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27 - 31 October 2014 Trento, Italy
Measurements of kaonic 4He and 3He at DANE
Achievements and Perspectives in Low-Energy QCD with Strangeness
Diana Laura Sirghi
INFN-LNF
on behalf of SIDDHARTA collaboration
the determination of the isospin dependent KN scattering lengths through a
~ eV measurement of the shift~ eV measurement of the shift and of the width
of the K line of kaonic hydrogen andthe first (similar) measurementfirst (similar) measurement of kaonic deuterium
The scientific aimThe scientific aim
Fundamental study of Fundamental study of strong interactionstrong interaction
between anti-K & nucleus at low energy limitbetween anti-K & nucleus at low energy limit
Fundamental study of Fundamental study of strong interactionstrong interaction
between anti-K & nucleus at low energy limitbetween anti-K & nucleus at low energy limit
The scientific aimThe scientific aim
SIDDHARTA measures the SIDDHARTA measures the X-ray transitionsX-ray transitions
occurring in the cascade processes occurring in the cascade processes
of kaonic atomsof kaonic atoms
In the framework of the SIDDHARTA experiment we have performed the measurements related with the Kaonic helium transition to the 2p level (L-lines):
- for first time in a gaseous target for 4He- for the first time ever for K3He
The interest for such type of measurement was rather high due to:
so-called “kaonic helium puzzle”
some theoretical predictions of possible very small energy shift
(if any)
Kaonic Helium measurements SIDDHARTA experiment
Kaonic Helium atomsKaonic Helium atoms
ε = E3d 2p (exp) – E3d 2p (e.m.)
The most suitable transition to observe the strong interaction effects
The most suitable transition to observe the strong interaction effects
The absorption is too strong to observe the radiative transition to 1s state
the last observable state is the 2p state
The absorption is too strong to observe the radiative transition to 1s state
the last observable state is the 2p state
Kaonic atom data (Z≥3)
Kaonic atom data (Z≥3)Used for studies of KbarN interaction
Optical model
Experimental X-ray data of shift & width:Well fitted with optical potentials
Expected shift of K-4He 2p state:ΔE ~ 0 eV
C.J. Batty et al., Physics Reports 287(1997) 385-445
The shift and widths of kaonic atom X-ray energy have been measured using targets with atomic numbers from Z=1 to Z-92, which provide very important quantities for understanding the antiKN strong
interaction.
There are discrepancies for:
Kaonic Hydrogen
(Z=1)
Kaonic Helium
(Z=2)
E2p(eV) 2p (eV)
-41±33 -
-35±12 30±30
-50±12 100±40
-43±8 55±34
Kaonic helium atom data (Z=2)Kaonic helium atom data (Z=2)
1971
1979
1983
Averageof above
Kaonic helium atoms theoretical valuesKaonic helium atoms theoretical values
Shift (eV) Ref.
-0.13±0.02 Batty, NPA508
(1990) 89c
-0.14±0.02 Batty, NPA508
(1990) 89c
-1.5 Akaishi, Proc. EXA05
There are two types of theories compared to the experimental results:
Optical-potential model:
(theoretical calculations based on kaonic atom data with Z> 2)
Tiny shift(E2p 0 eV)
Recent theoretical calculations:
Akaishi-Yamazaki model of deeply-bound kaon-nucleus states
Predicts a possible maximum shift:E2p of ± 10 eV
What is What is Kaonic helium puzzle?Kaonic helium puzzle?
Need a new K-4He X-ray measurement!
