Built on

C. D. Kreisch, F. Y. Cyr-Racine and O. Doré, “The Neutrino Puzzle: Anomalies, Interactions, and Cosmological Tensions,” arXiv:1902.00534 [astro-ph.CO]
Original
1902
Earlier work this paper cites.
K. L. Pandey, T. Karwal and S. Das, “Alleviating the H 0 H_{0} and σ 8 \sigma_{8} anomalies with a decaying dark matter model,” arXiv:1902.10636 [astro-ph.CO]
Original
1902
Earlier work this paper cites.
S. Hanany et al
Original
1902
Earlier work this paper cites.
A. G. Riess, S. Casertano, W. Yuan, L. M. Macri and D. Scolnic, “Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM,” Astrophys. J. 876
Original
1903
Earlier work this paper cites.
G. Pietrzyński et al
Original
1903
Earlier work this paper cites.
K. Vattis, S. M. Koushiappas and A. Loeb, “Late universe decaying dark matter can relieve the H 0 H_{0} tension,” arXiv:1903.06220 [astro-ph.CO]
Original
1903
Earlier work this paper cites.
M. Park, C. D. Kreisch, J. Dunkley, B. Hadzhiyska and F. Y. Cyr-Racine, “ Λ \Lambda CDM or self-interacting neutrinos? - how CMB data can tell the two models apart,” arXiv:1904.02625 [astro-ph.CO]
Original
1904
Earlier work this paper cites.
P. Agrawal, F. Y. Cyr-Racine, D. Pinner and L. Randall, “Rock ’n’ Roll Solutions to the Hubble Tension,” arXiv:1904.01016 [astro-ph.CO]
Original
1904
Earlier work this paper cites.
S. Taubenberger et al
Original
1905
Earlier work this paper cites.
T. Collett, F. Montanari and S. Rasanen, “Model-independent determination of H 0 H_{0} and Ω K 0 \Omega_{K0} from strong lensing and type Ia supernovae,” arXiv:1905.09781 [astro-ph.CO]
Original
1905
Earlier work this paper cites.
N. Blinov, K. J. Kelly, G. Z. Krnjaic and S. D. McDermott, “Constraining the Self-Interacting Neutrino Interpretation of the Hubble Tension,” arXiv:1905.02727 [astro-ph.CO]
Original
1905
Earlier work this paper cites.
M. X. Lin, G. Benevento, W. Hu and M. Raveri, “Acoustic Dark Energy: Potential Conversion of the Hubble Tension,” arXiv:1905.12618 [astro-ph.CO]
Original
1905
Earlier work this paper cites.
L. Verde, T. Treu and A. G. Riess, “Tensions between the Early and the Late Universe,” arXiv:1907.10625 [astro-ph.CO]
Original
1907
Earlier work this paper cites.
W. L. Freedman et al
Original
1907
Earlier work this paper cites.
W. Yuan, A. G. Riess, L. M. Macri, S. Casertano and D. Scolnic, arXiv:1908.00993 [astro-ph.GA]
Original
1908
Earlier work this paper cites.
A. Manzotti, “Future cosmic microwave background delensing with galaxy surveys,” Phys. Rev. D 97
Original
1908
Earlier work this paper cites.
R. A. Sunyaev and Y. B. Zeldovich, “Small scale fluctuations of relic radiation,” Astrophys. Space Sci. 7
1970
Earlier work this paper cites.
P. J. E. Peebles and J. T. Yu, “Primeval adiabatic perturbation in an expanding universe,” Astrophys. J. 162
1970
Earlier work this paper cites.
M. Kamionkowski, D. N. Spergel and N. Sugiyama, “Small scale cosmic microwave background anisotropies as a probe of the geometry of the universe,” Astrophys. J. 426
1994
Earlier work this paper cites.
G. Jungman, M. Kamionkowski, A. Kosowsky and D. N. Spergel, “Weighing the universe with the cosmic microwave background,” Phys. Rev. Lett. 76
1996
Earlier work this paper cites.
G. Jungman, M. Kamionkowski, A. Kosowsky and D. N. Spergel, “Cosmological parameter determination with microwave background maps,” Phys. Rev. D 54
1996
Earlier work this paper cites.

