A New Solution of The Cosmological Constant Problems

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Earlier work this paper cites.

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Earlier work this paper cites.

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Earlier work this paper cites.

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Cited alongside, same era.

M. Tegmark et al. , Phys. Rev. D 73

2006

Cited alongside, same era.

This is unlike the ever-present Λ \Lambda model of R. Sorkin, Int. J. Theo. Phys. 36

2007

Cited alongside, same era.

E. Komatsu et al

Original

Cited in the paper.

The sum over matter and metric configurations in Z ⁡ [ ℳ ] Z[\mathcal{M}] is performed with the same set of free boundary data, { Q A } \left\{Q^{A}\right\} , kept fixed as in the definition of Z Λ ​ [ M ] Z_{\Lambda}[M]

Cited in the paper.

We neglect black hole boundaries. They make a negligible contribution to the surface term in Eq.(2)

Cited in the paper.

The singular nature of ∂ ℳ I \partial\mathcal{M}_{\mathrm{I}} mandates an extra surface term on ∂ ℳ I \partial\mathcal{M}_{I} .See [ 9 ] for further details. The initial state and hence all terms on ∂ ℳ I \partial\mathcal{M}_{\mathrm{I}} are λ \lambda -independent and so these terms make no contribution to Eq.( 1

Cited in the paper.

Differently placed observers are most to observe when t ∼ t ms t\sim t_{\rm ms} , where t ms ∼ O ⁡ ( 10 10 ​ yrs ) t_{\rm ms}\sim O(10^{10}\,{\rm yrs}) is the main-sequence lifetime; they will all most likely observe Λ ∼ O ⁡ ( t ms − 2 ) \Lambda\sim O(t_{\rm ms}^{-2}) in our model

Cited in the paper.

G. W. Gibbons and N. Turok, Phys. Rev. D 77

2008

Later among the works it cites.

D.J. Shaw and J.D. Barrow, arXiv: 1010.4262 (2010)

2010

Closest in time.