Built on

NASA PICO
Original
1902
Earlier work this paper cites.
C. Dvorkin et al
Original
1903
Earlier work this paper cites.
J. I. Cayuso and M. C. Johnson, “Towards testing CMB anomalies using the kinetic and polarized Sunyaev-Zel’dovich effects,” Phys. Rev. D
Original
1904
Earlier work this paper cites.
B. Hadzhiyska, B. D. Sherwin, M. Madhavacheril, and S. Ferraro, “Improving Small-Scale CMB Lensing Reconstruction,” Phys. Rev. D
Original
1905
Earlier work this paper cites.
D. Copeland, A. Taylor, and A. Hall, “Towards determining the neutrino mass hierarchy: weak lensing and galaxy clustering forecasts with baryons and intrinsic alignments,” Mon. Not. Roy. Astron. Soc
Original
1905
Earlier work this paper cites.
N. Sehgal et al
Original
1906
Earlier work this paper cites.
K. Abazajian et al
Original
1907
Earlier work this paper cites.
P. Virtanen et al
Original
1907
Earlier work this paper cites.
L. Knox and M. Millea, “Hubble constant hunter’s guide,” Phys. Rev. D
Original
1908
Earlier work this paper cites.
S. C. Hotinli, J. B. Mertens, M. C. Johnson, and M. Kamionkowski, “Probing correlated compensated isocurvature perturbations using scale-dependent galaxy bias,” Phys. Rev
Original
1908
Earlier work this paper cites.
A. Schneider, A. Refregier, S. Grandis, D. Eckert, N. Stoira, T. Kacprzak, M. Knabenhans, J. Stadel, and R. Teyssier, “Baryonic effects for weak lensing. Part II. Combination with X-ray data and extended cosmologies,” JCAP
Original
1911
Earlier work this paper cites.
W. R. Coulton, P. D. Meerburg, D. G. Baker, S. Hotinli, A. J. Duivenvoorden, and A. van Engelen, “Minimizing gravitational lensing contributions to the primordial bispectrum covariance,” Phys. Rev. D
Original
1912
Earlier work this paper cites.
J. Silk, “Fluctuations in the Primordial Fireball,” Nature (London)
1967
Earlier work this paper cites.
P. J. E. Peebles and J. T. Yu, “Primeval adiabatic perturbation in an expanding universe,” Astrophys. J
1970
Earlier work this paper cites.
S. Weinberg, “Entropy generation and the survival of protogalaxies in an expanding universe,” Astrophys. J
1971
Earlier work this paper cites.
A. Mead, J. Peacock, C. Heymans, S. Joudaki, and A. Heavens, “An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models,” Mon. Not. Roy. Astron. Soc
Original
1975
Earlier work this paper cites.
N. Kaiser, “Small-angle anisotropy of the microwave background radiation in the adiabatic theory,” Mon. Not. R. Astron. Soc
1983
Earlier work this paper cites.
M. Birkinshaw and S. F. Gull, “A test for transverse motions of clusters of galaxies,” Nature (London)
1983
Earlier work this paper cites.
S. M. Carroll, G. B. Field, and R. Jackiw, “Limits on a Lorentz and Parity Violating Modification of Electrodynamics,” Phys. Rev. D
1990
Earlier work this paper cites.
D. Harari and P. Sikivie, “Effects of a Nambu-Goldstone boson on the polarization of radio galaxies and the cosmic microwave background,” Phys. Lett. B
1992
Earlier work this paper cites.
D. Polarski and A. A. Starobinsky, “Isocurvature perturbations in multiple inflationary models,” Phys. Rev. D
1994
Earlier work this paper cites.
W. Hu and N. Sugiyama, “Toward understanding CMB anisotropies and their implications,” Phys. Rev. D
1995
Earlier work this paper cites.
M. Zaldarriaga and D. D. Harari, “Analytic approach to the polarization of the cosmic microwave background in flat and open universes,” Phys. Rev. D
1995
Earlier work this paper cites.
W. Hu and M. J. White, “Acoustic signatures in the cosmic microwave background,” Astrophys. J
1996
Earlier work this paper cites.
A. Kosowsky and A. Loeb, “Faraday rotation of microwave background polarization by a primordial magnetic field,” Astrophys. J
1996
Earlier work this paper cites.
M. Zaldarriaga and U. Seljak, “An all sky analysis of polarization in the microwave background,” Phys. Rev. D
1997
Earlier work this paper cites.
M. Kamionkowski, A. Kosowsky, and A. Stebbins, “Statistics of cosmic microwave background polarization,” Phys. Rev. D
1997
Earlier work this paper cites.
M. Kamionkowski and A. Loeb, “Getting around cosmic variance,” Phys. Rev. D
1997
Earlier work this paper cites.
S. M. Carroll, “Quintessence and the rest of the world,” Phys. Rev. Lett
1998
Earlier work this paper cites.
A. Lue, L.-M. Wang, and M. Kamionkowski, “Cosmological signature of new parity violating interactions,” Phys. Rev. Lett
1999
Earlier work this paper cites.
S. Y. Sazonov and R. A. Sunyaev, “Microwave polarization in the direction of galaxy clusters induced by the CMB quadrupole anisotropy,” Mon. Not. Roy. Astron. Soc
1999
Earlier work this paper cites.
A. Lewis, A. Challinor, and A. Lasenby, “Efficient computation of CMB anisotropies in closed FRW models,” Astrophys. J
2000
Earlier work this paper cites.
M. Zaldarriaga, “Lensing of the CMB: Non-Gaussian aspects,” Phys. Rev. D
2000
Earlier work this paper cites.
C. Gordon, D. Wands, B. A. Bassett, and R. Maartens, “Adiabatic and entropy perturbations from inflation,” Phys. Rev. D
2000
Earlier work this paper cites.
J. A. Peacock and R. E. Smith, “Halo occupation numbers and galaxy bias,” Mon. Not. Roy. Astron. Soc
2000
Earlier work this paper cites.
U. Seljak, “Analytic model for galaxy and dark matter clustering,” Mon. Not. Roy. Astron. Soc
2000
Earlier work this paper cites.
W. Hu, “Angular trispectrum of the CMB,” Phys. Rev. D
2001
Earlier work this paper cites.
W. Hu, “Mapping the dark matter through the cmb damping tail,” Astrophys. J. Lett
2001
Earlier work this paper cites.
M. Bucher, K. Moodley, and N. Turok, “Constraining isocurvature perturbations with CMB polarization,” Phys. Rev. Lett
2001
Earlier work this paper cites.
W. Hu and T. Okamoto, “Mass reconstruction with cmb polarization,” Astrophys. J
2002
Earlier work this paper cites.
A. D. Dolgov, “Neutrinos in cosmology,” Phys. Rept
2002
Earlier work this paper cites.
L. Knox and Y.-S. Song, “A Limit on the detectability of the energy scale of inflation,” Phys. Rev. Lett
2002
Earlier work this paper cites.
M. Kesden, A. Cooray, and M. Kamionkowski, “Separation of gravitational wave and cosmic shear contributions to cosmic microwave background polarization,” Phys. Rev. Lett
2002
Earlier work this paper cites.
M. Millea, E. Anderes, and B. D. Wandelt, “Sampling-based inference of the primordial CMB and gravitational lensing,” Phys. Rev. D
Original
2002
Earlier work this paper cites.

