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PERSPECTIVES<br />

770<br />

a means for further optimizing the editing<br />

performance of Cas9.<br />

Effi cient strategies for directed editing<br />

of mamm<strong>al</strong>ian genomes will enable sophisticated<br />

gen<strong>et</strong>ic engineering for both fundament<strong>al</strong><br />

and applied purposes. Especi<strong>al</strong>ly in<br />

medic<strong>al</strong> applications, high-fi delity targ<strong>et</strong> recognition<br />

is critic<strong>al</strong>, as off-site nuclease activity<br />

will jeopardize the saf<strong>et</strong>y of the engineering<br />

operation; thus, long str<strong>et</strong>ches of nucleotides<br />

should be specifi c<strong>al</strong>ly recognized. In<br />

addition, adjusting the system’s specifi city<br />

toward new targ<strong>et</strong> sequences should be easy<br />

and affordable; this is a major advantage of<br />

the Cas9 system, as it merely requires changing<br />

the sequence of the guide RNA. Further-<br />

PHYSICS<br />

Demonstrating Uncertainty<br />

Gerard J. Milburn<br />

Anyone using a modern camera is<br />

implementing an optic<strong>al</strong> position<br />

measurement. In an active autofocus<br />

camera, a pulse of infrared light is emitted<br />

from the camera, and the time taken for<br />

it to be refl ected back to the camera is used<br />

to compute the distance b<strong>et</strong>ween the object<br />

and the image plane. Imagine how diffi cult<br />

it would be to operate such a system if the<br />

object recoiled every time the<br />

infrared pulse was refl ected from<br />

it. Heisenberg suggested that this<br />

is precisely what would happen if<br />

light were used to d<strong>et</strong>ermine the<br />

position of a quantum object as<br />

accurately as his famous uncertainty<br />

principle would <strong>al</strong>low. On<br />

page 801 of this issue, Purdy <strong>et</strong><br />

<strong>al</strong>. ( 1) demonstrate this quantum<br />

back-action effect in an optic<strong>al</strong><br />

measurement of the position of a<br />

macroscopic mirror.<br />

The mechanic<strong>al</strong> action of<br />

light has long been known ( 2).<br />

Kepler suggested that the reason<br />

com<strong>et</strong> tails point away from<br />

the Sun is due to the mechanic<strong>al</strong><br />

action of light. In the early<br />

1970s, Arthur Ashkin of Bell Sign<strong>al</strong><br />

Laboratories showed that optic<strong>al</strong><br />

intensity gradients could exert a Probe<br />

force on microm<strong>et</strong>er-size parti-<br />

Centre for Engineered Quantum Systems, The<br />

University of Queensland, St Lucia, Brisbane,<br />

QLD 4072, Austr<strong>al</strong>ia. E-mail: milburn@<br />

physics.uq.edu.au<br />

more, the recombination should be fast, effi -<br />

cient, and sc<strong>al</strong>able. Compared to the most<br />

promising currently available genome editing<br />

systems (zinc fi nger domains and TAL-<br />

ENs), the RNA-guided Cas9 nuclease probably<br />

is closest to me<strong>et</strong>ing these requirements.<br />

However, effi ciency and specifi city still can<br />

be improved—for instance, by laboratory<br />

evolution. Applying these genome surgery<br />

techniques to correct human disease-associated<br />

gen<strong>et</strong>ic mutations, resulting in function<strong>al</strong><br />

gene therapy and in curing gen<strong>et</strong>ic disorders,<br />

will therefore take time. The spectacular<br />

recent development of dedicated nucleases<br />

suggests, however, that we are entering<br />

the fi n<strong>al</strong> stage of this quest.<br />

cles. This observation eventu<strong>al</strong>ly led to laser<br />

cooling and the fi eld of atom optics.<br />

The history of using optic<strong>al</strong> transducers<br />

to monitor the quantized position of an<br />

object at the Heisenberg limit goes back to<br />

the early propos<strong>al</strong>s for the optic<strong>al</strong> d<strong>et</strong>ection<br />

