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Updated: Apr 4, 2026

The Generation of Higher-order Laguerre-Gauss Optical Beams for High-precision Interferometry
Published on: August 12, 2013
Zero average values of cosmological perturbations as an indispensable condition for the theory and simulations
Maxim Eingorn1, Maxim Brilenkov2, Branislav Vlahovic1
1CREST and NASA Research Centers, North Carolina Central University, Fayetteville st. 1801, Durham, NC 27707 USA.
Abstract:
We point out a weak side of the commonly used determination of scalar cosmological perturbations lying in the fact that their average values can be nonzero for some matter distributions. It is shown that introduction of the finite-range gravitational potential instead of the infinite-range one resolves this problem. The concrete illustrative density profile is investigated in detail in this connection.
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