Neutrinos in gravitational collapse: Analysis of the flux profile

Pramana ◽  
1984 ◽  
Vol 22 (3-4) ◽  
pp. 159-171 ◽  
Author(s):  
S V Dhurandhar ◽  
C V Vishveshwara
Keyword(s):  
Gravitational Collapse ◽  
Collapse Analysis ◽  
Flux Profile

The Coupled Boundary Layers and Air-Sea Transfer Experiment in Low to Moderate Winds (CBLAST-LOW): Flux Profile Relationships Across the Coupled Boundary Layers

2002 ◽  
Author(s):  
John H. Trowbridge ◽  
James B. Edson ◽  
Wade R. McGillis ◽  
Albert J. Plueddeman ◽  
Eugene A. Terray ◽  
...  
Keyword(s):  
Boundary Layers ◽  
Transfer Experiment ◽  
Flux Profile

Introduction

2018 ◽  
Author(s):  
Flavio Mercati
Keyword(s):  
Field Theory ◽  
General Relativity ◽  
Gravitational Collapse ◽  
Present State ◽  
Strong Gravity ◽  
Shape Dynamics

Shape Dynamics (SD) is a field theory that describes gravity in a different way than General Relativity (GR): it assumes a preferred notion of simultaneity, and the dynamical content of the theory consists of conformal 3- geometries. SD coincides with (GR) in most situations, in particular in the experimentally well-tested regimes, but it departs from it in some strong-gravity situations, for example at cosmological singularities or upon gravitational collapse. This chapter provides a quick introduction to the theory and a brief description of its present state.

Comparisons of design methods for beam string structure based on reliability and progressive collapse analysis

Structures ◽  
2021 ◽  
Vol 33 ◽  
pp. 2166-2176
Author(s):  
Hao Zhou ◽  
Youbao Jiang ◽  
Sondipon Adhikari ◽  
Qianqian Yin ◽  
Jianguo Cai
Keyword(s):  
Progressive Collapse ◽  
Design Methods ◽  
Collapse Analysis ◽  
String Structure ◽  
Progressive Collapse Analysis

Applicability of the Langmuir equation to simulate the vertical mass flux profile

2021 ◽  
Vol 14 (16) ◽  
Author(s):  
Huanyu Shi ◽  
Zhibao Dong ◽  
Nan Xiao ◽  
Qinni Huang
Keyword(s):  
Mass Flux ◽  
Langmuir Equation ◽  
Flux Profile

scholarly journals Magnetic field amplification in newly-born neutron stars

1996 ◽  
Vol 160 ◽  
pp. 435-436
Author(s):  
H.-J. Wiebicke ◽  
U. Geppert
Keyword(s):  
Magnetic Field ◽  
Neutron Stars ◽  
Gravitational Collapse ◽  
Dipole Field ◽  
Numerical Calculations ◽  
Selection Effects ◽  
Thermoelectric Effects ◽  
Field Amplification ◽  
Seed Field ◽  
Flux Conservation

AbstractWe present a scenario of magnetic field (MF) evolution of newly-born neutron stars (NSs). Numerical calculations show that in the hot phase of young NSs the MF can be amplified by thermoelectric effects, starting from a moderately strong seed-field. Therefore, there is no need to assume a 1012G dipole field immediately after the gravitational collapse of the supernova (SN) event. The widely accepted scenario for such a field to be produced by flux conservation during the collapse is critically discussed. Instead, it can be generated by amplification and selection effects in the first 104yrs, and by the subsequent fast ohmic decay of higher multipole components, when the NS cools down.

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