Quantum systems without a classical limit refer to systems that do not exhibit classical behavior even as they scale up in size. Examples include spin one-half particles and systems of coupled spin one-halfs. The concept challenges the notion that large quantum systems must eventually conform to classical physics. A white dwarf star exemplifies this idea, as it behaves quantum mechanically despite containing a vast number of particles, yet can transition to a classical state under certain conditions. The discussion highlights the complexity of defining classical limits in quantum mechanics.
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wdlang
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in the literature, people are talking about 'quantum systems without a classical limit'
Spin one-half. Or a system of coupled spin one-halfs.
#4
Ken G
Gold Member
4,949
573
I'm not sure what is meant by "no classical limit." A white dwarf star in a sense is not a classical limit, even though it is a huge number of particles, but if you heat it up high enough it would explode and be a very classical type Ia supernova.
Time reversal invariant Hamiltonians must satisfy ##[H,\Theta]=0## where ##\Theta## is time reversal operator. However, in some texts (for example see Many-body Quantum Theory in Condensed Matter Physics an introduction, HENRIK BRUUS and KARSTEN FLENSBERG, Corrected version: 14 January 2016, section 7.1.4) the time reversal invariant condition is introduced as ##H=H^*##. How these two conditions are identical?