Similar

M. Kamionkowski, A. Kosowsky and A. Stebbins, “Statistics of cosmic microwave background polarization,” Phys. Rev. D 55
1997
Cited alongside, same era.
M. Zaldarriaga and U. Seljak, “An all sky analysis of polarization in the microwave background,” Phys. Rev. D 55
1997
Cited alongside, same era.
M. Kamionkowski, A. Kosowsky and A. Stebbins, “A Probe of primordial gravity waves and vorticity,” Phys. Rev. Lett. 78
1997
Cited alongside, same era.
U. Seljak and M. Zaldarriaga, “Signature of gravity waves in polarization of the microwave background,” Phys. Rev. Lett. 78
1997
Cited alongside, same era.
M. Zaldarriaga and U. Seljak, “Gravitational lensing effect on cosmic microwave background polarization,” Phys. Rev. D 58
1998
Cited alongside, same era.

Then

J. L. Bernal, L. Verde and A. G. Riess, “The trouble with H 0 H_{0} ,” JCAP 1610
Original
2016
Later among the works it cites.
E. Di Valentino, A. Melchiorri and J. Silk, “Reconciling Planck with the local value of H 0 H_{0} in extended parameter space,” Phys. Lett. B 761
Original
2016
Later among the works it cites.
M. Kamionkowski and E. D. Kovetz, “The Quest for B Modes from Inflationary Gravitational Waves,” Ann. Rev. Astron. Astrophys. 54
Original
2016
Later among the works it cites.
W. L. Freedman, “Cosmology at a Crossroads,” Nat. Astron. 1
Original
2017
Later among the works it cites.
V. Bonvin et al
Original

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2019

Gravitational waves, CMB polarization, and the Hubble tension

Jeong, Donghui, Kamionkowski, Marc

Understand

The discrepancy between the Hubble parameter inferred from local measurements and that from the cosmic microwave background (CMB) has motivated careful scrutiny of the assumptions that enter both analyses.

Here we point out that the location of the recombination peak in the CMB B-mode power spectrum is determined by the light horizon at the surface of last scatter and thus provides an alternative early-Universe standard ruler.
It can thus be used as a cross-check for the standard ruler inferred from the acoustic peaks in the CMB temperature power spectrum and to test various explanations for the Hubble tension.
The measurement can potentially be carried out with a precision of $\lesssim2\%$ with stage-IV B-mode experiments.

Built on

C. D. Kreisch, F. Y. Cyr-Racine and O. Doré, “The Neutrino Puzzle: Anomalies, Interactions, and Cosmological Tensions,” arXiv:1902.00534 [astro-ph.CO]
Original
1902
Earlier work this paper cites.
K. L. Pandey, T. Karwal and S. Das, “Alleviating the H 0 H_{0} and σ 8 \sigma_{8} anomalies with a decaying dark matter model,” arXiv:1902.10636 [astro-ph.CO]
Original
1902
Earlier work this paper cites.
S. Hanany et al
Original
1902
Earlier work this paper cites.
A. G. Riess, S. Casertano, W. Yuan, L. M. Macri and D. Scolnic, “Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM,” Astrophys. J. 876
Original
1903
Earlier work this paper cites.
G. Pietrzyński et al
Original
1903
Earlier work this paper cites.
K. Vattis, S. M. Koushiappas and A. Loeb, “Late universe decaying dark matter can relieve the H 0 H_{0} tension,” arXiv:1903.06220 [astro-ph.CO]
Original
1903
Earlier work this paper cites.
M. Park, C. D. Kreisch, J. Dunkley, B. Hadzhiyska and F. Y. Cyr-Racine, “ Λ \Lambda CDM or self-interacting neutrinos? - how CMB data can tell the two models apart,” arXiv:1904.02625 [astro-ph.CO]
Original
1904
Earlier work this paper cites.
P. Agrawal, F. Y. Cyr-Racine, D. Pinner and L. Randall, “Rock ’n’ Roll Solutions to the Hubble Tension,” arXiv:1904.01016 [astro-ph.CO]
Original
1904
Earlier work this paper cites.
S. Taubenberger et al
Original
1905
Earlier work this paper cites.
T. Collett, F. Montanari and S. Rasanen, “Model-independent determination of H 0 H_{0} and Ω K 0 \Omega_{K0} from strong lensing and type Ia supernovae,” arXiv:1905.09781 [astro-ph.CO]
Original
1905
Earlier work this paper cites.
N. Blinov, K. J. Kelly, G. Z. Krnjaic and S. D. McDermott, “Constraining the Self-Interacting Neutrino Interpretation of the Hubble Tension,” arXiv:1905.02727 [astro-ph.CO]
Original
1905
Earlier work this paper cites.
M. X. Lin, G. Benevento, W. Hu and M. Raveri, “Acoustic Dark Energy: Potential Conversion of the Hubble Tension,” arXiv:1905.12618 [astro-ph.CO]
Original
1905
Earlier work this paper cites.
L. Verde, T. Treu and A. G. Riess, “Tensions between the Early and the Late Universe,” arXiv:1907.10625 [astro-ph.CO]
Original
1907
Earlier work this paper cites.
W. L. Freedman et al
Original
1907
Earlier work this paper cites.
W. Yuan, A. G. Riess, L. M. Macri, S. Casertano and D. Scolnic, arXiv:1908.00993 [astro-ph.GA]
Original
1908
Earlier work this paper cites.
A. Manzotti, “Future cosmic microwave background delensing with galaxy surveys,” Phys. Rev. D 97
Original
1908
Earlier work this paper cites.
R. A. Sunyaev and Y. B. Zeldovich, “Small scale fluctuations of relic radiation,” Astrophys. Space Sci. 7
1970
Earlier work this paper cites.
P. J. E. Peebles and J. T. Yu, “Primeval adiabatic perturbation in an expanding universe,” Astrophys. J. 162
1970
Earlier work this paper cites.
M. Kamionkowski, D. N. Spergel and N. Sugiyama, “Small scale cosmic microwave background anisotropies as a probe of the geometry of the universe,” Astrophys. J. 426
1994
Earlier work this paper cites.
G. Jungman, M. Kamionkowski, A. Kosowsky and D. N. Spergel, “Weighing the universe with the cosmic microwave background,” Phys. Rev. Lett. 76
1996
Earlier work this paper cites.
G. Jungman, M. Kamionkowski, A. Kosowsky and D. N. Spergel, “Cosmological parameter determination with microwave background maps,” Phys. Rev. D 54
1996
Earlier work this paper cites.

