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Proceedings of International Conference on Physics in ... - KEK

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REACHING THE SCHWINGER LIMIT WITH X-RAYS*<br />

Charles K. Rhodes, John Boguta, Alex B. Borisov, Shahab F. Khan, James W. L<strong>on</strong>gworth, John C.<br />

McCork<strong>in</strong>dale, Sankar Poopalas<strong>in</strong>gam, Erv<strong>in</strong> Racz # and Ji Zhao<br />

Laboratory for X-ray Microimag<strong>in</strong>g and Bio<strong>in</strong>formatics, Department <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>Physics</strong>, University <str<strong>on</strong>g>of</str<strong>on</strong>g><br />

Ill<strong>in</strong>ois at Chicago, Chicago, IL 60607-7059, USA<br />

Abstract<br />

The derivati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> an elementary figure <str<strong>on</strong>g>of</str<strong>on</strong>g> merit shows<br />

that atta<strong>in</strong>ment <str<strong>on</strong>g>of</str<strong>on</strong>g> an <strong>in</strong>tensity corresp<strong>on</strong>d<strong>in</strong>g to the<br />

Schw<strong>in</strong>ger/Heisenberg Limit (~ 4.6 x 10 29 W/cm 2 ) is<br />

significantly facilitated by the use <str<strong>on</strong>g>of</str<strong>on</strong>g> coherent x-ray<br />

sources <strong>in</strong> the kiloelectr<strong>on</strong>volt regime. For the Xe(L)<br />

system at ~ 4.5 keV, a m<strong>in</strong>imum pulse energy <str<strong>on</strong>g>of</str<strong>on</strong>g> ~ 1.5 J<br />

and corresp<strong>on</strong>d<strong>in</strong>g peak power P0 ~ 300 PW are estimated.<br />

INTRODUCTION<br />

The history <str<strong>on</strong>g>of</str<strong>on</strong>g> high-<strong>in</strong>tensity n<strong>on</strong>l<strong>in</strong>ear <strong>in</strong>teracti<strong>on</strong>s, that<br />

commenced <strong>in</strong> 1961 with the observati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> sec<strong>on</strong>d<br />

harm<strong>on</strong>ic radiati<strong>on</strong> [1] at 347.2 nm <strong>in</strong> crystall<strong>in</strong>e quartz,<br />

spans a range <str<strong>on</strong>g>of</str<strong>on</strong>g> ~ 10 18 <strong>in</strong> experimental <strong>in</strong>tensity and<br />

rema<strong>in</strong>s a stable, robust prov<strong>in</strong>ce <str<strong>on</strong>g>of</str<strong>on</strong>g> laser-based research<br />

after a half century. The generati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> focal <strong>in</strong>tensities <strong>in</strong><br />

the 10 20 -10 21 W/cm 2 range is presently a rout<strong>in</strong>e<br />

achievement. Over a period <str<strong>on</strong>g>of</str<strong>on</strong>g> ~ 25 years, a path <str<strong>on</strong>g>of</str<strong>on</strong>g><br />

research was cut through this field <str<strong>on</strong>g>of</str<strong>on</strong>g> n<strong>on</strong>l<strong>in</strong>ear<br />

phenomena that led to the development <str<strong>on</strong>g>of</str<strong>on</strong>g> a multikilovolt<br />

(~ 4.5 keV) x-ray amplifier <str<strong>on</strong>g>of</str<strong>on</strong>g> excepti<strong>on</strong>al peak brightness<br />

[2-5] that is excited by femtosec<strong>on</strong>d KrF* (248 nm)<br />

pulses and whose experimentally based power scal<strong>in</strong>g<br />

limit for a compact laboratory <strong>in</strong>strument falls <strong>in</strong> the<br />

multipetawatt realm [6]. The existence <str<strong>on</strong>g>of</str<strong>on</strong>g> advanced highenergy<br />

KrF* technology [7], that has been <strong>in</strong>dependently<br />

developed for fusi<strong>on</strong> applicati<strong>on</strong>s, could be readily<br />

adapted to extend the coherent x-ray power level <strong>in</strong>to the<br />

200 - 500 PW regime.<br />

* Sp<strong>on</strong>sored by Defense Advanced Research Projects<br />

Agency, Microsystems Technology Office (MTO),<br />

Program: Ultrabeam - The Scal<strong>in</strong>g <str<strong>on</strong>g>of</str<strong>on</strong>g> Coherent<br />

Amplificati<strong>on</strong> to the Gamma Ray Regi<strong>on</strong>, issued by<br />

DARPA/CMO under C<strong>on</strong>tract No. HR0011-10-C-0105.<br />

"The views and c<strong>on</strong>clusi<strong>on</strong>s c<strong>on</strong>ta<strong>in</strong>ed <strong>in</strong> this document<br />

are those <str<strong>on</strong>g>of</str<strong>on</strong>g> the authors and should not be <strong>in</strong>terpreted as<br />

represent<strong>in</strong>g the <str<strong>on</strong>g>of</str<strong>on</strong>g>ficial policies, either expressly or<br />

implied, <str<strong>on</strong>g>of</str<strong>on</strong>g> the Defense Advanced Research Projects<br />