of gravitation<strong>al</strong> radiation ( 3). The relative<br />

length of the two orthogon<strong>al</strong> arms<br />

in a Michelson-Morley interferom<strong>et</strong>er is<br />

Incident<br />

Reflected<br />

15 FEBRUARY 2013 VOL 339 SCIENCE www.sciencemag.org<br />

Published by AAAS<br />

Transmitted<br />

Sign<strong>al</strong><br />

Probe<br />

References<br />

1. L. Cong <strong>et</strong> <strong>al</strong>., Science 339, 819 (2013);<br />

10.1126/science.1231143.<br />

2. P. M<strong>al</strong>i <strong>et</strong> <strong>al</strong>., Science 339, 823 (2013);<br />

10.1126/science.1232033.<br />

3. B. L. Stoddard, Structure 19, 7 (2011).<br />

4. F. D. Urnov, E. J. Rebar, M. C. Holmes, H. S. Zhang,<br />

P. D. Gregory, Nat. Rev. Gen<strong>et</strong>. 11, 636 (2010).<br />

5. A. J. Bogdanove, D. F. Voytas, Science 333, 1843 (2011).<br />

6. K. Eisenschmidt <strong>et</strong> <strong>al</strong>., Nucleic Acids Res. 33, 7039<br />

(2005).<br />

7. B. Wiedenheft, S. H. Sternberg, J. A. Doudna, Nature<br />

482, 331 (2012).<br />

8. E. R. Westra <strong>et</strong> <strong>al</strong>., Annu. Rev. Gen<strong>et</strong>. 46, 311 (2012).<br />

9. E. Deltcheva <strong>et</strong> <strong>al</strong>., Nature 471, 602 (2011).<br />

10. M. Jinek <strong>et</strong> <strong>al</strong>., Science 337, 816 (2012).<br />

11. G. Gasiunas, R. Barrangou, P. Horvath, V. Siksnys, Proc.<br />

Natl. Acad. Sci. U.S.A. 109, E2579 (2012).<br />

12. M. Jinek <strong>et</strong> <strong>al</strong>., elife 2013; 2:300471 (2013).<br />

10.1126/science.1234726<br />

Heisenberg’s uncertainty principle is<br />

demonstrated with a vibrating macroscopic<br />

mirror.<br />

changed by the tid<strong>al</strong> forces exerted by gravitation<strong>al</strong><br />

waves. This length difference leads<br />

to changes in the interference of light at the<br />

output mirror. Monitoring the output intensity<br />

can thus be used to measure the relative<br />

position of the end mirrors.<br />

The effect is sm<strong>al</strong>l, however, and very<br />

sm<strong>al</strong>l changes in the intensity need to be<br />

d<strong>et</strong>ected. This eventu<strong>al</strong>ly runs into a problem<br />

caused by the essenti<strong>al</strong> granular<br />

nature of light (light pulses are<br />

made up of individu<strong>al</strong> photons).<br />

Even the most carefully stabilized<br />

laser produces light with<br />

intensity fl uctuations due to the<br />

random arriv<strong>al</strong> of individu<strong>al</strong> photons,<br />

c<strong>al</strong>led shot noise. We rarely<br />

need to account for this as the relative<br />

size of the intensity fl uctuation<br />

f<strong>al</strong>ls off as the inverse square<br />

root of the intensity, so we can<br />

<strong>al</strong>ways increase the intensity to<br />

improve the sign<strong>al</strong>-to-noise ratio.<br />

But there is another problem.<br />

If we take into account the<br />

mechanic<strong>al</strong> action of light, we<br />

see that a price must be paid for<br />

An optic<strong>al</strong> cavity with a vibrating<br />

mirror. As this mirror moves, the<br />

intensity of the transmitted light can<br />

be used to monitor its position. (Ins<strong>et</strong>)<br />

When the quantum nature of light is<br />

included, the random reflection of<br />

individu<strong>al</strong> photons shakes the mirror,<br />

adding radiation pressure noise to the<br />

position measurement.<br />

on February 14, 2013<br />

www.sciencemag.org<br />

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