“Gray molasses”的意思、由来-开放百科全书

There are many methods for sub-Doppler laser cooling of atoms to low temperatures. Among these, gray molasses is particularly efficient for atoms with poorly-resolved hyperfine structure, such as the isotopes of potassium and lithium.^[1] It combines the effects of Sisyphus cooling with a velocity-selective dark state, which prevents scattering of light by already-cold atoms.

Gray molasses relies on the presence of bright states, in which the atom interacts with the laser light, and dark states, which can be created either by using circularly polarized light on an

transition or EIT-like coherent dark states.^[2] A spatially varying light shift of the bright states allows moving atoms to undergo a Sisyphus-like cooling effect. From here, atoms can be optically pumped to dark states. The coupling between the dark and bright states is engineered so that the coldest atoms are trapped in dark states but hot atoms return to the Sisyphus cooling cycle.

Historically, gray molasses was introduced with atomic species such as rubidium^[3] and cesium^[4] on the D2 line, but has more recently been used to enable efficient cooling of potassium and lithium using the D1 line.^[1] Avoiding the need of a separate laser system, D2-line gray molasses cooling has also been demonstrated in ⁴⁰K.^[5]

References

1. ^¹{{Cite journal|last=Sievers|first=Franz|last2=Kretzschmar|first2=Norman|last3=Fernandes|first3=Diogo Rio|last4=Suchet|first4=Daniel|last5=Rabinovic|first5=Michael|last6=Wu|first6=Saijun|last7=Parker|first7=Colin V.|last8=Khaykovich|first8=Lev|last9=Salomon|first9=Christophe|date=2015-02-23|title=Simultaneous sub-Doppler laser cooling of fermionic $^{6}\\mathrm{Li}$ and $^{40}\\mathrm{K}$ on the ${D}_{1}$ line: Theory and experiment|url=https://link.aps.org/doi/10.1103/PhysRevA.91.023426|journal=Physical Review A|volume=91|issue=2|pages=023426|doi=10.1103/PhysRevA.91.023426|arxiv=1410.8545|bibcode=2015PhRvA..91b3426S}}
2. ^{{Cite journal|last=Nath|first=Dipankar|last2=Easwaran|first2=R Kollengode|last3=Rajalakshmi|first3=G.|last4=Unnikrishnan|first4=C. S.|date=2013-11-08|title=Quantum-interference-enhanced deep sub-Doppler cooling of ${}^{39}$K atoms in gray molasses|url=https://link.aps.org/doi/10.1103/PhysRevA.88.053407|journal=Physical Review A|volume=88|issue=5|pages=053407|doi=10.1103/PhysRevA.88.053407|arxiv=1305.5480|bibcode=2013PhRvA..88e3407N}}
3. ^{{Cite journal|last=Weidemüller|first=M.|last2=Esslinger|first2=T.|last3=Ol'shanii|first3=M. A.|last4=Hemmerich|first4=A.|last5=Hänsch|first5=T. W.|date=1994-01-01|title=A Novel Scheme for Efficient Cooling below the Photon Recoil Limit|url=http://stacks.iop.org/0295-5075/27/i=2/a=006|journal=EPL|language=en|volume=27|issue=2|pages=109|doi=10.1209/0295-5075/27/2/006|issn=0295-5075|bibcode=1994EL.....27..109W}}
4. ^{{Cite journal|last=Boiron|first=D.|last2=Triché|first2=C.|last3=Meacher|first3=D. R.|last4=Verkerk|first4=P.|last5=Grynberg|first5=G.|date=1995-11-01|title=Three-dimensional cooling of cesium atoms in four-beam gray optical molasses|url=https://link.aps.org/doi/10.1103/PhysRevA.52.R3425|journal=Physical Review A|volume=52|issue=5|pages=R3425–R3428|doi=10.1103/PhysRevA.52.R3425|bibcode=1995PhRvA..52.3425B}}
5. ^{{Cite journal|last=Bruce|first=G. D.|last2=Haller|first2=E.|last3=Peaudecerf|first3=B.|last4=Cotta|first4=D. A.|last5=Andia|first5=M.|last6=Wu|first6=S.|last7=Johnson|first7=M. Y. H.|last8=Lovett|first8=B. W.|last9=Kuhr|first9=S.|date=2017-01-01|title=Sub-Doppler laser cooling of 40 K with Raman gray molasses on the $D_2$ line|url=http://stacks.iop.org/0953-4075/50/i=9/a=095002|journal=Journal of Physics B: Atomic, Molecular and Optical Physics|language=en|volume=50|issue=9|pages=095002|arxiv=1612.04583|doi=10.1088/1361-6455/aa65ea|issn=0953-4075|bibcode=2017JPhB...50i5002B}}