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

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QGP is studied by us<strong>in</strong>g the particle energy and angle<br />

distributi<strong>on</strong> determ<strong>in</strong>ed just after the phase transiti<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g><br />

liquid phase <str<strong>on</strong>g>of</str<strong>on</strong>g> QCD to free particle state which is called<br />

freeze-out [40]. In case <str<strong>on</strong>g>of</str<strong>on</strong>g> laser driven vacuum breakdown,<br />

the lept<strong>on</strong> pair plasma is generated and its spatial<br />

scale is about 10 -4 cm (=1µm) and life time is about 10 -15 s<br />

(1fs) as schematically shown <strong>in</strong> Fig. 6. S<strong>in</strong>ce the plasma<br />

size and lifetime are milli<strong>on</strong> times bigger and l<strong>on</strong>ger than<br />

t h we can e develop the Q diagnostics G to P directly ,<br />

[1] V Yan<str<strong>on</strong>g>of</str<strong>on</strong>g>sky . et al., Opt. Express16, 2109n (2008)<br />

[2] G.A.Mourou, Phys. Today 51,No.1,22(1998).<br />

[3] http://www.extreme-light-<strong>in</strong>frastructure.eu/<br />

[4] Czech: http://www.eli-beams.eu/<br />

[5] Hungary:<br />

http://www.eli-beams.eu/news-from-hungary/<br />

[6] Romania: http://eli.ifa-mg.ro/<br />

[7] ELI: http://www.eli-beams.eu/evropsky-projekt/<br />

eli-v-kostce/<br />

[8] http://www.clf.rl.ac.uk/<br />

[9] http://apri.gist.ac.kr/eng/<strong>in</strong>dex.php<br />

[10] http://wwwapr.kansai.jaea.go.jp/outl<strong>in</strong>e.html<br />

[ 1 1 ] http://www.ile.osaka-u.ac.jp/<br />

[12] https://jlf.llnl.gov/html/facilities/titan/titan.html<br />

[13] http://www.lle.rochester.edu/<br />

[14] https://e-reports-ext.llnl.gov/pdf/349575.pdf<br />

[15] T.E. Cowan et al., Phys. Rev. Lett. 84, 903 (2000).<br />

[16] T.E. Cowan et al., Laser Part. Beams 17, 773<br />

(1999).<br />

[17] K. Nakashima and H. Takabe, Phys. Plasmas 9, 1505<br />

(2002).<br />

measure the properties <str<strong>on</strong>g>of</str<strong>on</strong>g> the pair plasma. For example,<br />

we can measure the turbulent spectrum <str<strong>on</strong>g>of</str<strong>on</strong>g> the highly<br />

n<strong>on</strong>l<strong>in</strong>ear stage <str<strong>on</strong>g>of</str<strong>on</strong>g> the pair plasma with a bright x-ray<br />

source <strong>in</strong> the range <str<strong>on</strong>g>of</str<strong>on</strong>g> atto-sec<strong>on</strong>d pulse technology to be<br />

developed <strong>in</strong> Hungary [5]. Deep understand<strong>in</strong>g <str<strong>on</strong>g>of</str<strong>on</strong>g> such<br />

plasma and verificati<strong>on</strong> and validati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> the computati<strong>on</strong>al<br />

model<strong>in</strong>g <str<strong>on</strong>g>of</str<strong>on</strong>g> the vacuum breakdown, avalanche<br />

effect, phot<strong>on</strong>-lept<strong>on</strong> <strong>in</strong>teracti<strong>on</strong>, and a variety <str<strong>on</strong>g>of</str<strong>on</strong>g> physics<br />

<str<strong>on</strong>g>of</str<strong>on</strong>g> highly relativistic pair plasma are sure to be very much<br />

beneficial for understand<strong>in</strong>g the QGP physics. We can say<br />

the vacuum breakdown physics is a model experiment <str<strong>on</strong>g>of</str<strong>on</strong>g><br />

