Science-2007-Nagaosa-758-9.pdf

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DOI: 10.1126/science.1150199 , 758 (2007); 318 Science Naoto Nagaosa A New State of Quantum Matter  This copy is for your personal, non-commercial use only.  clicking here. colleagues, clients, or customers by , you can order high-quality copies for your If you wish to distribute this articl e to others here. following the guidelines can be obtained by Permission to republish or repurpose articles or portions of articles   ): July 5, 2013 www.sciencemag.org (this information is current as of The following resources related to this article are available online at  http://www.sciencemag.org/content/318/5851/758.full.html version of this article at: including high-resolution figures, can be found in the online Updated information and services, http://www.sciencemag.org/content/318/5851/758.full.html#ref-list-1 , 5 of which can be accessed free: cites 15 articles This article 5 article(s) on the ISI Web of Science cited by This article has been http://www.sciencemag.org/content/318/5851/758.full.html#related-urls 1 articles hosted by HighWire Press; see: cited by This article has been http://www.sciencemag.org/cgi/collection/app_physics Physics, Applied subject collections: This article appears in the following registered trademark of AAAS. is a Science 2007 by the American Association for the Advancement of Science; all rights reserved. The title Copyright American Association for the Advancement of Science, 1200 New York Avenue NW, Washington, DC 20005. (print ISSN 0036-8075; online ISSN 1095-9203) is published weekly, except the last week in December, by the Science   o   n    J   u    l   y    5  ,    2    0    1    3   w   w   w  .   s   c    i   e   n   c   e   m   a   g  .   o   r   g    D   o   w   n    l   o   a    d   e    d    f   r   o   m  

Transcript of Science-2007-Nagaosa-758-9.pdf

 

DOI: 10.1126/science.1150199, 758 (2007);318Science 

Naoto NagaosaA New State of Quantum Matter

 This copy is for your personal, non-commercial use only.

 clicking here.colleagues, clients, or customers by, you can order high-quality copies for yourIf you wish to distribute this articl e to others

here.following the guidelines

can be obtained byPermission to republish or repurpose articles or portions of articles

  ): July 5, 2013 www.sciencemag.org (this information is current as of 

The following resources related to this article are available online at 

 http://www.sciencemag.org/content/318/5851/758.full.htmlversion of this article at:

including high-resolution figures, can be found in the onlineUpdated information and services,

http://www.sciencemag.org/content/318/5851/758.full.html#ref-list-1, 5 of which can be accessed free:cites 15 articlesThis article

5 article(s) on the ISI Web of Sciencecited byThis article has been

http://www.sciencemag.org/content/318/5851/758.full.html#related-urls1 articles hosted by HighWire Press; see:cited byThis article has been

http://www.sciencemag.org/cgi/collection/app_physicsPhysics, Applied

subject collections:This article appears in the following

registered trademark of AAAS.is aScience 2007 by the American Association for the Advancement of Science; all rights reserved. The title

CopyrightAmerican Association for the Advancement of Science, 1200 New York Avenue NW, Washington, DC 20005.(print ISSN 0036-8075; online ISSN 1095-9203) is published weekly, except the last week in December, by theScience 

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2 NOVEMBER 2007 VOL 318 SCIENCE www.sciencemag.org758

PERSPECTIVES

lation will predominate, and more and more

ST-KaiC will build up. As the concentration of 

ST-KaiC increases, S-KaiC will increase too.

The increasing S-KaiC will sequester more

and more KaiA, which increases the rate of 

formation of S-KaiC. This then causes more

sequestration of KaiA, and so on. Eventually

dephosphorylation dominates, and the system

is driven back to unphosphorylated KaiC.

What, then, flips the KaiA/S-KaiC switch

 back to release KaiA and favor phosphoryla-

tion? With KaiA sequestered, S-KaiC forma-

tion cannot be maintained indefinitely; the

rate of S-KaiC production from its immediate

 precursor ST-KaiC will eventually slow down

as ST-KaiC becomes depleted. This effect is

the equivalent of a slow negative-feedback 

loop—an increase in S-KaiC concentration

decreases the amount of ST-KaiC, which

decreases the rate of formation of S-KaiC.

