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We have considered the antikaon condensation in a neutron star in thepresence of strong magnetic fields by using the modified quark-meson coupling(MQMC) model. The structure of the neutron star is investigated with variousmagnetic fields and different kaon optical potentials, and the effects of themagnetic fields for kaon condensation is discussed. When employing strongmagnetic fields inside a neutron star with hyperons and kaon condensation, themagnetic fields can cause the equation of state to be stiff; thus, a largemaximum mass of the neutron star can be obtained.

Kaon Condensation in a Neutron Star under Strong Magnetic Fields by Using the Modified Quark-meson Coupling Model