QGP <strong>in</strong> relatively small scale laser facility.<br />

CONCLUSION<br />

With the progress <str<strong>on</strong>g>of</str<strong>on</strong>g> <strong>in</strong>tense laser technology, the<br />

physics to be solved <strong>in</strong> laser-matter <strong>in</strong>teracti<strong>on</strong> has<br />

already become relativistic regime for electr<strong>on</strong>s. In<br />

several years, we will come to the regime where laservacuum<br />

<strong>in</strong>teracti<strong>on</strong> becomes important and the 80-years<br />

stand<strong>in</strong>g theory <str<strong>on</strong>g>of</str<strong>on</strong>g> the vacuum breakdown will be really<br />

experimentally studied. We c<strong>on</strong>cluded that the electr<strong>on</strong><br />

pair creati<strong>on</strong> can be expected from 10 24 W/cm 2 with use<br />

<str<strong>on</strong>g>of</str<strong>on</strong>g> seed electr<strong>on</strong>s and thanks to the resultant avalanche<br />

effect. When the laser <strong>in</strong>tensity exceeds more than 10 26<br />

W/cm 2 [18] T. Cowan et al, 2002: H. Takabe, <strong>in</strong> “Hadr<strong>on</strong> and<br />

Nuclear <strong>Physics</strong> 09”, Edt. A. Hosaka et al., p.<br />

388-403 (World Scientifics, 2010)<br />

[19] Y. Sentoku, private communicati<strong>on</strong>.<br />

[20] For example; L. L. Stephan, Computer <strong>Physics</strong><br />

Communicati<strong>on</strong>s 72, Issues 2-3, November 1992,<br />

Pages 144-148<br />

[21]<br />

[22]<br />

[23]<br />

[24]<br />

A. Mizuta, S. Yamada, and H. Takabe,<br />

Astrophysical J. 606 804 (2004).<br />

H. Chen et al., Phys. Plasmas 16, 122702 (2009).<br />

References there <strong>in</strong>.<br />

H. Chen, H. Takabe et al, NIF proposal (2010) ,<br />

not published, approved by NIF committee.<br />

P. Dirac, The Pr<strong>in</strong>ciple <str<strong>on</strong>g>of</str<strong>on</strong>g> Quantum Mechanics.<br />

[25]<br />

(Oxford Univ. Press, 1930).<br />

A. R. Bell and J. G. Kirk, Phys. Rev. Lett., 101,<br />

200403 (2008)<br />

[26] Landau & Lifshitz, “Theory <str<strong>on</strong>g>of</str<strong>on</strong>g> Classical Field”,<br />

Chap. 9, S.75.<br />

[27] J. G. Kirk, A. R. Bell, and I. Arka, Plasam Phys.<br />

, we can really break down the pure vacuum with<br />

[28]<br />

[29]<br />

[30]<br />

[31]<br />

[32]<br />

C<strong>on</strong>trol Fusi<strong>on</strong> 51 085008 (2009).<br />

H. Takabe, “Relativistic Plasma <strong>Physics</strong>”, J.<br />

Plasma Fusi<strong>on</strong> Res. 78 427-438 (2002), <strong>in</strong><br />

Japanese<br />

N. Elk<strong>in</strong>a and H. Ruhl, <strong>in</strong> this proceed<strong>in</strong>g<br />

N. B. Narozhny et al., JETP Letters<br />

R. Ruff<strong>in</strong>i et al., <strong>Physics</strong> Reports 487, 1-140<br />

(2010)<br />

A. M. Fedotov, Laser <strong>Physics</strong> 19, 214 (2009)<br />

help <str<strong>on</strong>g>of</str<strong>on</strong>g> pairs appear<strong>in</strong>g by quantum tunnel<strong>in</strong>g effect. W e [33] S. S. Bulanov et al., Phys. Rev. Lett. 104, 220404<br />

also po<strong>in</strong>ted out that this lept<strong>on</strong> fireball physics will be (2010)<br />

beneficial to model<strong>in</strong>g quark-glu<strong>on</strong> plasmas.<br />

[34] G. Miyaji, PhD Thesis, January, 2004<br />

[35] For example; F. D. Seward and P. A. Charles,<br />

REFERENCES<br />

“Explor<strong>in</strong>g the X-ray Universe” 2 nd editi<strong>on</strong><br />

(Cambridge, 2010)<br />

[36] T. N. Kato, Astrophysical J. 668 974-979, (2007);<br />

P. Chang, A. Spitkovsky, and J. Ar<strong>on</strong>s 674 378,<br />

(2008).<br />

[37] M. Asakawa et al., Phys. Rev. Lett. 96, 252301<br />

(2006)<br />

[38] RHIC: http://www.bnl.gov/rhic/<br />

[39] LHC: http://lhc.web.cern.ch/lhc/<br />

[40] S. A. Bass and A. Dumitru, Phys. Rev. C 61,<br />

064909 (2000)

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