Thus, the circadian oscillator system can

 be thought of as a bistable switch, toggled first

 by the slow accumulation of S-KaiC and then

 by a slow negative-feedback loop. This type of 

circuit can oscillate, as Rust et al . demonstrate

through a simple differential equation model

whose parameters are constrained by their 

experimental observations.

At first glance, the circadian oscillator of 

eukaryotes does not seem to work in the same

way. It is composed mainly of transcriptional

regulators and directed protein degradation

(6 ), rather than a stoichiometrically controlled 

autophosphorylating adenosine triphospha-

tase like KaiC, and none of the eukaryotic

components have any sequence homology to

KaiA, KaiB, or KaiC. On the other hand,

the design principles of the two oscillators

may be quite similar. Both circuits include

double–negative-feedback loops that might

function as bistable triggers, and both

include slow negative-feedback loops (8). In

terms of systems-level logic, these oscilla-

tors appear more similar than different.

Maybe this is how a successful circadian

oscillator has to be built.

References1. M. Nakajima et al., Science 308, 414 (2005).2. T. Nishiwaki et al., EMBO J. 26, 4029 (2007).3. M. J. Rust, J. S. Markson, W. S. Lane, D. S. Fisher, E. K.

O’Shea, Science 318, 809 (2007); published online 4October 2007 (10.1126/science.1148596).

4. J. E. Ferrell Jr., R. R. Bhatt, J. Biol. Chem. 272, 19008(1997).

5. Y. Zhao, Z. Y. Zhang, J. Biol. Chem. 276, 32382(2001).

6. S. M. Reppert, D. R. Weaver, Nature 418, 935 (2002).

10.1126/science.1150740

Electrons have a property known as spin,

and these spins can be controlled and 

directed by applied electric and mag-

netic fields. In recent years, researchers in the

relatively young field of spintronics have

explored this effect for applications in micro-

electronics [reviewed in (1)]. The goal is to

control and use spins much as today’s inte-

grated circuits use the property of electric

charge for computing operations. On page

766 of this issue, Königet al . (2) report exper-

imental results that show the existence of a

new state of matter that may take spintronics

even further. Not only does this work offer us

a look at fundamentally new physical phe-

nomena, it may also allow the development of 

novel spintronics devices.

Many researchers have explored the so-

called spin Hall effect as a possible route to

spintronic applications. The original Hall effect

goes back to the late 1800s, when Edwin Hall

noticed that a voltage would form perpendicu-

larly to a current flowing in a conductor in a

magnetic field. In the quantum Hall effects,

which were discovered in the 1980 and 1982,

the electrical conductance takes on quantized 

values. In the spin Hall effect, the direction of 

the flow of electrons can be controlled, depend-

ing on whether the spin is up or down, by an

applied electric field. The spin Hall effect was

 proposed theoretically long ago based on an

“extrinsic” mechanism (3), in which impurities

in a material deflect the spin-up and spin-down

electrons in opposite ways. However, recent

interest has centered on an intrinsic form of 

spin Hall effect and the possibility of spin flow

without energy dissipation.

Instead of impurities, the intrinsic mecha-

nism relies on the interplay of the spin and 

orbital motion of the electrons in the perfect

 periodic background of the crystal lattice,

leading to different paths for the up and down

spins. The theoretical proposals for this effect

(4, 5) were followed by the experimental dis-

covery of the spin Hall effect in GaAs (6, 7 )

and also in metallic systems

(8 – 10). However, the detailed 

mechanism in these cases still

needs to be scrutinized; the

flow of charges can still be

distorted by impurity scatter-

ing and thus contribute to

the spin current. Therefore, we

need to obtain clear obser-

vations of a truly dissipation-

less spin current.

Dissipationless flow is known

to occur in the conventional

quantum Hall effect, where the

electrons are deflected into cir-

cular paths by a magnetic field 

(see the left panel of the figure).

This motion is not random among electrons

 but is coherently organized, leading to a collec-

tive state. This state is stable because a finite

amount of energy (the energy gap) is required 

to disturb it. In a real sample, the electrons

 bounce back from the edges, causing a net one-

dimensional motion, which corresponds to a

flow of current around the edge. Because the

direction of this motion is one-way, it cannot

 be scattered backward, and so the dissipation

of the flow of charge is suppressed in the quan-

tum Hall system.

