(he/him)
Google Scholar: https://scholar.google.com/citations?user=GRSIcsEAAAAJ
GitHub: https://github.com/Christopher-K-Long
ORCiD: https://orcid.org/0009-0001-3230-942X
In the stack I retain the sinc terms. You can either approx these as delta function first or just integrate the probability over the emission frequency. This will give total probability of emission after a time t.
In the stack I retain the sinc terms. You can either approx these as delta function first or just integrate the probability over the emission frequency. This will give total probability of emission after a time t.
www.karlin.mff.cuni.cz/~holub/soubo...
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www.karlin.mff.cuni.cz/~holub/soubo...
(4/4)
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Kitaev introduced the phase estimation with a single output bit (arxiv.org/abs/quant-ph...).
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Kitaev introduced the phase estimation with a single output bit (arxiv.org/abs/quant-ph...).
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physics.stackexchange.com/a/649933/305...
Keep the emission term instead. Also you will probably need more than minimal couping to the EM field to get the spin flip on emission.
physics.stackexchange.com/a/649933/305...
Keep the emission term instead. Also you will probably need more than minimal couping to the EM field to get the spin flip on emission.
pypi.org/project/py-s...
pypi.org/project/py-s...
go.bsky.app/357wFNf
go.bsky.app/KBgRwmZ
~got bored this afternoon, do forgive me. But on a serious note would love to know who I haven't discovered on here yet (or mistakenly omitted due to the sheer amount of people)
go.bsky.app/AUTn1di