Agency or the U.S. Government."<br />

rhodes@uic.edu<br />

# KFKI Research Institute for Particle and Nuclear<br />

<strong>Physics</strong>, EURATOM Associati<strong>on</strong>, P.O. Box 49,1525,<br />

Budapest, Hungary<br />

DISCUSSION<br />

The use <str<strong>on</strong>g>of</str<strong>on</strong>g> coherent x-rays for the atta<strong>in</strong>ment <str<strong>on</strong>g>of</str<strong>on</strong>g><br />

<strong>in</strong>tensities approach<strong>in</strong>g the Schw<strong>in</strong>ger Limit [8] <str<strong>on</strong>g>of</str<strong>on</strong>g> ~ 4.6 x<br />

10 29 W/cm 2 , a c<strong>on</strong>diti<strong>on</strong> <strong>in</strong>itially discussed by Sauter [9]<br />

and Heisenberg and Euler [10], is supported by very<br />

powerful scal<strong>in</strong>g relati<strong>on</strong>ships. A summary <str<strong>on</strong>g>of</str<strong>on</strong>g> the key<br />

physical parameters is presented <strong>in</strong> Fig. (1); the<br />

assessment gives the comparis<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> an <strong>in</strong>frared source<br />

(ħω ≅ 1eV) with a corresp<strong>on</strong>d<strong>in</strong>g source deliver<strong>in</strong>g (ħω<br />

≅ 4.5 keV) x-rays. The chief outcome is a figure <str<strong>on</strong>g>of</str<strong>on</strong>g> merit<br />

that measures the propensity to generate a high <strong>in</strong>tensity,<br />

and the x-ray illum<strong>in</strong>ator is favored over the <strong>in</strong>frared<br />

system by a factor that exceeds 10 21 , a result predicated<br />

<strong>on</strong> a relati<strong>on</strong>ship proporti<strong>on</strong>al to ω 6 . Furthermore, it is<br />

known that the overall physical situati<strong>on</strong> govern<strong>in</strong>g the<br />

atta<strong>in</strong>ment <str<strong>on</strong>g>of</str<strong>on</strong>g> the Schw<strong>in</strong>ger c<strong>on</strong>diti<strong>on</strong> is generally<br />

assisted by the existence <str<strong>on</strong>g>of</str<strong>on</strong>g> particularly propitious<br />

geometries <str<strong>on</strong>g>of</str<strong>on</strong>g> irradiati<strong>on</strong> [11,12].<br />

An additi<strong>on</strong>al advantage <str<strong>on</strong>g>of</str<strong>on</strong>g> an x-ray wavelength is the<br />

very large elevati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> the <strong>in</strong>tensity characteristic <str<strong>on</strong>g>of</str<strong>on</strong>g> the<br />

relativistic regime that flows from a fundamental scal<strong>in</strong>g<br />

proporti<strong>on</strong>al to ω 2 . Basically, the electric field E<br />

corresp<strong>on</strong>d<strong>in</strong>g to the relativistic regime is given by the<br />

c<strong>on</strong>diti<strong>on</strong><br />

eE<br />

mc ω<br />

= 1 (1)<br />

which, for Xe(L) radiati<strong>on</strong> with ħω ≅ 4.5 keV, yields an<br />

<strong>in</strong>tensity <str<strong>on</strong>g>of</str<strong>on</strong>g> ~ 10 25 W/cm 2 . This value is regarded both as<br />

(a) sufficiently high to produce observable c<strong>on</strong>sequences<br />

from the dynamics <str<strong>on</strong>g>of</str<strong>on</strong>g> the vacuum [13] and (b) free <str<strong>on</strong>g>of</str<strong>on</strong>g> the<br />

cascade limit for <strong>in</strong>tensities up to the Schw<strong>in</strong>ger/<br />

Heisenberg value, <strong>in</strong> c<strong>on</strong>trast to the <strong>in</strong>frared case [14].<br />

The ability to produce stable self-channeled propagati<strong>on</strong><br />

<str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>in</strong>tense pulses <str<strong>on</strong>g>of</str<strong>on</strong>g> radiati<strong>on</strong> <strong>in</strong> an underdense<br />

plasma is a well established phenomen<strong>on</strong> at quantum<br />

energies below ~5 eV [15-18]. An immediate c<strong>on</strong>sequence<br />

<str<strong>on</strong>g>of</str<strong>on</strong>g> the availability <str<strong>on</strong>g>of</str<strong>on</strong>g> a high power source <str<strong>on</strong>g>of</str<strong>on</strong>g> coherent<br />

x-rays is the possibility <str<strong>on</strong>g>of</str<strong>on</strong>g> extend<strong>in</strong>g the generati<strong>on</strong><br />

<str<strong>on</strong>g>of</str<strong>on</strong>g> these highly c<strong>on</strong>f<strong>in</strong>ed stable [16] modes <str<strong>on</strong>g>of</str<strong>on</strong>g> deeply<br />

penetrat<strong>in</strong>g propagati<strong>on</strong> to x-ray wavelengths <strong>in</strong> materials<br />

at solid density. If such channels can be pro-duced with<br />

multi-kilovolt x-rays <strong>in</strong> high-Z solids, the producti<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g><br />

power densities <strong>on</strong> the order <str<strong>on</strong>g>of</str<strong>on</strong>g> ~ 10 30 W/cm 3 are<br />

projected [19,20].

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