A crucial question is whether a similar 

state is possible for the spin current. My col-

leagues and I studied this question theoreti-

cally in 2004 (11), and we considered the spin

A New State of Quantum MatterNaoto Nagaosa

PHYSICS

The author is in the Department of Applied Physics,University of Tokyo, Tokyo 113-8656, Japan. E-mail:[email protected]

Magnetic field

Spin up

Spin down

Quantum Hall system Quantum spin Hall system

Spin control. In the conventional quantum Hall system (left), theapplied magnetic field causes electrons to bounce off the edge of thesample in circular orbits, forming a net flow of charge around theboundary of the material. No magnetic field is needed, however, inthe quantum spin Hall system (right), where spin-up and spin-downcarriers flow in opposite directions in edge channel states.

Experiments show that electron spins can

flow without dissipation in a novel electrical

insulator.

Published by AAAS

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Hall conductivity for a band insulator with a

finite band gap caused by the spin-orbit inter-

action. In this case, the electrons have a veloc-

ity transverse to the external electric field and 

a direction that depends on the spin. That is,

the spin currents in the totally occupied bands

do not cancel each other out, and finite spin

Hall conductivity results even in the band 

insulator. This state was called a spin Hall

insulator, and the candidate materials we pro-

 posed included HgTe, HgSe, HgS, PbTe,

PbSe, and PbS. However, it was not clear how

to fundamentally distinguish these materials

from the usual band insulators.

Kane and Mele (12, 13) achieved a break-

through when they invented a model for 

graphene with spin-orbit interaction, which

revealed an insulating state with robust helical

edge modes, i.e., the modes with opposite

spins have opposite directions of propagation.

When the number of these helical edge modes

is even, some perturbation induces the hy-

 bridization of these helical modes and hinders

their propagation. This does not occur for an

odd number of modes, where the propagation

is stable and protected (see the right panel of 

the figure). The latter case corresponds to a

new class of band insulator, i.e., the quantum

spin Hall system, and the former to the usual

insulator (12, 13).

Soon after these results, Berneviget al . (14)

 proposed a different way to create a quantum

spin Hall system. They looked at the problem

as a phase transition between the conventional

insulator and the quantum spin Hall system. It

turned out that the phase transition is accompa-

nied by a “band crossing,” which changes the

number of helical edge modes. Furthermore,

they proposed a specific system, i.e., the quan-

tum well of CdTe/HgTe/CdTe, where this

 phase transition could be induced by changing

the thickness of the HgTe layer. This was a

strong proposal and appealing enough to moti-

vate experimentalists to try testing it.

König et al . now report the experimental

observation of these robust helical edge

modes. They fabricated quantum well struc-

tures and changed the thickness d of the HgTe

layer. As d increases, the energy gap decreases

and eventually collapses at a critical thickness

of d c

= 6.3 nm. This gap closing corresponds

to the quantum phase transition between the

usual insulator atd < d cand quantum spin Hall

state at d > d c. König et al . confirmed this by

measuring the expected quantized charge con-

ductance consistently with a helical mode for 

each of the two edges, while observing a much

smaller conductance at smaller thickness,

indicating the usual insulating state.

This conclusion is further reinforced by the

magnetic field dependence of the charge con-

ductance. The conductance should show a rapid 

decrease as the magnetic field  B increases,

which König et al . also observed experimen-

tally. In this case, the authors did not directly

measure the spin Hall conductance, which is not

“quantized.” This is because, unlike the charge,

the total spin is not a conserved quantity in

the presence of the spin-orbit interaction.

Therefore, although the search for the intrinsic

spin Hall effect in the insulator leads to a new

classification of the electron states in solids, the

implications for the magneto-transport proper-

ties still remain to be studied.

The impact of this work will be far-reach-

ing because it has revealed that there are fun-

damentally different kinds of insulators. Even

after 80 years, the band theory of materials

still has new and surprising aspects. A more

complete classification scheme for these

unusual insulating states is now being con-

structed, including the three-dimensional sys-

tems (15). Eventually, the quantum spin Hall

system might enable the design of spin current

circuits without dissipation, which will open

up new possibilities in spintronics.

