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Antilensing: the bright side of voids
Krzysztof Bolejko1, Chris Clarkson, Roy Maartens
1Sydney Institute for Astronomy, The University of Sydney, Sydney, New South Wales 2006, Australia.
Physical Review Letters
|February 7, 2013
Summary
Cosmic voids, typically thought to dim distant objects, actually brighten them due to a neglected relativistic Doppler effect. This finding impacts weak lensing and supernova observations.
Area of Science:
- Cosmology
- Astrophysics
- General Relativity
Background:
- Cosmic voids constitute over half the universe's volume.
- Weak lensing by voids is conventionally assumed to cause dimming.
- This dimming is attributed to reduced photon counts from smaller apparent object sizes.
Purpose of the Study:
- To investigate the lensing magnification effect of cosmic voids.
- To re-evaluate the standard weak lensing integral predictions.
- To explore relativistic effects on void lensing.
Main Methods:
- Analysis of the relativistic Doppler term in lensing.
- Comparison of linear relativistic theory with exact solutions.
- Estimation of nonlinear corrections to lensing convergence.
Main Results:
- A relativistic Doppler term, typically neglected, dominates void lensing at low redshifts.
- Contrary to expectations, voids cause magnification (brightening) of distant objects.
- Nonlinear corrections significantly enhance the relativistic effect, exceeding linear predictions by over 20% for deep voids.
Conclusions:
- The standard weak lensing model is insufficient for accurately describing void effects.
- Relativistic effects, including nonlinear corrections, are crucial for understanding void lensing.
- This phenomenon poses a significant systematic error for cosmological measurements like weak lensing density reconstruction and supernova surveys.
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