Built on

S. Deser and E. Witten, Dynamical Properties of Antisymmetric Tensor Fields
1981
Earlier work this paper cites.
J. Preskill, M. B. Wise, and F. Wilczek, Cosmology of the Invisible Axion
1983
Earlier work this paper cites.
L. F. Abbott and P. Sikivie, A Cosmological Bound on the Invisible Axion
1983
Earlier work this paper cites.
M. Dine and W. Fischler, The Not So Harmless Axion
1983
Earlier work this paper cites.
G. Lazarides, R. K. Schaefer, D. Seckel, and Q. Shafi, Dilution of Cosmological Axions by Entropy Production
1990
Earlier work this paper cites.
B. de Carlos, J. Casas, F. Quevedo, and E. Roulet, Model independent properties and cosmological implications of the dilaton and moduli sectors of 4-d strings
1993
Earlier work this paper cites.
T. Banks, D. B. Kaplan, and A. E. Nelson, Cosmological implications of dynamical supersymmetry breaking
1994
Earlier work this paper cites.
V. Balasubramanian, P. Berglund, J. P. Conlon, and F. Quevedo, Systematics of moduli stabilisation in Calabi-Yau flux compactifications
2005
Earlier work this paper cites.
J. P. Conlon, F. Quevedo, and K. Suruliz, Large-volume flux compactifications: Moduli spectrum and D3/D7 soft supersymmetry breaking
Original
2005
Earlier work this paper cites.

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Then

T. Higaki and F. Takahashi, Dark Radiation and Dark Matter in Large Volume Compactifications
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2012
Later among the works it cites.
M. Cicoli, J. P. Conlon, and F. Quevedo, Dark Radiation in LARGE Volume Models
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J. P. Conlon and M. C. D. Marsh, The Cosmophenomenology of Axionic Dark Radiation
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S. Angus, J. P. Conlon, U. Haisch, and A. J. Powell, Loop corrections to Δ N e f f \Delta N_{eff} in large volume models
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2015

The Axiverse induced Dark Radiation Problem

Acharya, Bobby Samir, Pongkitivanichkul, Chakrit

Understand

The string/$M$ theory Axiverse -- a plethora of very light Axion Like Particles (ALPs) with a vast range of masses -- is arguably a generic prediction of string/$M$ theory.

String/$M$ theory also tends to predict that the early Universe is dominated by moduli fields.
When the heavy moduli decay, before nucleosynthesis, they produce dark radiation in the form of relativistic ALPs.
Generically one estimates that the number of relativistic species grows with the number of axions in the Axiverse, in contradiction to the observations that $N_{eff} \leq 4$.

Built on

S. Deser and E. Witten, Dynamical Properties of Antisymmetric Tensor Fields
1981
Earlier work this paper cites.
J. Preskill, M. B. Wise, and F. Wilczek, Cosmology of the Invisible Axion
1983
Earlier work this paper cites.
L. F. Abbott and P. Sikivie, A Cosmological Bound on the Invisible Axion
1983
Earlier work this paper cites.
M. Dine and W. Fischler, The Not So Harmless Axion
1983
Earlier work this paper cites.
G. Lazarides, R. K. Schaefer, D. Seckel, and Q. Shafi, Dilution of Cosmological Axions by Entropy Production
1990
Earlier work this paper cites.
B. de Carlos, J. Casas, F. Quevedo, and E. Roulet, Model independent properties and cosmological implications of the dilaton and moduli sectors of 4-d strings
1993
Earlier work this paper cites.
T. Banks, D. B. Kaplan, and A. E. Nelson, Cosmological implications of dynamical supersymmetry breaking
1994
Earlier work this paper cites.
V. Balasubramanian, P. Berglund, J. P. Conlon, and F. Quevedo, Systematics of moduli stabilisation in Calabi-Yau flux compactifications
2005
Earlier work this paper cites.
J. P. Conlon, F. Quevedo, and K. Suruliz, Large-volume flux compactifications: Moduli spectrum and D3/D7 soft supersymmetry breaking
Original
2005
Earlier work this paper cites.