Abstract

In this work, we consider effects of the dynamical vacuum in quantum cosmology in presence of a minimum length introduced by the GUP (generalized uncertainty principle) related to the modified commutation relation [{hat{X}},{hat{P}}] := frac{ihbar }{ 1 - beta {hat{P}}^2 }. We determine the wave function of the Universe psi _{qp}(xi ,t), which is solution of the modified Wheeler–DeWitt equation in the representation of the quasi-position space, in the limit where the scale factor of the Universe is small. Although psi _{qp}(xi ,t) is a physically acceptable state it is not a realizable state of the Universe because psi _{qp}(xi ,t) has infinite norm, as in the ordinary case with no minimal length.

Highlights

  • We determine the wave function of the Universe ψqp(ξ, t), which is solution of the modified

  • The most common modified or deformed commutation relation (MCR) associated with a Generalized Uncertainty Principle (GUP) (KMM GUP [37]) is quadratic in the momentum operator, effects of a MCR with a linear term in the momentum operator, which leads to a minimal length and a maximum momentum [38], have been studied in contexts of cosmological models

  • Since GUP corresponds to a modification of the commutation relation between the operator and its conjugate operator, the WDW equation in a minimal-length scenario can be obtained imposing that some or all of those operators and its conjugate momentum operators satisfy modified commutation relations

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Summary

Introduction

We can obtain a minimal-length scenario by modifying the Heisenberg uncertainty principle (HUP) between the position and momentum operators. In a minimal-length scenario that scalar field and its conjugate momentum have to obey the modified commutation relations [43,44,45,46] As it is well known, the ordinary approach of the third quantization of the Wheeler–DeWitt (WDW) equation leads to the vanishing of the cosmological constant. Since GUP corresponds to a modification of the commutation relation between the operator and its conjugate operator, the WDW equation in a minimal-length scenario can be obtained imposing that some or all of those operators (which have come from the quantization of remaining degrees of freedom in the mini-superspace approach) and its conjugate momentum operators satisfy modified commutation relations. We determine the modified WDW equation up to O(β2) considering a quantum cosmology model of dynamical vacuum in a minimal-length scenario induced by the commutation relation proposed by Pedram [66,67],.

Minimal-length scenario
Gravity action
Fluid action
The modified Wheeler–DeWitt equation
Solution of the modified Wheeler–DeWitt equation
Solution: first method
Solution: second method
Validity range
Physically acceptable solutions
Norm of the wave function
Conclusion

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