Similar

W. Hu, “Dark synergy: Gravitational lensing and the CMB,” Phys. Rev. D
2002
Cited alongside, same era.
F. Bernardeau, S. Colombi, E. Gaztanaga, and R. Scoccimarro, “Large scale structure of the universe and cosmological perturbation theory,” Phys. Rept
2002
Cited alongside, same era.
A. Cooray and R. K. Sheth, “Halo Models of Large Scale Structure,” Phys. Rept
2002
Cited alongside, same era.
T. Okamoto and W. Hu, “CMB lensing reconstruction on the full sky,” Phys. Rev. D
2003
Cited alongside, same era.
M. Kaplinghat, L. Knox, and Y.-S. Song, “Determining neutrino mass from the CMB alone,” Phys. Rev. Lett
2003
Cited alongside, same era.
C. M. Hirata and U. Seljak, “Analyzing weak lensing of the cosmic microwave background using the likelihood function,” Phys. Rev. D

Then

M. P. van Daalen, J. Schaye, C. M. Booth, and C. D. Vecchia, “The effects of galaxy formation on the matter power spectrum: A challenge for precision cosmology,” Mon. Not. Roy. Astron. Soc
Original
2011
Later among the works it cites.
K. M. Smith, D. Hanson, M. LoVerde, C. M. Hirata, and O. Zahn, “Delensing CMB Polarization with External Datasets,” JCAP
Original
2012
Later among the works it cites.
M. Millea et al
Original
2012
Later among the works it cites.
E. Alizadeh and C. M. Hirata, “How to detect gravitational waves through the cross-correlation of the galaxy distribution with the CMB polarization,” Phys. Rev. D
Original
2012
Later among the works it cites.
S. C. Hotinli and M. C. Johnson, “Reconstructing large scales at cosmic dawn,” arXiv:2012.09851 [astro-ph.CO]

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2021

The Benefits of CMB Delensing

Hotinli, Selim C., Meyers, Joel, Trendafilova, Cynthia et al.

Understand

The effects of gravitational lensing of the cosmic microwave background (CMB) have been measured at high significance with existing data and will be measured even more precisely in future surveys.

Reversing the effects of lensing on the observed CMB temperature and polarization maps provides a variety of benefits.
Delensed CMB spectra have sharper acoustic peaks and more prominent damping tails, allowing for improved inferences of cosmological parameters that impact those features.
Delensing reduces $B$-mode power, aiding the search for primordial gravitational waves and allowing for lower variance reconstruction of lensing and other sources of secondary CMB anisotropies.

