rasmus ischebeck synchrotron radiation...wir schaffen wissen – heute fÜr morgen synchrotron...

13
WIR SCHAFFEN WISSEN – HEUTE FÜR MORGEN Synchrotron Radiation Joint Universities Accelerator School Rasmus Ischebeck

Upload: others

Post on 15-Mar-2020

7 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: Rasmus Ischebeck Synchrotron Radiation...WIR SCHAFFEN WISSEN – HEUTE FÜR MORGEN Synchrotron Radiation Joint Universities Accelerator School Rasmus Ischebeck

WIRSCHAFFENWISSEN–HEUTEFÜRMORGEN

Synchrotron Radiation JointUniversitiesAcceleratorSchool

RasmusIschebeck

Page 2: Rasmus Ischebeck Synchrotron Radiation...WIR SCHAFFEN WISSEN – HEUTE FÜR MORGEN Synchrotron Radiation Joint Universities Accelerator School Rasmus Ischebeck

Nick Veasey

How Did You Like the Course?

Page 3: Rasmus Ischebeck Synchrotron Radiation...WIR SCHAFFEN WISSEN – HEUTE FÜR MORGEN Synchrotron Radiation Joint Universities Accelerator School Rasmus Ischebeck

Accelerator Research for X-Ray Science

�3T. Plettner and R. L. Byer, Phys. Rev. ST Accel. Beams 11, 030704

Page 4: Rasmus Ischebeck Synchrotron Radiation...WIR SCHAFFEN WISSEN – HEUTE FÜR MORGEN Synchrotron Radiation Joint Universities Accelerator School Rasmus Ischebeck

Accelerator Research for X-Ray Science

�4Pizzi et al., CLEO 2018

FW4H.7.pdf CLEO 2018 © OSA 2018

setup overcomes the inherent limitations that occur in a single layer scenario having an exponential field decay in the transverse direction, and allows to scale up the output radiation intensity by increasing the thickness (i.e. NG) of the stack (Fig. 1.c). For a very large NG (e.g. NG > 50 for s = 25 nm, i.e. a stack thicker than 1.25 µm) the driving field cannot penetrate uniformly through the whole structure, preventing a further increase of the output intensity.

Fig. 1. Generation of X-rays from a 5 MeV electron beam interacting with the metamaterial’s GPs. a) 2D schematic of the setup for NG = 10 layers in the stack. The driving laser is coupled with GPs by mean of a grating structure; the free electrons of the beam (dashed yellow lines) are wiggled by the plasmonic field (glowing red and blue bars) when passing through the structure, emitting X-ray radiation. b) The emission is directional and highly monochromatic. Emitted radiation in units of photons per second, per steradian, per 1% bandwidth, in the case of dielectric spacings of thickness s = 25 nm, NG = 50 layers, average current IC = 40 mA, transversal spread σ = 1 µm and driving laser wavelength λ0 = 7.0864 µm. c) Maximum intensity versus the number NG of graphene layers in the stack for different beam cross-sections σ and currents IC, while keeping the beam current density constant. Increasing the overall thickness of the metamaterial leads to larger interaction areas and more intense emissions, especially for large beams (e.g. Imax(NG = 50) = 65Imax(NG = 1) for σ = 1 µm). d) Transverse component of the electric field for a n = 2 plasmonic resonance for λ0 = 4.9207 µm, s = 15 nm. The correspondent emitted radiation is shown (with logarithmic colorbar) in e) for IC = 40 mA and σ = 1 µm. We notice that the n-th (that is 2-nd) emission harmonic is the brightest one.

4. Tunability of the light source

We show how to obtain higher energy emissions exploiting the higher order plasmonic resonances. The multiple spatial harmonics of the GP field result in higher order harmonics in the emission spectrum [2]. By tuning the driving laser frequency, it is possible to couple a n-th order GP with longitudinal wavevector q = 2nπ/p (e.g. n = 2 in Fig. 1.d). The brightest harmonic of the correspondent output emission will then be the n-th one (n = 2 in Fig. 1.e). With higher order GPs, it is thus possible to effectively access high energy output harmonics, overcoming the need of reducing the grating periodicity to increase the radiation energy.