Experiment:Large shift
(E2p 40 eV)
Theory:E2p 0 eV
or< ± 10 eV
New KNew K44He results by KEK PS E570He results by KEK PS E570
PLB 653 (2007) 387
E2p =2±2(stat.)±2(syst.) eV)
K4He 3d→2p: 1500 events
3x higher statistics2x better Energy resolution6x better S/N
Solving the kaonic helium puzzleSolving the kaonic helium puzzle
Old experiments:Large shift(-43±8 eV)
E570 experiment:Small shift
(+2±2±2 eV)
Theory:E2p 0 eV
or< ± 10 eV
Difference between the new and the old experiments
Experimental confirmation need!SIDDHARTA experiment
SIDDHARTA experimentSIDDHARTA experiment
Monochromatic, low-momentum kaon beam from DANE (127 MeV/c)
No hadronic background due to the beam line (compare with hadron beam line :e.g with KEK line)
Big advantages of the SIDDHARTA experiment:
•Low density gas target (higher yields of the atomic state in gaseous helium over the liquid one, due to the density dependent Stark mixing; negligible Compton scattering in helium).
•The availability of kaons with low energy and low momentum spread results in efficient kaon stopping in gas target.
•Silicon Drift Detector (SDDs) as detector
1515
xy
z
e-
510 MeV/c510 MeV/ce+
510 MeV/c510 MeV/c127 MeV/127 MeV/ccΔΔpp//pp=0.1%=0.1% K+
K-
Φ
TargetTarget
DetectDetectby SDDsby SDDs
Detect by Detect by two two scintillatorsscintillators
SIDDHARTA overviewSIDDHARTA overview
1 cm1 cm22 x 144 x 144 SDDsSDDs
Silicon Drift Detector - SDD Silicon Drift Detector - SDD
SDD Energy resolution: 150 eV (at 6 keV)
SDDs & SDDs & TargetTarget(inside (inside vacuum)vacuum)
Kaon Kaon detectordetector
SIDDHARTA setup SIDDHARTA setup
Kaonic Kaonic 44He dataHe dataSIDDHARTA experimentSIDDHARTA experiment
The Kaonic 4He X-ray data were taken for about two weeks in January 2009.
In this period, an integrated luminosity of about 20pb-1 was collected.
This corresponds to about 4.7 × 106 kaons detected by the kaon detector.
SDD spectrum of X-ray uncorrelated with kaon production.Ti and Mn X-ray peaks are produced by the 55Fe source in normal condition of beam
Energy resolution: FWHM (@6.4 keV): 151 ± 2 eV
Energy calibrationEnergy calibration
Target
Ti foil
Fe55
Degrader
K-He data taking
Energy spectrum of K-Energy spectrum of K-44He X-raysHe X-rays
Energy of K4He L (3d2p) line:
Eexp = 6463.6±5.8 eV
New results of K-New results of K-44He 2p level shiftHe 2p level shift
Eexp = 6463.6±5.8 eV Ee.m. = 6463.5±0.2 eV
E = Eexp – Ee.m. = 0±6(stat) ±2(syst) eV
Published in PLB 681(2009) 310-314
“kaonic helium puzzle” solved
SIDDHARTA’s results is consistent with the results obtained by E570 experiment
Data taking periods Data taking periods of SIDDHARTA in 2009of SIDDHARTA in 2009
DANE shutdown in Summer
New alignment of setupImprove S/N ratio
K-He3 data (~4days)
55Fe source: Good for reduce sys. error on K-4HeBad for “background” events on K-H,K-D
Removed 55Fe source in other data
e e
SDDs
Ti/Cu foil
X-ray tube
Data taking scheme at DAFNE
calibration data
e e
K
K
SDDs
degrader
Scintillators
Production data
Calibration data with X-ray tube have been collected under the beam condition in regular interval of the production runs.
For that purpose a remote controlled mechanism was built to move away the kaon detector and instead have the x-ray tube
in place.