Built on

NASA PICO
Original
1902
Earlier work this paper cites.
C. Dvorkin et al
Original
1903
Earlier work this paper cites.
J. I. Cayuso and M. C. Johnson, “Towards testing CMB anomalies using the kinetic and polarized Sunyaev-Zel’dovich effects,” Phys. Rev. D
Original
1904
Earlier work this paper cites.
B. Hadzhiyska, B. D. Sherwin, M. Madhavacheril, and S. Ferraro, “Improving Small-Scale CMB Lensing Reconstruction,” Phys. Rev. D
Original
1905
Earlier work this paper cites.
D. Copeland, A. Taylor, and A. Hall, “Towards determining the neutrino mass hierarchy: weak lensing and galaxy clustering forecasts with baryons and intrinsic alignments,” Mon. Not. Roy. Astron. Soc
Original
1905
Earlier work this paper cites.
N. Sehgal et al
Original
1906
Earlier work this paper cites.
K. Abazajian et al
Original
1907
Earlier work this paper cites.
P. Virtanen et al
Original
1907
Earlier work this paper cites.
L. Knox and M. Millea, “Hubble constant hunter’s guide,” Phys. Rev. D
Original
1908
Earlier work this paper cites.
S. C. Hotinli, J. B. Mertens, M. C. Johnson, and M. Kamionkowski, “Probing correlated compensated isocurvature perturbations using scale-dependent galaxy bias,” Phys. Rev
Original
1908
Earlier work this paper cites.
A. Schneider, A. Refregier, S. Grandis, D. Eckert, N. Stoira, T. Kacprzak, M. Knabenhans, J. Stadel, and R. Teyssier, “Baryonic effects for weak lensing. Part II. Combination with X-ray data and extended cosmologies,” JCAP
Original
1911
Earlier work this paper cites.
W. R. Coulton, P. D. Meerburg, D. G. Baker, S. Hotinli, A. J. Duivenvoorden, and A. van Engelen, “Minimizing gravitational lensing contributions to the primordial bispectrum covariance,” Phys. Rev. D
Original
1912
Earlier work this paper cites.
J. Silk, “Fluctuations in the Primordial Fireball,” Nature (London)
1967
Earlier work this paper cites.
P. J. E. Peebles and J. T. Yu, “Primeval adiabatic perturbation in an expanding universe,” Astrophys. J
1970
Earlier work this paper cites.
S. Weinberg, “Entropy generation and the survival of protogalaxies in an expanding universe,” Astrophys. J
1971
Earlier work this paper cites.
A. Mead, J. Peacock, C. Heymans, S. Joudaki, and A. Heavens, “An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models,” Mon. Not. Roy. Astron. Soc
Original
1975
Earlier work this paper cites.
N. Kaiser, “Small-angle anisotropy of the microwave background radiation in the adiabatic theory,” Mon. Not. R. Astron. Soc
1983
Earlier work this paper cites.
M. Birkinshaw and S. F. Gull, “A test for transverse motions of clusters of galaxies,” Nature (London)
1983
Earlier work this paper cites.
S. M. Carroll, G. B. Field, and R. Jackiw, “Limits on a Lorentz and Parity Violating Modification of Electrodynamics,” Phys. Rev. D
1990
Earlier work this paper cites.
D. Harari and P. Sikivie, “Effects of a Nambu-Goldstone boson on the polarization of radio galaxies and the cosmic microwave background,” Phys. Lett. B
1992
Earlier work this paper cites.
D. Polarski and A. A. Starobinsky, “Isocurvature perturbations in multiple inflationary models,” Phys. Rev. D
1994
Earlier work this paper cites.
W. Hu and N. Sugiyama, “Toward understanding CMB anisotropies and their implications,” Phys. Rev. D
