Recently, isomeric states are discovered for the first time in
101In,
123,125Ag, and
218Pa. The nuclear shell model is used to explain the underlying physics in these and related isomers in In, Ag isotopes, and the
N\!=\!127 isotones. The observed excitation energies of the
1/2^- isomeric states in odd-A In isotopes,
101-109In, are rather similar among five isotopes, which can be explained by introducing the strong neutron configuration mixing between the
0g_7/2 and
1d_5/2 orbitals. In addition, from the
9/2^+ ground state to the
1/2^- isomeric state in these odd-A In isotopes, a proton moves from the
1p_1/2 orbital to the
0g_9/2 orbital, which may induce the change on the single particle energies of the neutron
0g_7/2 and
1d_5/2 orbitals. Such configuration dependent shell evolution in one nucleus is called the type II shell evolution. Similar to In isotopes, the isomeric states in
123,125Ag are found to be the
1/2^- states, which correspond to a proton hole in
1p_1/2 orbital. But
1/2^- states are ground states in
115,117Ag, which indicates an inversion of the proton
1p_1/2 and
0g_9/2 orbitals around
N\!=\!72. The shell-model analysis shows that the tensor force is the key reason of the inversion of the two orbitals.
\rm A~1^- ground state and a high spin isomeric state are observed previously along the odd-odd
N\!=\!127 isotones,
210Bi,
212At,
214Fr, and
216Ac. However, the ground state and the newly discovered isomeric state of
218Pa are suggested to be
8^- and
1^-, respectively, based on the properties of
\alpha decay and the shell-model calculations. The evolution of the ground states and isomeric states along the odd-odd
N\!=\!127 isotones are caused by the transition of the proton-neutron interaction from particle-particle type to hole-particle type and the proton configuration mixing. In general, the nuclear shell model gives nice descriptions on these newly discovered isomeric states in nuclei around the doubly magic nuclei
100Sn,
132Sn, and
208Pb. The isomeric states in nuclei around doubly magic nuclei, so called the shell-model isomers, are of high importance in the nuclear structure study, because they often provide the first spectroscopic properties in the extreme neutron-rich and neutron-deficient nuclei in the medium and heavy mass region and include a plenty of information in physics, such as the proton-neutron interaction and its role in shell evolution.