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