BEGIN:VCALENDAR VERSION:2.0 PRODID:-//Drupal iCal API//EN X-WR-CALNAME:Events items teaser X-WR-TIMEZONE:America/Toronto BEGIN:VTIMEZONE TZID:America/Toronto X-LIC-LOCATION:America/Toronto BEGIN:DAYLIGHT TZNAME:EDT TZOFFSETFROM:-0500 TZOFFSETTO:-0400 DTSTART:20230312T070000 END:DAYLIGHT BEGIN:STANDARD TZNAME:EST TZOFFSETFROM:-0400 TZOFFSETTO:-0500 DTSTART:20231105T060000 END:STANDARD END:VTIMEZONE BEGIN:VEVENT UID:682a198692399 DTSTART;TZID=America/Toronto:20240124T120000 SEQUENCE:0 TRANSP:TRANSPARENT DTEND;TZID=America/Toronto:20240124T130000 URL:/institute-for-quantum-computing/events/iqc-student -seminar-featuring-everett-patterson SUMMARY:IQC Student Seminar Featuring Everett Patterson CLASS:PUBLIC DESCRIPTION:Summary \n\nUNRUH PHENOMENA AND THERMALIZATION FOR QUDIT DETECT ORS\n\nQuantum-Nano Centre\, 200 University Ave West\, Room QNC 1201 Water loo\,\nON CA N2L 3G1\n\nThe Unruh effect is the flat space analogue to Haw king radiation\,\ndescribing how an observer in flat spacetime perceives t he quantum\nvacuum state to be in a thermal state when moving along a cons tantly\naccelerated trajectory. This effect is often described operational ly\nusing the qubit-based Unruh-DeWitt detector.\n\nWe study Unruh phenome na for more general qudit detectors coupled to a\nquantized scalar field\, noting the limitations to the utility of the\ndetailed balance condition as an indicator for Unruh thermality of\nhigher-dimensional qudit detector models. We illustrate these\nlimitations using two types of qutrit detect or models based on the\nspin-1 representations of SU(2) and the non-Hermit ian generalization\nof the Pauli observables (the Heisenberg-Weyl operator s).\n\n[2309.04598] Unruh phenomena and thermalization for qudit detectors \n(arxiv.org) [https://arxiv.org/abs/2309.04598]\n DTSTAMP:20250518T173150Z END:VEVENT END:VCALENDAR