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

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Contents Overview and Tutorial talks A Recent Development in High Field Science (T. Tajima and G. Mourou) 1 The Heisenberg-Schwinger Effect: Nonperturbative Vacuum Pair Production (G. Dunne) 7 Nonlinear QED QED in Ultra-Intense Laser Fields (T. Heinzl) 14 Strong-Field Effects in Beam-Beam Interaction in Linear Colliders (K. Yokoya) 19 Second Order QED Processes and Their Radiative Corrections (A. Hartin) 23 Heavy-ion collisions and Quark-Gluon Plasma Strong Field Dynamics in Heavy Ion Collisions (K. Itakura) 26 Yoctosecond photon pulse generation in heavy ion collisions (A. Ipp) 32 Fields, Instantons, and Currents (K. Fukushima) 36 Critical Behavior <strong>of</strong> Charmonium: QCD Second Order Stark Effect (K. Morita and S.H. Lee) 40 Unruh radia on On the Unruh Effect (R. Schützhold) 44 Can We Detect ″Unruh Radiation″ in the High Intensity Lasers? (S. Zhang, et al.) 46 Quantum Fields in Accelerated Frames (F. Lenz) 50 Axion-like par cle searches Shining Light through Walls: en Route towards a New Particle Physics Frontier (A. Lindner) 54 Probing Extremely Light Fields via Resonance Scattering by Focusing Intense Laser (K. Homma) 59 Schwinger mechanism in QGP and condensed ma er Dynamical View <strong>of</strong> Pair Creation via the Schwinger Mechanism (N. Tanji) 63 Exact Solutions <strong>of</strong> Pair Productions in Strong Electric Field with Finite Width (A. Iwazaki) 67 Strong Field Physics in Condensed Matter (T. Oka) 70 Non-Linear Charge Transport in Plasma under Strong Field (S. Nakamura) 74 Recent developments in Schwinger mechanism Brilliant Hard γ-Production and e + e – -Creation in Vacuum with Ultra-High Laser Fields: Testing Theoretical Predictions at ELI-NP (D. Habs, et al.) 78 Numerical Simulation <strong>of</strong> QED Cascades in Intense Laser Fields (N. Elkina and H. Ruhl) 83 Schwinger Limit Attainability with Extreme Light (S.V. Bulanov, et al.) 88 Pair Creation in QED-Strong Pulsed Laser Fields (N. Naumova, et al.) 93 Laser Acceleration up to Black Holes and B-meson Decay (H. Hora, et al.) 97 vii
Page 1 and 2: Proceedings <stron
Page 3: Conference poster
Page 7: Preface The international conferenc
Page 12 and 13: energy and Ip the ionization potent
Page 14 and 15: estoring frequency (or the shorter
Page 17 and 18: The Heisenberg-Schwinger effect: No
Page 19 and 20: take into account the fact that the
Page 21 and 22: cult to extract the exponentially s
Page 23 and 24: [35] M. B. Voloshin and K. G. Seliv
Page 25 and 26: quency measured in the lab. By Maxw
Page 27 and 28: positrons, each of
Page 29 and 30: Abstract Strong-Field Effects in Be
Page 31 and 32: At high field a is nolonger a const
Page 33 and 34: Abstract Second order QED processes
Page 35 and 36: p f p i Figure 4: The BIP vertex co
Page 37 and 38: Figure 1: (Left) Time evolution <st
Page 39 and 40: momenta of left an
Page 41 and 42: many interesting phenomena were fou
Page 43 and 44: ted photons could provide a window
Page 45 and 46: various sources [28]. These include
Page 47 and 48: where A(x) denotes a vector potenti
Page 49 and 50: The above equation gives a microsco
Page 51 and 52: confinement-deconfinement transitio
Page 53 and 54: (α s /π)∆E 2 [GeV 4 ] 0.003 0.0
Page 55 and 56: In the stationary case, it is usefu
Page 57 and 58: tained the relaxation time
Page 59 and 60:
Let’s compare this relaxation tim
Page 61 and 62:
S = 1 2 dτ dξ d d−1 x⊥ (∂
Page 64 and 65:
Abstract Shining Light through Wall
Page 66 and 67:
Figure 3: Schematic view of
Page 68 and 69:
Figure 6: Estimates of</str
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theory provides a natural explanati
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states rather than from the vacuum
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Real-time description Because the s
Page 76 and 77:
Figure 6: A schematic of</s
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E(t = 0) is the electric field swit
Page 80 and 81:
Abstract Strong field physics in co
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IV-characteristics conductance
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What we shall do in the present wor
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conductor. The current is given by
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This implies that E 2 − c 2 B 2
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1 , MεV § dN/d¦ 10 5 10 4 10 3 1
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Abstract Numerical simulation <stro
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Figure 1: Cascading in a laser focu
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Figure 2: Clustering of</st
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10 k 0z 0 -10 0 k 0r a) 1 10 0 -10
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y the well known expression [13] ha
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PAIR CREATION IN QED-STRONG PULSED
Page 105 and 106:
Figure 2: Distribution functions <s
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LASER ACCELERATION UP TO BLACK HOLE
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(1) charged B-mesons Irel = 1.2×10
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Present Status of
Page 113 and 114:
neutral pair plasma production as s
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small for the electric field weaker
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REACHING THE SCHWINGER LIMIT WITH X
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Fig. (3): Channel production in sol
Page 121 and 122:
Abstract Non-linear QED effects by
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Figure 4: Refractive indices <stron
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with the canonical momentum Πµ
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Basic Concepts NEUTRON STARS When t
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General behavior MAGNETARS About 15
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QCD ORIGIN OF STRONG MAGNETIC FIELD
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states in quark matter have been st
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Recent progress and prospects on la
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the wakefields. In the case <strong
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pulse with I = 10 21 Wcm -2 at = 0
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Plasma Flying mirrors Driver pulse
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REFERENCES [1] D. Strickland and G.
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Figure 6: To reduce the laser waist
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Amplified Pulse Energy (mJ) 100 Hor
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demonstration encourages four-beams
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Radio Pulsar Number 250 200 150 100
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Abstract THE NIELSEN-OLESEN INSTABI
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GLASMA INSTABILITIES IN A BOX Recen
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field because of t
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FAST VACUUM DECAY INTO PARTICLE PAI
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E/E 0 N/N max 1 0.5 0 -0.5 -1 -6 -4
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where p = pc − mca is the mechani
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PARTICLE BASED INTEGRATED CODE EPIC
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P(k x ) (a) 44.3psec (b) 45.3pec (c
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the position of th
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Table 2: crossing angle and the ran
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e replaced by its average K → K0
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Abstract Unruh radiation and Interf
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The integrand can be written as ∫
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15:15 break [15] [Unruh radiation :
Page 187 and 188:
10:35 break (20) [Magnetars : chair
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