SDD X-ray energy spectra
Cal
ibra
tion
data
with
X-r
ay t
ub
eCalibration Ti&Cu
e e
SDDs
Ti/Cu foil
X-ray tube
calibration data
Instead of Fe source, “X-ray tube” data taken
Estimated systematic error ~ 3-4 eV
In-beam
X ray tube
Ti, Cu foils
SDD X-ray energy spectra
Cal
ibra
tion
data
with
X-r
ay t
ub
eN
ot
corr
elat
ed t
o
Kao
n si
gnal
s
Pro
duct
ion
data
Energy scale determinedby X-ray tube data
Energy spectrum withuncorrected to kaon timing[Fig. (b)]
ee
K
K
X-ray SDDs
degrader
Scintillators
ee
K
K
X-ray SDDs
degrader
Scintillators
Calibration Ti&Cu
providing large statistics background events + X-Ray lines form the target maetrials induced
by the beam background
SDD X-ray energy spectra
Cal
ibra
tion
data
with
X-r
ay t
ub
eN
ot
corr
elat
ed t
o
Kao
n si
gnal
sS
elec
ted
with
K+
K-
& S
DD
tim
ingPro
duct
ion
data
Kaon detector
Time difference between SDD & Kaon detector
providing kaonic atom X-ray energy spectra with a high background suppression.
SDD X-ray energy spectra
Cal
ibra
tion
data
with
X-r
ay t
ub
eN
ot
corr
elat
ed t
o
Kao
n si
gnal
s
Pro
duct
ion
data
The shift is due to the instability of our electronics caused by differing conditions between the production and X-ray tube data.The largest contribution is a rate-dependent effect on the SDDs.The hit rate of the SDDs in the X-ray tube data was about 10 times higher than that in the production data, causing the observed shift.
High rate
Low rate
High rate
Low rate
The X-ray peak fit
The accuracy of the energy scale was determined by using X-rays energis of the TiKa, CuKa and Au La lines.The intensities of these X-ray lines in the kaonic helium data were not high enough to observe systematic effects on the energy calibration and energy resolution of the SDDs, so the data measured with the deuterium target, which were taken for about 20 days, were also analyzed using the same method.
Natural line widths taken into account
X-ray peaks are fitted with Voigt function
Determination of the accuracy of the energy scale of the SDDs: using production data not correlated with the kaon signal
The peak position
The vertical axis gives the difference between the fit values and the reference data.
Result of the fit:energy scale in the production data is shifted by −6 eV compared to the reference data.
The accuracy of the energy determination was ±4 eV in the energy region from 4 keV to 10 keV.
The variation of ±4 eV corresponds to the uncertainty of about ±0.2 channels in the analogue-to-digital converters (ADCs) used in the measurements. The variation could be related to the nonlinearity of ADCs.
The uncertainty of ±4 eV is taken as a systematic error in the energy determination.
DAFNE shutdown in Summer
Kaonic Kaonic 33Helium data SIDDHARTA experimentHelium data SIDDHARTA experiment
The Kaonic- 3He X-ray data were taken for about 4 days in November 2009.
In this period, an integrated luminosity of about 16 pb-1 was collected.
The Kaonic-The Kaonic-33He caseHe case
TransitionKaonic-3He e.m.
(eV)(*)
3d->2p 6224
4d->2p 8399
5d->2p 9406
There are NOT previous experiments done for the X-ray measurements for Kaonic- 3He
Planned experiments: SIDDHARTA (done);
E17 (to be done)
(*)Zeitschrift fur Physik D 15 (1990) 321
Kaonic Helium-3 energy spectrumextraction of the strong interaction shift
Eexp=6223.0±2.4(stat)±3.5(syst.) eV
Ee.m.=6224.6 eV
The calculation of the e.m. energies for kaonic 3He was done using the Klein –Gordon equation and the vacuum polarization from the first order term of the Uehling potential.
ε=ΔE2p= Eexp-Ee.m. = -2±2(stat)±4(syst)
World First !Observation of K-3He X-rays
Determination of strong-interaction shift
PLB 697 (2011) 199. Cited 13 times
Target material: Kapton Polymide (C22H10N2O5)
DANE shutdown in Summer
K-4He (3d-2p)
eV)(4)(352 sysstaE p
More date on K-More date on K-44He 2p level shiftHe 2p level shift
Experimental results for the widths Experimental results for the widths of kaonic helium atomsof kaonic helium atoms
Average:
Theory: -0.13+-0.02 1.8+-0.05
Nuclear Physics A392 (1983) 297-310
“The shift measurements are seen to be in good agreement. The situation for the width values is much less satisfactory and theerror bars of the two measured values do not overlap. The error on the quoted average has been taken from the external variance of the measured values.”
