TY - JOUR

T1 - Lunar laser ranging constraints on nonminimally coupled dark energy and standard sirens

AU - Tsujikawa, Shinji

N1 - Funding Information:
The author thanks Michele Maggiore for useful discussions. The author is supported by the Grant-in-Aid for Scientific Research Fund of the JSPS No. 16K05359 and MEXT KAKENHI Grant-in-Aid for Scientific Research on Innovative Areas “Cosmic Acceleration” (No. 15H05890).
Publisher Copyright:
© 2019 American Physical Society.

PY - 2019/8/6

Y1 - 2019/8/6

N2 - In dark energy models where a scalar field φ is coupled to the Ricci scalar R of the form e-2Q(φ-φ0)/MplR, where Q is a coupling constant, φ0 is today's value of φ, and Mpl is the reduced Planck mass, we study how the recent Lunar Laser Ranging (LLR) experiment places constraints on the nonminimal coupling from the time variation of gravitational coupling. Besides a potential of the light scalar responsible for cosmic acceleration, we take a cubic Galileon term into account to suppress fifth forces in overdensity regions of the Universe. Even if the scalar-matter interaction is screened by the Vainshtein mechanism, the time variation of gravitational coupling induced by the cosmological background field φ survives in the solar system. For a small Galileon coupling constant β3, there exists a kinetically driven φ-matter-dominated-epoch (φMDE) prior to cosmic acceleration. In this case, we obtain the stringent upper limit Q≤3.4×10-3 from the LLR constraint. For a large β3 without the φMDE, the coupling Q is not particularly bounded from above, but the cosmological Vainshtein screening strongly suppresses the time variation of φ such that the dark energy equation of state wDE reaches the value close to -1 at high redshifts. We study the modified gravitational wave propagation induced by the nonminimal coupling to gravity and show that, under the LLR bound, the difference between the gravitational wave and luminosity distances does not exceed the order 10-5 over the redshift range 0

AB - In dark energy models where a scalar field φ is coupled to the Ricci scalar R of the form e-2Q(φ-φ0)/MplR, where Q is a coupling constant, φ0 is today's value of φ, and Mpl is the reduced Planck mass, we study how the recent Lunar Laser Ranging (LLR) experiment places constraints on the nonminimal coupling from the time variation of gravitational coupling. Besides a potential of the light scalar responsible for cosmic acceleration, we take a cubic Galileon term into account to suppress fifth forces in overdensity regions of the Universe. Even if the scalar-matter interaction is screened by the Vainshtein mechanism, the time variation of gravitational coupling induced by the cosmological background field φ survives in the solar system. For a small Galileon coupling constant β3, there exists a kinetically driven φ-matter-dominated-epoch (φMDE) prior to cosmic acceleration. In this case, we obtain the stringent upper limit Q≤3.4×10-3 from the LLR constraint. For a large β3 without the φMDE, the coupling Q is not particularly bounded from above, but the cosmological Vainshtein screening strongly suppresses the time variation of φ such that the dark energy equation of state wDE reaches the value close to -1 at high redshifts. We study the modified gravitational wave propagation induced by the nonminimal coupling to gravity and show that, under the LLR bound, the difference between the gravitational wave and luminosity distances does not exceed the order 10-5 over the redshift range 0

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U2 - 10.1103/PhysRevD.100.043510

DO - 10.1103/PhysRevD.100.043510

M3 - Article

AN - SCOPUS:85072174345

SN - 2470-0010

VL - 100

JO - Physical Review D

JF - Physical Review D

IS - 4

M1 - 043510

ER -