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Earlier work this paper cites.
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1989
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Paranjape A., Lam T. Y., Sheth R. K., 2012, MNRAS, 420, 1429, 1105.1990
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1990
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Dubinski J., da Costa L. N., Goldwirth D. S., Lecar M., Piran T., 1993, ApJ, 410, 458, ADS
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Bernardeau F., 1994, A& A, 291, 697, astro-ph/9403020
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Mo H. J., White S. D. M., 1996, MNRAS, 282, 347, astro-ph/9512127 , ADS
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Sheth R. K., 1998, MNRAS, 300, 1057, astro-ph/9805319
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Sheth R. K., Diaferio A., 2001, MNRAS, 322, 901, astro-ph/0009166 , ADS
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Sheth R. K., Diaferio A., Hui L., Scoccimarro R., 2001, MNRAS, 326, 463, astro-ph/0010137 , ADS
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Sheth R. K., Mo H., Tormen G., 2001, MNRAS, 323, 1, astro-ph/9907024
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Sheth R. K., van de Weygaert R., 2004, MNRAS, 350, 517, astro-ph/0311260 , ADS
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Martino M. C., Sheth R. K., 2009, ArXiv e-prints, 0911.1829 , ADS
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2018

Density and velocity profiles around cosmic voids

Massara, Elena, Sheth, Ravi K.

Understand

We study the evolution of the cross-correlation between voids and the mass density field - i.e.

of void profiles.
We show that approaches based on the spherical model alone miss an important contribution to the evolution on large scales of most interest to cosmology: they fail to capture the well-known fact that the large-scale bias factor of conserved tracers evolves.
We also show that the operations of evolution and averaging do not commute, but this difference is only significant within about two effective radii.

Built on

Gunn J. E., Gott III J. R., 1972, Astrophys.J., 176, 1, ADS
1972
Earlier work this paper cites.
Bardeen J. M., Bond J. R., Kaiser N., Szalay A. S., 1986, ApJ, 304, 15
1986
Earlier work this paper cites.
Cole S., Kaiser N., 1989, MNRAS, 237, 1127, ADS
1989
Earlier work this paper cites.
Paranjape A., Lam T. Y., Sheth R. K., 2012, MNRAS, 420, 1429, 1105.1990
Original
1990
Earlier work this paper cites.
Dubinski J., da Costa L. N., Goldwirth D. S., Lecar M., Piran T., 1993, ApJ, 410, 458, ADS
1993
Earlier work this paper cites.
Bernardeau F., 1994, A& A, 291, 697, astro-ph/9403020
1994
Earlier work this paper cites.
Nusser A., Davis M., 1994, ApJ, 421, L1, astro-ph/9309009 , ADS
1994
Earlier work this paper cites.
Fisher K. B., 1995, ApJ, 448, 494, astro-ph/9412081 , ADS
1995
Earlier work this paper cites.
Mo H. J., White S. D. M., 1996, MNRAS, 282, 347, astro-ph/9512127 , ADS
1996
Earlier work this paper cites.
Sheth R. K., 1998, MNRAS, 300, 1057, astro-ph/9805319
1998
Earlier work this paper cites.
Sheth R. K., Diaferio A., 2001, MNRAS, 322, 901, astro-ph/0009166 , ADS
2001
Earlier work this paper cites.
Sheth R. K., Diaferio A., Hui L., Scoccimarro R., 2001, MNRAS, 326, 463, astro-ph/0010137 , ADS
2001
Earlier work this paper cites.
Sheth R. K., Mo H., Tormen G., 2001, MNRAS, 323, 1, astro-ph/9907024
2001
Earlier work this paper cites.
Sheth R. K., van de Weygaert R., 2004, MNRAS, 350, 517, astro-ph/0311260 , ADS
2004
Earlier work this paper cites.
Martino M. C., Sheth R. K., 2009, ArXiv e-prints, 0911.1829 , ADS
Original
2009
Earlier work this paper cites.