scholarly journals Majorana dark matter in a classically scale invariant model

2015 ◽  
Vol 2015 (1) ◽  
Author(s):  
Sanjin Benić ◽  
Branimir Radovčić
2016 ◽  
Vol 94 (5) ◽  
Author(s):  
Amine Ahriche ◽  
Adrian Manning ◽  
Kristian L. McDonald ◽  
Salah Nasri

Author(s):  
Siavash H. Sohrab

A scale-invariant model of statistical mechanics is described leading to invariant Boltzmann equation and the corresponding invariant Enskog equation of change. A modified form of Cauchy stress tensor for fluid is presented such that in the limit of vanishing intermolecular spacing all tangential forces vanish in accordance with perceptions of Cauchy and Poisson. The invariant forms of mass, thermal energy, linear momentum, and angular momentum conservation equations derived from invariant Enskog equation of change are described. Also, some exact solution of the conservation equations for the problems of normal shock, flow over a flat plate, and flow within a spherical droplet located at the stagnation point of opposed cylindrically-symmetric gaseous jets are presented.


2014 ◽  
Vol 137 (1) ◽  
Author(s):  
Siavash H. Sohrab

A scale-invariant model of statistical mechanics is described leading to invariant Enskog equation of change that is applied to derive invariant forms of conservation equations for mass, thermal energy, linear momentum, and angular momentum in chemically reactive fields. Modified hydro-thermo-diffusive theories of laminar premixed flames for (1) rigid-body and (2) Brownian-motion flame propagation models are presented and are shown to be mathematically equivalent. The predicted temperature profile, thermal thickness, and propagation speed of laminar methane–air premixed flame are found to be in good agreement with existing experimental observations.


2015 ◽  
Vol 91 (11) ◽  
Author(s):  
Jun Guo ◽  
Zhaofeng Kang ◽  
P. Ko ◽  
Yuta Orikasa
Keyword(s):  

2016 ◽  
Vol 2016 (2) ◽  
Author(s):  
Naoyuki Haba ◽  
Hiroyuki Ishida ◽  
Ryo Takahashi ◽  
Yuya Yamaguchi

2002 ◽  
Vol 17 (29) ◽  
pp. 4273-4280
Author(s):  
ALEJANDRO GANGUI

In the framework of inflationary models with non-vacuum initial states for cosmological perturbations, we study non-Gaussian signatures on the cosmic microwave background (CMB) radiation produced by a broken-scale-invariant model which incorporates a feature at a privileged scale in the primordial power spectrum.


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