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The structure of neutron-rich Cr isotopes is systematically investigated by using the spherical shell model. The calculations reproduce well the known energy levels for the even-even Cr and odd-mass Cr nuclei, and predict a lowering of excitation energies around neutron number N=40. The calculated systematics shows a pronounced collectivity around N=40; a similar characteristic behavior has been suggested for Zn and Ge isotopes. Causes for the sudden drop of the energy in Cr and the appearance of very low states around N=40 are discussed. We also predict a new band with strong collectivity built on the state in the N=40 isotope Cr.

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