C R E S β A N E W M E T H O D T O WA R D S β¨ M E A S U R I N G T H E π - M A S S S E B A S T I A N B Γ S E R 7 T H J U N E 2 0 1 6 | G D R N E U T R I N O 2 0 1 6 | G R E N O B L E
M E A S U R I N G π - M A S S Project8 β 2
T R I T I U M B E TA - D E C AY 3 H β 3 He + + e - + π Μ e β’ Sum of masses and kinetic energy must add β¨ up to mass of initial nucleus Project8 β 3
T R I T I U M B E TA - S P E C T R U M dN q ( E β E 0 ) 2 β m 2 dE βΌ F ( Z, E ) p e ( E + m e ) Ξ² ) Project8 β 4
T R I T I U M B E TA - S P E C T R U M β β ( E β E 0 ) 2 β 1 dN 2 m 2 dE βΌ F ( Z, E ) p e ( E + m e ) Ξ² ) Endpoint of spectrum changes with π -mass β¨ β direct measurement of mass β¨ (independent of βnatureβ of mass) Project8 β 5
T R I T I U M B E TA - S P E C T R U M β’ Fraction of e β in ROI β’ 10 eV: 2 Γ 10 β 10 1 eV: 2 Γ 10 β 13 β’ β’ Requirements β’ high count rate β’ high resolution Endpoint of spectrum changes with π -mass β¨ β direct measurement of mass β¨ (independent of nature of mass) Project8 β 6
S TAT E O F T H E A R T β K AT R I N Key component: MAC-E filter β’ align e - momentum p ? β p k Project8 β 7
K AT R I N Karlsruhe Trititum Neutrino Experiment Sensitivity goal β’ m Ξ² < 200meV Limited by β’ size of spectrometer β’ systematic effects β need a new and β¨ Inverted hierarchy complementary approach Normal hierarchy Project8 β 8
C Y C L O T R O N R A D I AT I O N Cyclotron radiation eB β₯ f c = 1 m e 2 Ο relativistic correction f Ξ³ = f c eB β₯ Ξ³ = 1 m e + E kin 2 Ο β Never measure anything but frequency β - A. L. Schawlow Project8 β 9
R E S O L U T I O N Energy resolution β¨ f β Ξ E/E ~ Ξ f β’ Ξ E/E ~ 1eV / 511 keV = 2ppm β¨ β easy! Frequency resolution β¨ Ξ f ~ 1/ Ξ t β’ Ξ t = 20 ΞΌ s ~ 1400m @ 18keV β¨ β hard! A. L. Schawlow Project8 β 10
Idea β’ fill volume with 3 H gas β’ add magnetic field β’ decay electrons spiral around field lines β’ add antennas to detect cyclotron radiation B. Monreal and J. Formaggio, Phys. Rev D80:051301 Project8 β 11
F R E Q U E N C Y S C A L E magnetic field of 1T β cyclotron frequency in K-Band 83m Kr provides electrons close to tritium endpoint Project8 β 12
R A D I AT E D P O W E R Larmor formula q 4 B 2 1 2 ( Ξ³ 2 β 1) sin 2 ΞΈ P ( Ξ³ , ΞΈ ) = 4 ΟΞ΅ 0 3 m 2 e p e Emitted power ΞΈ β pitch angle β’ 1.1 fW for 18 keV e - at 90ΒΊ B-field β’ 1.7 fW for 30.4 keV e - at 90ΒΊ β Low-noise cryogenic RF-system needed! Project8 β 13
P R O J E C T 8 P R O T O T Y P E Signal Project8 β 14
WAV E G U I D E C E L L Project8 β 15
S I G N A L A M P L I F C AT I O N A N D N O I S E fine Swedish β¨ Noise temperature: T eff = 150K amplifier β’ Primary background β¨ β thermal noise from waveguide and amplifiers Project8 β 16
R E C E I V E R S TA G E β’ Double-stage down-mixing β’ Digitizer: 8-bit, 500Ms/s, 125MHz bandwidth β¨ β untriggered Project8 β 17
M A G N E T I C B O T T L E 1 + cot 2 ΞΈ β β f Ξ³ = f c eB Ξ³ = 1 Harmonic e - trap β 2 Ο m e + E kin 2 5mT Different β¨ pitch angles Magentic β¨ bottle coil Effect of trap on measured frequency easily calculable! Project8 β 18
E X P E C T E D S I G N A L Spectrogram β’ time slices β¨ β consecutive β¨ power spectrum Signal β’ narrow-band β¨ β horizontal line β’ energy loss by radiation β¨ β line is tilted Project8 β 19
A C T U A L S P E C T R O G R A M Data Taking on 06/06/2014 immediately shows trapped electrons PhysRevLett.114.162501 (2015) First detection of single-electron cyclotron radiation! Project8 β 20
S P E C T R O G R A M I N F O R M AT I O N Project8 β 21
E N E R G Y S P E C T R U M Initial frequency determines initial energy Project8 β 22
F I R S T E N E R G Y S P E C T R U M Both 83m Kr lines β¨ β clearly seen Resolution β’ FWHM: 140 eV Phys. Rev. Lett. 114, 162501 (2015) Project8 β 23
I M P R O V E D T R A P Shallower Harmonic trap β’ better field uniformity β’ smaller acceptance β lower rate & β¨ better resolution Bathtub trap β’ two coils at end of cell β’ better uniformity β’ larger trap size β larger rate & β¨ better resolution Project8 β 24
C R E S β C Y C L O T R O N R A D I AT I O N β¨ E M I S S O N S P E C T R O S C O P Y Hardware β¨ improvements β’ better field β¨ uniformity β’ reduced β¨ noise level β’ better β¨ temperature β¨ stability Project8 β 25
