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We observed the high-mass star-forming region G335.579-0.292 with the AtacamaLarge Millimeter/submillimeter Array (ALMA) at 226 GHz with an angularresolution of 0.3'' ($\sim 1000$ au resolution at the source distance).G335.579-0.292 hosts one of the most massive cores in the Galaxy (G335-MM1).The continuum emission shows that G335-MM1 fragments into at least fivesources, while molecular line emission is detected in two of the continuumsources (ALMA1 and ALMA3). We found evidence of large and small scale infall inALMA1 revealed by an inverse P-Cygni profile and the presence of a blue-shiftedspot at the center of the first moment map of the CH$_3$CN emission. Inaddition, hot gas expansion in the innermost region is unveiled by ared-shifted spot in the first moment map of HDCO and (CH$_3$)$_2$CO (both with$E_u > 1100$ K). Our modeling reveals that this expansion motion originatesclose to the central source, likely due to reversal of the accretion flowinduced by the expansion of the HII region, while infall and rotation motionsoriginate in the outer regions. ALMA3 shows clear signs of rotation, with arotation axis inclination with respect to the line of sight close to$90^\circ$, and a system mass (disk + star) in the range of 10-30 M$_\odot$.

Digging into the Interior of Hot Cores with ALMA (DIHCA). I. Dissecting the High-mass Star-Forming Core G335.579-0.292 MM1