New Conservation Law and a Consideration as to When Forming a Cosmological Constant Term: Using Fifth Force for Frequency of BEC “Gravitons” and Cosmological Constant Formed before BEC Gravitons Form  

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

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

出　　处：《Journal of High Energy Physics, Gravitation and Cosmology》2023年第2期489-495,共7页高能物理（英文）

摘　　要：We use scalar fields. The scalar field version which we are using is one from Padmanabhan, and the problem is that the scalar field in the Padmanabhan representation is initially only dependent on time. We also refer to a new assumed conservation law which will give new structure as to inflationary expansion and its immediate aftermath. That of the Hubble “constant” is divided by the “time derivative” of the scalar field in the inflation regime and then a long time afterwards. In doing so, we help define when the cosmological constant may form and what they says about the advent of dark energy.We use scalar fields. The scalar field version which we are using is one from Padmanabhan, and the problem is that the scalar field in the Padmanabhan representation is initially only dependent on time. We also refer to a new assumed conservation law which will give new structure as to inflationary expansion and its immediate aftermath. That of the Hubble “constant” is divided by the “time derivative” of the scalar field in the inflation regime and then a long time afterwards. In doing so, we help define when the cosmological constant may form and what they says about the advent of dark energy.

关 键 词：INFLATON Fifth Force Gravitational Waves GRAVITONS Hubble Parameter 

分 类 号：P15[天文地球—天文学]