New experiment for the widths of the 2p state for kaonic helium: SIDDHARTA experiment
Uncertainty of detector resolutionUncertainty of detector resolution
Due to the strong correlation between the detector resolution and line width of KHe, the detector resolution was fiexd form the production data not correlated with the kaon signal
Since all the positions are located within the error curves, the error is taken as the accuracy of the determination of the dector resolution for the fit of the kaonic helium X-rays.
3d→2p = (65.4±2.3) eV
K-3He
3d→2p = (66.4±2.3) eV
K-4He
The energy dependence of the energy resolution of the SDDs: evaluated from the widths of the peaks of Ti, Cu and Au
The deviations from the fit file are plotted for
each target material
Results for the widths of K-3He and K-4HeResults for the widths of K-3He and K-4He
The energy shift and broadening of the 3d→2p transition can be obtained from the peak fit using a Voigt Function V=V(, ), where represents the strong-interaction 2p width and was fixed using the values obtained from the energy resolution of the detector.
The systematic error was evaluated from the uncertainity of the resolution .
In addition, since the K-3He peak partially overlaps the K-O transition, the systematic error of the width of K-3He includes the uncertainity of its intensity.
Summary of the results
Experiment Target Shift [eV] Reference
KEK E570 Liquid +2±2±2 PLB653(07)387
SIDDHARTA (He4 with 55Fe) Gas +0±6±2 PLB681(2009)310
SIDDHARTA (He4) Gas +5±3±4 arXiv:1010.4631,
PLB697(2011)199SIDDHARTA (He3) Gas -2±2±4
*error bar 22 )()( syststat
Results for the shifts and widths Results for the shifts and widths of K-3He and K-4Heof K-3He and K-4He
• The large shift and width obtained by the experiments done in 70-80 was not observed in kaonic 3He and 4He.
• The results for shift and width agree with the theoretical calculations.
• No abnornally large shift abd width were found.
L-series X-ray yields ofL-series X-ray yields ofKaonic Helium atoms in gaseous Kaonic Helium atoms in gaseous
targetstargets
By using accurate Monte Carlo simulations, the absolute yields of the kaonic 3He and 4He X-ray transitions to the 2p state was successfully determined by the SIDDHARTA experiment .
The measured yields provide information for understanding the cascade processes of kaonic helium atoms as a function of the target density.
L-series X-ray yields ofL-series X-ray yields ofKaonic Helium atoms in gaseous targetsKaonic Helium atoms in gaseous targets
The absolute X-ray yield is defined as the X-ray intensityper stopped kaon.
The X ray detection efficiency is defined as the number of measured X-rays normalized by the number of K+K− events recorded in the kaon detector :
Comparing these efficiencies to those given by Monte Carlo simulations, the absolute yields of the kaonic atom X-
rays can be determined.
(*) C.E. Wiegand, R. Pehl, Phys. Rev. Lett. 27, 1410 (1971).(**) S. Baird et al., Nucl. Phys. A 392, 297 (1983).
• The yields of the Lα lines in gas are about 2.0–2.5 times higher than in liquid• The yields of the Lβ and Lγ lines are consistent. •The intensities of the Lhigh lines in gas are obviously higher than those in liquid.
These yield differences are related to the density dependence of the cascade processes, such as the molecular Stark effect and molecular ion formation.
D (2.50 g/l)
3He (0.96 g/l)
4He (1.65 g/l)
4He (2.15 g/l)
The absolute X-ray yield (Y ) per stopped K−:In performing the comparison, the normalization was done using the number of K+K− events detected by the kaon detector.
