Does a Fine Tuning of a Quartic Potential Allow for an Invariant Cosmological Constant? How This Supposition Could Lead to a Macro Model of Pressure in the Start of Inflation?  

作　　者：Andrew Walcott Beckwith Andrew Walcott Beckwith(Physics Department, Chongqing University, Huxi Campus, Chongqing, China)

机构地区：[1]Physics Department, Chongqing University, Huxi Campus, Chongqing, China

出　　处：《Journal of High Energy Physics, Gravitation and Cosmology》2023年第2期552-560,共9页高能物理（英文）

摘　　要：Our assumptions in this paper are for a more traditional cosmological constant, not varying over time, which has the result of forming a much simpler entropy expression. But in doing so, we have to make note of how a quartic phase transition initially may impose a level of precision in parameters impossible to verify with present experimental equipment. We also have the conundrum of how this may be linked to macroscopic interpretation of pressure in the initial phases of the universe, using black hole physics in Pre Planckian to Planckian physics domains.Our assumptions in this paper are for a more traditional cosmological constant, not varying over time, which has the result of forming a much simpler entropy expression. But in doing so, we have to make note of how a quartic phase transition initially may impose a level of precision in parameters impossible to verify with present experimental equipment. We also have the conundrum of how this may be linked to macroscopic interpretation of pressure in the initial phases of the universe, using black hole physics in Pre Planckian to Planckian physics domains.

关 键 词：High-Frequency Gravitational Waves (HFGW) Symmetry Causal Discontinuity 

分 类 号：O17[理学—数学]