Similar

M. Kamionkowski, A. Kosowsky and A. Stebbins, “Statistics of cosmic microwave background polarization,” Phys. Rev. D 55
1997
Cited alongside, same era.
M. Zaldarriaga and U. Seljak, “An all sky analysis of polarization in the microwave background,” Phys. Rev. D 55
1997
Cited alongside, same era.
M. Kamionkowski, A. Kosowsky and A. Stebbins, “A Probe of primordial gravity waves and vorticity,” Phys. Rev. Lett. 78
1997
Cited alongside, same era.
U. Seljak and M. Zaldarriaga, “Signature of gravity waves in polarization of the microwave background,” Phys. Rev. Lett. 78
1997
Cited alongside, same era.
M. Zaldarriaga and U. Seljak, “Gravitational lensing effect on cosmic microwave background polarization,” Phys. Rev. D 58
1998
Cited alongside, same era.

Then

J. L. Bernal, L. Verde and A. G. Riess, “The trouble with H 0 H_{0} ,” JCAP 1610
Original
2016
Later among the works it cites.
E. Di Valentino, A. Melchiorri and J. Silk, “Reconciling Planck with the local value of H 0 H_{0} in extended parameter space,” Phys. Lett. B 761
Original
2016
Later among the works it cites.
M. Kamionkowski and E. D. Kovetz, “The Quest for B Modes from Inflationary Gravitational Waves,” Ann. Rev. Astron. Astrophys. 54
Original
2016
Later among the works it cites.
W. L. Freedman, “Cosmology at a Crossroads,” Nat. Astron. 1
Original
2017
Later among the works it cites.
V. Bonvin et al
Original

Beyond the bibliography

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

Open on alphaXiv

alphaXiv is searching for related work…

M. Kamionkowski and A. Kosowsky, “Detectability of inflationary gravitational waves with microwave background polarization,” Phys. Rev. D 57

1998

Cited alongside, same era.

A. H. Jaffe, M. Kamionkowski and L. M. Wang, “Polarization pursuers’ guide,” Phys. Rev. D 61

2000

Cited alongside, same era.

A. Lewis, A. Challinor and A. Lasenby, “Efficient computation of CMB anisotropies in closed FRW models,” Astrophys. J. 538

2000

Cited alongside, same era.

M. Kesden, A. Cooray and M. Kamionkowski, “Separation of gravitational wave and cosmic shear contributions to cosmic microwave background polarization,” Phys. Rev. Lett. 89

2002

Cited alongside, same era.

L. Knox and Y. S. Song, “A Limit on the detectability of the energy scale of inflation,” Phys. Rev. Lett. 89

2002

Cited alongside, same era.

J. R. Pritchard and M. Kamionkowski, “Cosmic microwave background fluctuations from gravitational waves: An Analytic approach,” Annals Phys. 318

2005

Cited alongside, same era.

R. Flauger and S. Weinberg, “Tensor Microwave Background Fluctuations for Large Multipole Order,” Phys. Rev. D 75

2007

Cited alongside, same era.

2017

Later among the works it cites.