Abstract

Oscillations of neutral meson (K0-\( \overline {K^0 } \), D0-\( \overline {D^0 } \), and B0-\( \overline {B^0 } \) are extremely sensitive to the meson and antimeson energies at rest. This energy is determined as mc2—with the corresponding inertial mass—and as the energy of gravitational interaction. Assuming that the CPT theorem is correct for inertial masses and estimating the gravitational potential for which the largest contribution originates from the field of the galaxy center, we obtain the estimate from experimental data on K0-\( \overline {K^0 } \) oscillations: $$ \left| {\left( {\frac{{m_g }} {{m_i }}} \right)_{K^0 } - \left( {\frac{{m_g }} {{m_i }}} \right)_{\overline {K^0 } } } \right| \leqslant 8 \times 10^{ - 13} , at C.L. = 90\% $$ . This estimate is model dependent; in particular, it depends on the method used to estimate the gravitational potential. An analysis of K0-\( \overline {K^0 } \), D0-\( \overline {D^0 } \), and B0-\( \overline {B^0 } \) oscillations provides weaker but model independent estimates which, in particular, eliminate the possibility of antigravity for antimatter.

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