4. References [1] Plettner, T., and R. L. Byer. "Proposed dielectric-based microstructure laser-driven undulator." Phys. Rev. Accel. Beams 11.3 (2008): 030704. [2] Rosolen, G., et al. "Efficient hard X-ray source enabled by metallic nano-gratings." Opt. InfoBase Conf. Papers, Part F42-CLEO_QELS, 2017 [3] Karagodsky, V., et al. "Enhancing x-ray generation by electron-beam–laser interaction in an optical Bragg structure." Phys. Rev. Lett. 104.2 (2010): 024801. [4] Wong, L. J., et al. "Towards graphene plasmon-based free-electron infrared to X-ray sources." Nature Photonics 10.1 (2016): 46. [5] Jablan, M., et al. "Plasmonics in graphene at infrared frequencies." Physical review B 80.24 (2009): 245435. [6] Seltzer, S. M., & Martin J. B. Int. J. Appl. Radiat. Isot. 33, 1219 (1982); Int. J. Appl. Radiat. Isot. 35, 665 (1984).

FW4H.7.pdf CLEO 2018 © OSA 2018

setup overcomes the inherent limitations that occur in a single layer scenario having an exponential field decay in the transverse direction, and allows to scale up the output radiation intensity by increasing the thickness (i.e. NG) of the stack (Fig. 1.c). For a very large NG (e.g. NG > 50 for s = 25 nm, i.e. a stack thicker than 1.25 µm) the driving field cannot penetrate uniformly through the whole structure, preventing a further increase of the output intensity.

Fig. 1. Generation of X-rays from a 5 MeV electron beam interacting with the metamaterial’s GPs. a) 2D schematic of the setup for NG = 10 layers in the stack. The driving laser is coupled with GPs by mean of a grating structure; the free electrons of the beam (dashed yellow lines) are wiggled by the plasmonic field (glowing red and blue bars) when passing through the structure, emitting X-ray radiation. b) The emission is directional and highly monochromatic. Emitted radiation in units of photons per second, per steradian, per 1% bandwidth, in the case of dielectric spacings of thickness s = 25 nm, NG = 50 layers, average current IC = 40 mA, transversal spread σ = 1 µm and driving laser wavelength λ0 = 7.0864 µm. c) Maximum intensity versus the number NG of graphene layers in the stack for different beam cross-sections σ and currents IC, while keeping the beam current density constant. Increasing the overall thickness of the metamaterial leads to larger interaction areas and more intense emissions, especially for large beams (e.g. Imax(NG = 50) = 65Imax(NG = 1) for σ = 1 µm). d) Transverse component of the electric field for a n = 2 plasmonic resonance for λ0 = 4.9207 µm, s = 15 nm. The correspondent emitted radiation is shown (with logarithmic colorbar) in e) for IC = 40 mA and σ = 1 µm. We notice that the n-th (that is 2-nd) emission harmonic is the brightest one.

4. Tunability of the light source

We show how to obtain higher energy emissions exploiting the higher order plasmonic resonances. The multiple spatial harmonics of the GP field result in higher order harmonics in the emission spectrum [2]. By tuning the driving laser frequency, it is possible to couple a n-th order GP with longitudinal wavevector q = 2nπ/p (e.g. n = 2 in Fig. 1.d). The brightest harmonic of the correspondent output emission will then be the n-th one (n = 2 in Fig. 1.e). With higher order GPs, it is thus possible to effectively access high energy output harmonics, overcoming the need of reducing the grating periodicity to increase the radiation energy.

4. References [1] Plettner, T., and R. L. Byer. "Proposed dielectric-based microstructure laser-driven undulator." Phys. Rev. Accel. Beams 11.3 (2008): 030704. [2] Rosolen, G., et al. "Efficient hard X-ray source enabled by metallic nano-gratings." Opt. InfoBase Conf. Papers, Part F42-CLEO_QELS, 2017 [3] Karagodsky, V., et al. "Enhancing x-ray generation by electron-beam–laser interaction in an optical Bragg structure." Phys. Rev. Lett. 104.2 (2010): 024801. [4] Wong, L. J., et al. "Towards graphene plasmon-based free-electron infrared to X-ray sources." Nature Photonics 10.1 (2016): 46. [5] Jablan, M., et al. "Plasmonics in graphene at infrared frequencies." Physical review B 80.24 (2009): 245435. [6] Seltzer, S. M., & Martin J. B. Int. J. Appl. Radiat. Isot. 33, 1219 (1982); Int. J. Appl. Radiat. Isot. 35, 665 (1984).

