Can Thermal Input from a Prior Universe Account for Relic Graviton Production and Imply Usage of the Bogomolnyi Inequality, as a Bridge between Brane World Models and Loop Quantum Gravity in Early Universe Conditions?  

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》2016年第3期412-431,共20页高能物理（英文）

摘　　要：The author uses a low temperature and low entropy pre inflation state to create a bridge between String theory and loop quantum gravity. We use this analysis in lieu of the CMB barrier as of z = 1000 since it is our way to come up with a working model of quintessence scalar fields, which permits relic generation of dark matter and dark energy. Not only referencing this bridge, we do it in such a way as to utilize the low entropy condition which the Brane world model of Randal and Sundrum creates, and to show how it is in common with what Caroll and Chen wrote up in 2005., i.e. when the universe was about 1000 times smaller and 100,000 times younger than today.The author uses a low temperature and low entropy pre inflation state to create a bridge between String theory and loop quantum gravity. We use this analysis in lieu of the CMB barrier as of z = 1000 since it is our way to come up with a working model of quintessence scalar fields, which permits relic generation of dark matter and dark energy. Not only referencing this bridge, we do it in such a way as to utilize the low entropy condition which the Brane world model of Randal and Sundrum creates, and to show how it is in common with what Caroll and Chen wrote up in 2005., i.e. when the universe was about 1000 times smaller and 100,000 times younger than today.

关 键 词：BRANES Axion Walls Bogomolnyi Inequality Four- and Five-Dimensional Cosmological Constant 

分 类 号：O17[理学—数学]