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TRIµP Laser Spectroscopy: Status and Future U Dammalapati TRI  P Facility Lasers for Na  -decay Ra Spectroscopy & EDM Towards cooling of Heavy Alkaline.

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Presentation on theme: "TRIµP Laser Spectroscopy: Status and Future U Dammalapati TRI  P Facility Lasers for Na  -decay Ra Spectroscopy & EDM Towards cooling of Heavy Alkaline."— Presentation transcript:

1 TRIµP Laser Spectroscopy: Status and Future U Dammalapati TRI  P Facility Lasers for Na  -decay Ra Spectroscopy & EDM Towards cooling of Heavy Alkaline Earth Elements Outlook

2 Production Target RFQ Cooler Optical Trap Beyond The Standard Model TeV Physics TRI  P Facility AGOR Magnetic Separator Atomic Physics Nuclear Physics Particle Physics Energy: MeVeVneV Ion Catcher keV Separator commissioning Successful A Rogachevskiy RFQ prototype test and simulations E Traykov Charge exchange at low energies L Willmann G P Berg, U Dammalapati, P G Dendooven, O Dermois, G Ebberink, M N Harakeh, R Hoekstra, L Huisman, K Jungmann, H Kiewiet, R Morgenstern, G Onderwater, A Rogachevskiy, M Sanchez-Vega, M Sohani, M Stokroos, R Timmermans, E Traykov, L Willmann and H W Wilschut TRIµP – Trapped Radioactive Isotopes: µ-laboratories for fundamental Physics

3  - angular correlations in nuclear  -decay Suitable isotope 21 Na p, q  1MeV/c  260 a.u. E recoil = (p + q) 2 /2M recoil  100 eV  3.6 a.u. p q J Double differential decay probability: Na  -decay

4 Violation of T-Symmetry H= -(d.E+µ.B) d - EDM µ - magnetic dipole moment I - Nuclear spin Limit for nuclear EDM Hg d< 2.1 x 10 –28 e cm M. V. Romalis et al. Phys.Rev.Lett. 86, 2505 (2001) Radium: Excellent candidate V. A. Dzuba et al. Phys. Rev.A61 062509(2000) EDMs violate - Parity - Time Reversal

5 Radium Atomic Structure 482.7 nm 714 nm 7s 2 1 S 0 7s 7p 1 P 1 7s 7p 3 P 7s 6d 1 D 2 7s 6d 3 D 1 2 3 210210 1438 nm 1488 nm  2.8  m Energy level data: E. Rasmussen, Z. Phys. 86, 24 (1933) and 87, 607 (1934); H.N. Russel, Phys. Rev. 46, 989 (1934) Calculations done by K Pachuki and Flaumbam, Dzuba et al. Lifetime measurement Energy level spacing Hyperfine structure Needed for atomic structure calculations Spectroscopy of P and D states

6 Heavy Alkaline Earth Element: Barium  – 8.4nsec I s =14mW/cm 2 1 2 3 Life time measurement Hyperfine structure Laser cooling of barium Develop trapping strategy 791.3 nm 6s 2 1 S 0 6s 6p 1 P 1 6s 5d 1 D 2 6s 6p 3 P 210210 1130 nm 1499 nm 6s 5d 3 D  3  m 1108 nm  – 1.4 µsec I s =30µW/cm 2 553.7 nm Spectroscopy of P and D states

7 Verdi pump at 532 nm Collimator Ba Oven 500  C PD M1 BS Dye Laser Power Stabilization PMT AOM Optical fiber from 791.3 nm diode laser 553.7 nm Coherent 699 Single mode dye laser BB /2

8 138 Ba 137 Ba F=5/2 138 Ba 135 Ba 136 Ba in Polarization plane  Polarization plane Fluorescence at 553.7 nm from different Ba isotopes Counts [kHz] PMT Counts [kHz] Frequency [MHz]

9 Hanle effect Life time of 1 P 1 state P laser  B field  eff = h/(2  g J   B 1/2 )  eff = 8 nsec  0.5sec 138 Ba 136 Ba 138 Ba 136 Ba Counts [kHz] Magnetic Field [G]

10 553.7 nm 791.3 nm 6s 2 1 S 0 6s 6p 1 P 1 6s 6p 3 P 1 6s 5d 3 D  3  m 1.4 µsec 8.4 nsec 40% 60% Creation of intense beam of meta-stable D-state atoms 321321 Intercombination line 1 S 0 – 3 P 1

11 FM Saturated absorption spectroscopy of I 2 Diode Laser 791.3 nm I 2 Oven (560ºC) M1 M3 BS PD Lock-In Amp Feedback Control VCO /4 AOM To Beat note Lock point Reference Line P(52)(0-15) transition f=f 0 +f 1 Sin(wt) w=90.5kHz 599 MHz away from 1 S 0 – 3 P 1 in 138 Ba

12 Hyperfine Splitting of 1 S 0 – 3 P 1 transition in an External Magnetic field  = g J µ m J B  IS = 138 Ba– 136 Ba= 108.5 (3) MHz 2.3 MHz

13 Outlook Diode Laser for 1 P 1 – 1 D 2 transition @1500nm and for 1 P 1 – 3 D 2 and 1 P 1 – 3 D 1 transitions @1130&1108nm) Towards Radium Laser @482.5nm for 1 S 0 – 1 P 1 transition by frequency doubling Ti:Sapp Laser Production of Radium at TRIµP by end of 2004 Spectroscopy in a Radium beam Laser Cooling of Barium

14 Producing light for Ra 1 S 0 - 1 P 1 transiton Second harmonic generation in linear cavity using KNbO 3 (b-cut, 19°) 3 or 5mm; temperature tunable and high efficiency Wavelength tunable from 480 nm (10°C) to 490 nm (40°C) M1 M2 Telescope BS Split PD PZT R=-50mm, HR485 nm & 970 nm Faraday Isolator Ti:Sapp Dichroic Mirror KNb0 3 HR AR Blue output


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