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We here discuss a new model of $\gamma$-ray bursts (GRBs) based ondifferentially rotating strange stars. Strange stars in this model anddifferentially rotating neutron stars in the Klu\'zniak-Ruderman model canproduce extremely relativistic, variable fireballs required by GRBs and thenbecome millisecond pulsars. The effect of such pulsars on expansion of thepostburst fireballs through magnetic dipole radiation is studied. We show thatthese two models can explain naturally not only various features of GRBs butalso light curves of afterglows.Comment: 10 pages + 1 figure, Latex file, Physical Review Letters (accepted

physical review letters

<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="italic">γ</mml:mi></mml:math>-Ray Bursts and Afterglows from Rotating Strange Stars and Neutron Stars

γ-Ray Bursts and Afterglows from Rotating Strange Stars and Neutron Stars