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20092024
most citedNeutron Interferometry constrains dark energy chameleon fields

90 citations · 451 across the 37 of their papers we have counts for

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8 papers · 1 filter

gr-qc2021★ 20 cited

Quantum gravitational states of ultracold neutrons as a tool for probing of beyond-Riemann gravity

A. N. Ivanov, M. Wellenzohn, H. Abele

We analyze a possibility to probe beyond-Riemann gravity (BRG) contributions, introduced by Kostelecky and Li (see Phys. Rev. D 103, 024059 (2021) and Phys. Rev. D 104, 044054 (202…

gr-qc2016★ 34 cited

Einstein-Cartan Gravity with Torsion Field Serving as Origin for Cosmological Constant or Dark Energy Density

A. N. Ivanov, M. Wellenzohn

We analyse the Einstein-Cartan gravity in its standard form cal-R = R + cal-K^2, where cal-R and R are the Ricci scalar curvatures in the Einstein-Cartan and Einstein gravity, resp…

gr-qc2016★ 1 cited

Can Chameleon Field be identified with Quintessence ?

A. N. Ivanov, M. Wellenzohn

In the Einstein-Cartan gravitational theory with the chameleon field, changing its mass in dependence of a density of its environment, we analyze the Friedmann-Einstein equations f…

gr-qc2016★ 27 cited

Exact Solution for Chameleon Field, Self-Coupled Through the Ratra-Peebles Potential with n = 1 and Confined Between Two Parallel Plates

A. N. Ivanov, G. Cronenberg, R. Höllwieser +4

We calculate the chameleon field profile, confined between two parallel plates, filled with air at pressure and room temperature and separated by the dist…

gr-qc2016★ 10 cited

Spin Precession of Slow Neutrons in Einstein-Cartan Gravity with Torsion, Chameleon and Magnetic Field

A. N. Ivanov, M. Wellenzohn

We analyse a spin precession of slow neutrons in the Einstein-Cartan gravity with torsion, chameleon and magnetic field. For the derivation of the Heisenberg equation of motion of…

gr-qc2015★ 6 cited

Effective Low-Energy Potential for Slow Dirac Fermions in Einstein-Cartan Gravity with Torsion and Chameleon

A. N. Ivanov, M. Wellenzohn

We derive the most general effective low-energy potential to order O(1/m) for slow Dirac fermions with mass m, coupled to gravitational, chameleon and torsion fields in the Einstei…