References and Notes

1. S. A. Wolf et al., Science 294, 1488 (2001).2. M. König et al., Science 318, 766 (2007); published

online 20 September 2007 (10.1126/science.1148047).3. M. I. D’yakonov, V. I. Perel’,  JETP Lett . 13, 467 (1971).4. S. Murakami, N. Nagaosa, S.-C. Zhang, Science 301,

1348 (2003).5. J. Sinova et al., Phys. Rev. Lett. 92, 126603 (2004).6. Y. K. Kato, R. C. Myers, A. C. Gossard, D. D. Awschalom,

 Science 306, 1910 (2004).7. J. Wunderlich, B. Kaestner, J. Sinova, T. Jungwirth, Phys.

Rev. Lett . 94, 047204 (2005).8. S. O. Valenzuela, M. Tinkham, Nature 442, 176 (2006).9. E. Saitoh, M. Ueda, H. Miyajima, G. Tatara, Appl. Phys.

Lett. 88, 182509 (2006).10. T. Kimura et al., Phys. Rev. Lett . 98, 249901 (2007).11. S. Murakami, N. Nagaosa, S.-C. Zhang, Phys. Rev. Lett.

93, 156804 (2004).12. C. L. Kane, E. J. Mele, Phys. Rev. Lett . 95, 146802

(2005).13. C. L. Kane, E. J. Mele, Phys. Rev. Lett. 95, 226801

(2005).14. B. A. Bernevig, T. L. Hughes, S.-C. Zhang, Science 314,

1757 (2006).15. L. Fu, C. L. Kane, Phys. Rev. B 76, 045302 (2007).16. I acknowledge financial support from the Grant-in-Aids

under grant numbers 15104006, 16076205, and17105002, and National Research Grid InitiativeNanoscience Project from the Ministry of Education,Culture, Sports, Science, and Technology, Japan.

10.1126/science.1150199

www.sciencemag.org SCIENCE  VOL 318 2 NOVEMBER 2007 759

PERSPECTIVES

A new generation of telescopes is helping researchers explore transient energetic processes

outside our Galaxy.

Mining for the EphemeralGeoffrey C. Bower

ASTRONOMY  

O bserved at radio wavelengths, the sky

has revealed in recent years that it

 plays host to a zoo of variable and 

transient sources that pulse, flicker, burst, and 

 burp. In the most recent manifestation of 

such ephemeral phenomena, Lorimer et al .

(1) report on page 777 of this issue the dis-

covery of a single radio burst so intense that it

overloaded the detector of the Parkes Radio

Telescope in Australia.

The authors argue that the burst originated 

outside of the Galaxy, possibly at a distance

of more than 1 billion light years. This indi-

cates an enormous and unprecedented lumi-

nosity as well as possibly providing a new

method for studying the intergalactic medium

(IGM), one of the most poorly characterized 

constituents of the universe. More detections

could give the first complete census of 

 baryons (i.e., particles such as protons and 

neutrons) in the IGM, which is believed to

account for 90% of the total baryons in the

universe. On the basis of the small sliver of 

sky and the limited sampling time that led to

this discovery, it appears that hundreds of sim-

ilar events occur throughout the sky every day.

The burst heralds a new era of transient dis-

covery at radio and other wavelengths, driven

 by new telescopes and advanced technology

for performing and analyzing enormous sur-

veys of the sky.

In the past century, astronomers escaped 

the limited spectrum visible to the human eye

and developed instruments capable of observ-

ing wavelengths from radio waves to gamma

rays. As a result, researchers have made

numerous discoveries including the micro-

wave background, pulsars, massive black 

holes, and gamma-ray bursts. Although the

static sky has not been fully explored, the

objects that vary over time represent the new

terra incognita of astronomy. The available

 parameter space is vast: Transient events are

observed at all wavelengths, in a wide variety

The author is in the Department of Astronomy, Universityof California, 601 Campbell Hall, Berkeley, CA 94720,USA. E-mail: [email protected]

Published by AAAS

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