vol 102 (30) ◽  
pp. 6089-6094 ◽  
Author(s):  
Jörg Enderlein ◽  
David L. Robbins ◽  
W. Patrick Ambrose ◽  
Richard A. Keller
Keyword(s):  
Fluid Flow ◽  
Size Distribution ◽  
Single Molecule ◽  
Shot Noise ◽  
Burst Size ◽  
Noise Burst ◽  
Single Molecule Detection ◽  
Flow Effects

scholarly journals Size Distribution of Emitted Energies in Local Load Sharing Fiber Bundles

2021 ◽  
Vol 9 ◽  
Author(s):  
Subhadeep Roy ◽  
Soumyajyoti Biswas
Keyword(s):  
Size Distribution ◽  
Power Law ◽  
Linear Relation ◽  
Fiber Bundle ◽  
Average Energy ◽  
Load Sharing ◽  
Local Load ◽  
Fiber Bundles ◽  
Avalanche Size ◽  
Fiber Bundle Model

We study the local load sharing fiber bundle model and its energy burst statistics. While it is known that the avalanche size distribution of the model is exponential, we numerically show here that the avalanche size (s) and the corresponding average energy burst (〈E〉) in this version of the model have a non-linear relation (〈E〉 ~ sγ). Numerical results indicate that γ ≈ 2.5 universally for different failure threshold distributions. With this numerical observation, it is then possible to show that the energy burst distribution is a power law, with a universal exponent value of −(γ + 1).

The high–energy muon flux at sea level up to 10 TeV derived from an observation of the burst-size spectrum

1968 ◽  
Vol 46 (10) ◽  
pp. S297-S300 ◽  
Author(s):  
S. Chin ◽  
Y. Hanayama ◽  
T. Hara ◽  
S. Higashi ◽  
T. Kitamura ◽  
...  
Keyword(s):  
Energy Spectrum ◽  
Size Distribution ◽  
Sea Level ◽  
Burst Size ◽  
High Energy ◽  
Muon Flux ◽  
Size Spectrum ◽  
High Energy Muon ◽  
Relativistic Particles

Bursts produced by high-energy muons in rock have been observed at a depth of 40 m.w.e. underground by the use of two layers of scintillator 20 m2 in area and 2 m apart. The size distribution of bursts with several hundreds to 30 000 relativistic particles was obtained during an observing time of 11 424.13 hours. Following the method of Christy and Kusaka (1941), the energy spectrum of muons up to 10 TeV was derived from the burst-size distribution.

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