We look at, starting with Shankar’s treatment of the partition function, inserting in the data of the modified Heisenberg uncertainty principle as to give a role to the inflaton in the formation of a partition of the...We look at, starting with Shankar’s treatment of the partition function, inserting in the data of the modified Heisenberg uncertainty principle as to give a role to the inflaton in the formation of a partition of the universe. The end result will be, even with the existence of a multiverse, i.e. simultaneous universes, uniform physical laws throughout the multiple universes.展开更多
文摘We look at, starting with Shankar’s treatment of the partition function, inserting in the data of the modified Heisenberg uncertainty principle as to give a role to the inflaton in the formation of a partition of the universe. The end result will be, even with the existence of a multiverse, i.e. simultaneous universes, uniform physical laws throughout the multiple universes.
