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Bright Multi-keV Harmonic Generation from Relativistically Oscillating Plasma Surfaces

B. DromeyDepartment of Physics and Astronomy, Queens University, Belfast, UKS. KarDepartment of Physics and Astronomy, Queens University, Belfast, BT7 1NN, United KingdomC. BelleiBlackett Laboratory, Imperial College, London, SW7 2BZ, United KingdomD. C. CarrollSUPA, Department of Physics, University of Strathclyde, Glasgow, G4 0NG, United KingdomR. J. ClarkeCentral Laser Facility, CCLRC Rutherford Appleton Laboratory, Chilton, Didcot, OX11 0QX, United KingdomJ.S. GreenBlackett Laboratory, Imperial College, London, SW7 2BZ, United KingdomS. KneipBlackett Laboratory, Imperial College, London, SW7 2BZ, United KingdomK. MarkeyDepartment of Physics and Astronomy, Queens University, Belfast, BT7 1NN, United KingdomS. R. NagelBlackett Laboratory, Imperial College, London, SW7 2BZ, United KingdomP. T. SimpsonDepartment of Physics and Astronomy, Queens University, Belfast, BT7 1NN, United KingdomL. WillingaleBlackett Laboratory, Imperial College, London, SW7 2BZ, United KingdomP. McKennaSUPA, Department of Physics, University of Strathclyde, Glasgow, G4 0NG, United KingdomD. NeelyCentral Laser Facility, CCLRC Rutherford Appleton Laboratory, Chilton, Didcot, OX11 0QX, United KingdomZ. NajmudinBlackett Laboratory, Imperial College, London, SW7 2BZ, United KingdomK. KrushelnickBlackett Laboratory, Imperial College, London, SW7 2BZ, United KingdomP. A. NorreysCentral Laser Facility, CCLRC Rutherford Appleton Laboratory, Chilton, Didcot, OX11 0QX, United KingdomM. ZepfDepartment of Physics and Astronomy, Queens University, Belfast, BT7 1NN, United Kingdom
2007en
ABI

Аннотация

The first evidence of x-ray harmonic radiation extending to 3.3 \AA{}, 3.8 keV (order $n>3200$) from petawatt class laser-solid interactions is presented, exhibiting relativistic limit efficiency scaling ($\ensuremath{\eta}\ensuremath{\sim}{n}^{\ensuremath{-}2.5}--{n}^{\ensuremath{-}3}$) at multi-keV energies. This scaling holds up to a maximum order, ${n}_{\mathrm{RO}}\ensuremath{\sim}{8}^{1/2}{\ensuremath{\gamma}}^{3}$, where $\ensuremath{\gamma}$ is the relativistic Lorentz factor, above which the first evidence of an intensity dependent efficiency rollover is observed. The coherent nature of the generated harmonics is demonstrated by the highly directional beamed emission, which for photon energy $h\ensuremath{\nu}>1\text{ }\text{ }\mathrm{keV}$ is found to be into a cone angle $\ensuremath{\sim}4\ifmmode^\circ\else\textdegree\fi{}$, significantly less than that of the incident laser cone (20\ifmmode^\circ\else\textdegree\fi{}).

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