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The primary concern of this contribution is that accreting millisecondpulsars (AMXPs) show a much larger amount of information than is commonlybelieved. The three questions to be addressed are: 1. Is the apparent spintorque observed in AMXPs real ? 2. Why do we see correlations andanti-correlations between fractional amplitudes and timing residuals in someAMXPs ? 3. Why the timing residuals, the lightcurve and the 1Hz QPO in SAXJ1808.4$-$3658 are related ?

Motion of the hot spot and spin torque in accreting millisecond pulsars