1995
Earlier work this paper cites.
M. Zaldarriaga and D. D. Harari, “Analytic approach to the polarization of the cosmic microwave background in flat and open universes,” Phys. Rev. D
1995
Earlier work this paper cites.
W. Hu and M. J. White, “Acoustic signatures in the cosmic microwave background,” Astrophys. J
1996
Earlier work this paper cites.
A. Kosowsky and A. Loeb, “Faraday rotation of microwave background polarization by a primordial magnetic field,” Astrophys. J
1996
Earlier work this paper cites.
M. Zaldarriaga and U. Seljak, “An all sky analysis of polarization in the microwave background,” Phys. Rev. D
1997
Earlier work this paper cites.
M. Kamionkowski, A. Kosowsky, and A. Stebbins, “Statistics of cosmic microwave background polarization,” Phys. Rev. D
1997
Earlier work this paper cites.
M. Kamionkowski and A. Loeb, “Getting around cosmic variance,” Phys. Rev. D
1997
Earlier work this paper cites.
S. M. Carroll, “Quintessence and the rest of the world,” Phys. Rev. Lett
1998
Earlier work this paper cites.
A. Lue, L.-M. Wang, and M. Kamionkowski, “Cosmological signature of new parity violating interactions,” Phys. Rev. Lett
1999
Earlier work this paper cites.
S. Y. Sazonov and R. A. Sunyaev, “Microwave polarization in the direction of galaxy clusters induced by the CMB quadrupole anisotropy,” Mon. Not. Roy. Astron. Soc
1999
Earlier work this paper cites.
A. Lewis, A. Challinor, and A. Lasenby, “Efficient computation of CMB anisotropies in closed FRW models,” Astrophys. J
2000
Earlier work this paper cites.
M. Zaldarriaga, “Lensing of the CMB: Non-Gaussian aspects,” Phys. Rev. D
2000
Earlier work this paper cites.
C. Gordon, D. Wands, B. A. Bassett, and R. Maartens, “Adiabatic and entropy perturbations from inflation,” Phys. Rev. D
2000
Earlier work this paper cites.
J. A. Peacock and R. E. Smith, “Halo occupation numbers and galaxy bias,” Mon. Not. Roy. Astron. Soc
2000
Earlier work this paper cites.
U. Seljak, “Analytic model for galaxy and dark matter clustering,” Mon. Not. Roy. Astron. Soc
2000
Earlier work this paper cites.
W. Hu, “Angular trispectrum of the CMB,” Phys. Rev. D
2001
Earlier work this paper cites.
W. Hu, “Mapping the dark matter through the cmb damping tail,” Astrophys. J. Lett
2001
Earlier work this paper cites.
M. Bucher, K. Moodley, and N. Turok, “Constraining isocurvature perturbations with CMB polarization,” Phys. Rev. Lett
2001
Earlier work this paper cites.
W. Hu and T. Okamoto, “Mass reconstruction with cmb polarization,” Astrophys. J
2002
Earlier work this paper cites.
A. D. Dolgov, “Neutrinos in cosmology,” Phys. Rept
2002
Earlier work this paper cites.
L. Knox and Y.-S. Song, “A Limit on the detectability of the energy scale of inflation,” Phys. Rev. Lett
2002
Earlier work this paper cites.
M. Kesden, A. Cooray, and M. Kamionkowski, “Separation of gravitational wave and cosmic shear contributions to cosmic microwave background polarization,” Phys. Rev. Lett
2002
Earlier work this paper cites.
M. Millea, E. Anderes, and B. D. Wandelt, “Sampling-based inference of the primordial CMB and gravitational lensing,” Phys. Rev. D
Original
2002
Earlier work this paper cites.

