EINSTEIN-CARTAN GRAVITY WITH TORSION FIELD SERVING AS AN ORIGIN FOR THE COSMOLOGICAL CONSTANT OR DARK ENERGY DENSITY von Ivanov, A. N., Wellenzohn, M.

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Quantum gravitational states of ultracold neutrons as a tool for probing of beyond-Riemann gravity von Ivanov, A.N., Wellenzohn, M., Abele, H.

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Probing of violation of Lorentz invariance by ultracold neutrons in the Standard Model Extension von Ivanov, A.N., Wellenzohn, M., Abele, H.

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Neutron interferometry constrains dark energy chameleon fields von Lemmel, H., Brax, Ph, Ivanov, A.N., Jenke, T., Pignol, G., Pitschmann, M., Potocar, T., Wellenzohn, M., Zawisky, M., Abele, H.

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Erratum: Spin precession of slow neutrons in Einstein-Cartan gravity with torsion, chameleon, and magnetic field [Phys. Rev. D 93 , 045031 (2016)] von Ivanov, A. N., Wellenzohn, M.

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Erratum: Effective low-energy potential for slow Dirac fermions in Einstein-Cartan gravity with torsion and chameleon field [Phys. Rev. D 92 , 125004 (2015)] von Ivanov, A. N., Wellenzohn, M.

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Erratum: Tests of the standard model in neutron beta decay with polarized electrons and unpolarized neutrons and protons [Phys. Rev. D 99 , 053004 (2019)] von Ivanov, A. N., Höllwieser, R., Troitskaya, N. I., Wellenzohn, M., Berdnikov, Ya. A.

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Neutron dark matter decays and correlation coefficients of neutron β−-decays von Ivanov, A.N., Höllwieser, R., Troitskaya, N.I., Wellenzohn, M., Berdnikov, Ya.A.

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Spin precession of slow neutrons in Einstein-Cartan gravity with torsion, chameleon, and magnetic field von Ivanov, A. N., Wellenzohn, M.

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Can a Chameleon Field Be Identified with Quintessence? von Ivanov, A. N., Wellenzohn, M.

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Radiative corrections of order O ( α E e / m N ) to Sirlin’s radiative corrections of order O ( α / π ) , induced by the hadronic structure of the neutron von Ivanov, A. N., Höllwieser, R., Troitskaya, N. I., Wellenzohn, M., Berdnikov, Ya. A.

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Tests of the standard model in neutron beta decay with polarized electrons and unpolarized neutrons and protons von Ivanov, A. N., Höllwieser, R., Troitskaya, N. I., Wellenzohn, M., Berdnikov, Ya. A.

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Theoretical description of the neutron beta decay in the standard model at the level of 10 − 5 von Ivanov, A. N., Höllwieser, R., Troitskaya, N. I., Wellenzohn, M., Berdnikov, Ya. A.

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Precision analysis of pseudoscalar interactions in neutron beta decays von Ivanov, A.N., Höllwieser, R., Troitskaya, N.I., Wellenzohn, M., Berdnikov, Ya.A.

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On the correlation coefficient T(Ee) of the neutron beta decay, caused by the correlation structure invariant under discrete P, C and T symmetries von Ivanov, A.N., Höllwieser, R., Troitskaya, N.I., Wellenzohn, M., Berdnikov, Ya.A.

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Exact solution for chameleon field, self-coupled through the Ratra-Peebles potential with n = 1 and confined between two parallel plates von Ivanov, A. N., Cronenberg, G., Höllwieser, R., Jenke, T., Pitschmann, M., Wellenzohn, M., Abele, H.

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Nonrelativistic approximation of the Dirac equation for slow fermions coupled to the chameleon and torsion fields in the gravitational field of the Earth von Ivanov, A. N., Wellenzohn, M.

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Radiative corrections of order O ( α E e / m N ) to Sirlin’s radiative corrections of order O ( α / π ) to the neutron lifetime von Ivanov, A. N., Höllwieser, R., Troitskaya, N. I., Wellenzohn, M., Berdnikov, Ya. A.

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Erratum: Effective low-energy gravitational potential for slow fermions coupled to linearized massive gravity [Phys. Rev. D 92 , 105034 (2015)] von Ivanov, A. N., Pitschmann, M., Wellenzohn, M.

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Precision theoretical analysis of neutron radiative beta decay to order O ( α 2 / π 2 ) von Ivanov, A. N., Höllwieser, R., Troitskaya, N. I., Wellenzohn, M., Berdnikov, Ya. A.

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