P O T E N T I A L π - M A S S R E A C H Ο (B) ~ 0.1ppm, 1 year of data per cm 3 per cm 3 per cm 3 per cm 3 Sensitivity limited by gas density! Project8 β 26
P O T E N T I A L π - M A S S R E A C H current cell β¨ volume current limit per cm 3 per cm 3 inverted hierarchy bound per cm 3 Inverted hierarchy limit in reach with atomic tritium! Project8 β 27
P R O J E C T 8 β¨ C O L L A B O R AT I O N T. ThΓΌmmler Karlsruhe Institute of Technology S. BΓΆser, C. Claessens * Johannes Gutenberg-UniversitΓ€t, Mainz K. Kazkaz Lawrence Livermore National Laboratory J. Formaggio, N. Oblath, E. Zayas * Massachusetts Institute of Technology * indicates graduate student M. Guigue, A. M. Jones, J. Tedeschi, B. VanDevender Pacific Northwest National Lab S. Doelman, J. Weintroub, A. Young Smithsonian Astrophysical Observatory K. Heeger, L. Saldana*, P. Slocum L. de Viveros, B. LaRoque * , B. Monreal Yale University University of California, Santa Barbara P. Doe, A. Ashtari Esfahani * , M. Fertl, E. Machado * , R.G.H. Robertson, L. Rosenberg, G. Rybka University of Washington, Center for Experimental Nuclear Physics and Astrophysics Project8 β 28
A P H A S E D A P P R O A C H P h a s e Ti m e l i n e S o u rce R & D M i le s to n e s S c i e n ce G o al s COMPLETED s i ng le e le ct ro n co n v ers i o n e le ct ro n I 2 0 1 0 -2 0 16 8 3 m K r d e t e ct i o n s p e ct r um o f 8 3 m K r p ro o f o f co n ce p t F i n al - s t at e s p e ct r um t e s t Ku r i e p lot I I 2 0 1 5 -2 0 1 7 T 2 3 H - 3 H e m a s s d iff ere n ce s y s te m at i c s t u d i e s m π < 1 0 - 1 0 0 eV/c 2 h i g h - r at e s e n s i t i v i t y I I I 2 0 16 -2 0 2 0 T 2 m π < 2 eV/c 2 B- F i e l d m a p p i ng m π < 4 0 m eV/c 2 ato m i c t r i t i um I V 2 0 1 7 β¦ T s o u rce m e a s u re m π o r d e t e r m i n e no r m al h i er arc hy Project8 β 29
P H A S E - I I : T R I T I U M Improved insert installed β’ first 83m Kr data available β very promising β’ T 2 - system ready to be installed Project8 β 30
P H A S E I I I - L A R G E V O L U M E Example antenna configuration and vertex resolution being modeled β’ Larger bore ~1T magnet β exists β’ Phased array antenna configurations β¨ β under study Project8 β 31
M O L E C U L A R T R I T I U M L I M I TAT I O N S Molecular excitations β¨ ( 3 HeT) + in daughter molecule ( 3 HeH) + β’ blur tritium endpoint β fundamental limit β¨ to measurement β¨ of π -mass Need atomic tritium for ultimate experiment! Advances in High Energy Physics 2013 (2013) 39 Project8 β 32
P H A S E I V: AT O M I C T R I T I U M Studying Ioffe-Pritchard trap β’ couple to nuclear magnetic moment Β΅ Β· ~ β E = β ~ B β’ similar to BEC and anti- hydrogen traps (ALPHA) Challenges β’ cool atomic tritium β¨ to sub-Kelvin β’ need high T/T 2 purity Alexi Radovinsky, MIT Magnet Lab Project8 β 33
S U M M A RY Project 8: β’ new technology: CRES - Cyclotron Radiation Emission Spectroscopy Next step β’ measure full tritium spectrum Longer-term future β’ large scale setup limited by tritium density and molecular excitations β¨ β phased antenna array β¨ β atomic tritium source Project8 β 34
B A C K U P
A D I A B AT I C I N VA R I A N C E Adiabatic invariance β’ Ξ¦ = B β A = B Ο r cycl2 β¨ β p β₯ 2 / (q β B) = const Slowly changing B β’ p β₯ β p || 36 Project8 β
M A C - E F I LT E R Magnetic Adiabatic Collimation with Electrostatic Filter Combination of β’ Adiabatically β¨ changing B-field β¨ β convert E β₯ to E || β’ E-field to β¨ filter by energy Resolution β’ ratio of B s / B A β¨ β limited by size 37 Project8 β
D I S E N TA N G L I N G E N E R G Y A N D A N G L E Electron oscillates in trap β’ axial mode (in harmonic trap) β β 1 β 4 sin ΞΈ a Ο a β v sin ΞΈ + m e cos 2 ΞΈ main β¨ frequency β’ sidebands to β¨ noise level sidebands cyclotron peak β’ distance depends β¨ on pitch angle ΞΈ Project8 β 38
S I D E B A N D O B S E R VAT I O N frequency [MHz] time [s] Project8 β 39
T H R E E D E G R E E S O F F R E E D O M Project8 β 40
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