Similar

W. Hu, “Dark synergy: Gravitational lensing and the CMB,” Phys. Rev. D
2002
Cited alongside, same era.
F. Bernardeau, S. Colombi, E. Gaztanaga, and R. Scoccimarro, “Large scale structure of the universe and cosmological perturbation theory,” Phys. Rept
2002
Cited alongside, same era.
A. Cooray and R. K. Sheth, “Halo Models of Large Scale Structure,” Phys. Rept
2002
Cited alongside, same era.
T. Okamoto and W. Hu, “CMB lensing reconstruction on the full sky,” Phys. Rev. D
2003
Cited alongside, same era.
M. Kaplinghat, L. Knox, and Y.-S. Song, “Determining neutrino mass from the CMB alone,” Phys. Rev. Lett
2003
Cited alongside, same era.
C. M. Hirata and U. Seljak, “Analyzing weak lensing of the cosmic microwave background using the likelihood function,” Phys. Rev. D

Then

M. P. van Daalen, J. Schaye, C. M. Booth, and C. D. Vecchia, “The effects of galaxy formation on the matter power spectrum: A challenge for precision cosmology,” Mon. Not. Roy. Astron. Soc
Original
2011
Later among the works it cites.
K. M. Smith, D. Hanson, M. LoVerde, C. M. Hirata, and O. Zahn, “Delensing CMB Polarization with External Datasets,” JCAP
Original
2012
Later among the works it cites.
M. Millea et al
Original
2012
Later among the works it cites.
E. Alizadeh and C. M. Hirata, “How to detect gravitational waves through the cross-correlation of the galaxy distribution with the CMB polarization,” Phys. Rev. D
Original
2012
Later among the works it cites.
S. C. Hotinli and M. C. Johnson, “Reconstructing large scales at cosmic dawn,” arXiv:2012.09851 [astro-ph.CO]

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

2003

Cited alongside, same era.

M. G. Santos, A. Cooray, Z. Haiman, L. Knox, and C.-P. Ma, “Small - scale CMB temperature and polarization anisotropies due to patchy reionization,” Astrophys. J

2003

Cited alongside, same era.

VIRGO Consortium

2003

Cited alongside, same era.

U. Seljak and C. M. Hirata, “Gravitational lensing as a contaminant of the gravity wave signal in CMB,” Phys. Rev. D

2004

Cited alongside, same era.

S. Bashinsky and U. Seljak, “Neutrino perturbations in CMB anisotropy and matter clustering,” Phys. Rev

2004

Cited alongside, same era.

K. M. Smith, W. Hu, and M. Kaplinghat, “Weak lensing of the CMB: Sampling errors on B-modes,” Phys. Rev. D

2004

Cited alongside, same era.

M. J. White, “Baryons and weak lensing power spectra,” Astropart. Phys

2004

Cited alongside, same era.