Page 5: Rasmus Ischebeck Synchrotron Radiation...WIR SCHAFFEN WISSEN – HEUTE FÜR MORGEN Synchrotron Radiation Joint Universities Accelerator School Rasmus Ischebeck

Accelerator Research for X-Ray Science

�5Sven Reiche

LaserIncoupling1

LaserIncoupling2

Modulator1Modulator2

Radiator

1stR56fromArc

2ndR56fromChicane

Unusedspace

295 10peakB ≈ ⋅

Page 6: Rasmus Ischebeck Synchrotron Radiation...WIR SCHAFFEN WISSEN – HEUTE FÜR MORGEN Synchrotron Radiation Joint Universities Accelerator School Rasmus Ischebeck

Accelerator Research for X-Ray Science

�6Benedikt Hermann

Page 7: Rasmus Ischebeck Synchrotron Radiation...WIR SCHAFFEN WISSEN – HEUTE FÜR MORGEN Synchrotron Radiation Joint Universities Accelerator School Rasmus Ischebeck

Booksonsynchrotrons• Acceleratorside:

Resources for You

�7

Helmut Wiedemann Synchrotron Radiation [3-642-07777-3; 3-662-05312-8]

• Userside:

Philip Willmott An Introduction to Synchrotron Radiation [1119280397]

Page 8: Rasmus Ischebeck Synchrotron Radiation...WIR SCHAFFEN WISSEN – HEUTE FÜR MORGEN Synchrotron Radiation Joint Universities Accelerator School Rasmus Ischebeck

• AbookonFELs

Resources for You

�8

Schmüser, Dohlus & Rossbach Ultraviolet and Soft X-Ray Free-Electron Lasers [978-3-540-79571-1]

• DerivationofsynchrotronradiationfromMaxwell’sEquations

John David Jackson Classical Electrodynamics [978-0471309321]

“Undergraduate E&M is about solving the simple problems exactly. Jackson E&M is about learning to approximate

reliably. The entire book, with few exceptions, is a mathematical

discussion on finding way to solve only 4 equations for different boundary

conditions.” (Davon Ferrara)

Page 9: Rasmus Ischebeck Synchrotron Radiation...WIR SCHAFFEN WISSEN – HEUTE FÜR MORGEN Synchrotron Radiation Joint Universities Accelerator School Rasmus Ischebeck

On-Line Resources

�9

Page 10: Rasmus Ischebeck Synchrotron Radiation...WIR SCHAFFEN WISSEN – HEUTE FÜR MORGEN Synchrotron Radiation Joint Universities Accelerator School Rasmus Ischebeck

On-Line Resources

�10

Page 11: Rasmus Ischebeck Synchrotron Radiation...WIR SCHAFFEN WISSEN – HEUTE FÜR MORGEN Synchrotron Radiation Joint Universities Accelerator School Rasmus Ischebeck

• On-line:http://xdb.lbl.gov/xdb-new.pdf

The X-Ray Data Booklet

�11

Page 12: Rasmus Ischebeck Synchrotron Radiation...WIR SCHAFFEN WISSEN – HEUTE FÜR MORGEN Synchrotron Radiation Joint Universities Accelerator School Rasmus Ischebeck

• Theexamwillbeanopen-bookexam.• Youarepermittedtouseallthecoursematerials,aswellasyournotes.• Pleasebringacalculator,installacalculatorapponyourcomputer/tablet,orusePython/Matlab/Mathematica.(Makesureyourapplicationrunswithoutanonlineconnection.)

• Pleasedownloadalllecturematerialtoyourcomputer/tablet.• Inaddition,pleasedownloadfromtheIndicosite:• TheX-RayDataBooklet• Thesheetwithnaturalconstants

• Theexamwilldiffersomewhatfromlastyear’sexam: therewillbequestionsontheusesofsynchrotronradiation.Theproblemswillbesimilartotheonesinthisyear’sexercises.

• Mobilephonesarenotpermitted.Onlyyourlaptop/tabletisallowed.• On-lineconnectionsduringtheexamsarenotpermitted.• TurnyourWi-Fioff,switchyourtablettoairplanemode,anddeposityourmobilephonewiththeinstructors.

Resources for the Exam

�12

Page 13: Rasmus Ischebeck Synchrotron Radiation...WIR SCHAFFEN WISSEN – HEUTE FÜR MORGEN Synchrotron Radiation Joint Universities Accelerator School Rasmus Ischebeck

• e-mail:[email protected]• webpage:https://ischebeck.net

• see(someof)youatPSI!

Any More Questions…

�13