ConclusionsConclusions SIDDHARTA experiment measured the kaonic helium 3d2p transitions:
for the first time ever for 3He.
for the first time in a gaseous target for 4He
Shift and width are founded to be few eV both in K-3He and K-4He
No abnormally large shift and width were found in K-3He and K-4He
These results agree with theoretical calculations
The kaonic helium puzzle was solved for shift and width both K-3He and K-4He.
These results agree with theoretical calculations
The absolute X-ray yields of L-series lines were determined for the first time
DANE proves to be a “ideal” kaonic atom “factory”.
Future plansFuture plans
The upgrade of the SIDDHARTA experimental setup
Precise measurements for the X-ray transitions for kaonic deuterium.
Measuring, with higher precision, the X-ray transitions for Kaonic 4He and Kaonic 3He to the 2p level and the first tempt to get the transitions to the 1s level.
SIDDHARTA 2 experiment
Kaonic atoms data (Z>3)Kaonic atoms data (Z>3)
The shifts and widths for kaonic atoms with Z≥3 are systematically well understood;
The optical model expressing the kaonic atom data have been used for calculation of the antiKaonN interaction.
C.J. Batty et al., Physics Reports 287(1997) 385-445
The shift and widths of kaonic atom X-ray energy have been measured using targets with atomic numbers from Z=1 to Z-92, which provide very important quantities for understanding
the antiKN strong interaction.
There are discrepancies for:
Kaonic Hydrogen
(Z=1)
Kaonic Helium
(Z=2)
See talk of A. Romero Vidal
DAFNE shutdown in Summer New alignment of setupImprove S/N ratio
K-He3 data (~4days)
55Fe source: Good for reduce sys. error on K-4HeBad for “background” events on K-H,K-D
Removed 55Fe source in other data
Data taking periods Data taking periods of SIDDHARTA in 2009of SIDDHARTA in 2009
X ray energy (keV)
Cou
nts
/ bin
KH
e (3
-2)
KC
(6-
5)
KH
e (4
-2)
transition e.m.energy events(3-2) 6.464 1047 ± 37(4-2) 8.722 154 ± 21(5-2) 9.767 91.8 ± 19(6-2) 10.333 82.4 ± 25higher < 11.63 131 ± 41
Ti K
KHe used forgasstop optimization+ physics interest1)
data from setup 2(no Fe55 source)
1) compare KEK E570KHe L lines in liquid He,consistent result,first measurement in gas
KH
e (5
-2)
KN
(5-
4)
KH
e L h
igh
p r e l i m i n a r y
KC
(5-
4)
KH
e (6
-2)
KO
(6-
5)
KO
(7-
6)
Higher statistics of the K-4He L lines (L, Lβ, L)
Smaller statistics in shift, determination of width
X-ray yield information in gas (for the first time)
Very preliminary K-Very preliminary K-44He spectrum He spectrum
e e
SDDs
Ti/Cu foil
X-ray tube
Data taking at DAFNE -Calibration
calibration data
Estimated systematic error ~ 3-4 eV
Seminar TUM, 27 June 2011
e e
K
K
SDDs
degrader
Scintillators
Production data
Data taking at DAFNE - Production
Seminar TUM, 27 June 2011
X ray energy (keV)
Cou
nts
/ bin
KH
e (3
-2)
KC
(6-
5)
KH
e (4
-2)
KC
(5-
4)
transition e.m.energy events(3-2) 6.224 1209 ± 40(4-2) 8.399 220 ± 22(5-2) 9.406 90.0 ± 18(6-2) 9.953 65.8 ± 24higher < 11.4 397 ± 40
Ti K
KHe3never measured before !
KH
e (5
-2)
p r e l i m i n a r y
KH
e L h
igh
KH
e (6
-2)
KO
(6-
5)
KN
(5-
4)
KO
(7-
6)
Very preliminary K-Very preliminary K-33He spectrumHe spectrum
The statistical error for the transition 3d2p in K 3He is less than 3 eV.
Target Shift [eV]
KEK E570 Liquid +2±2±2 eV
SIDDHARTA (w/ 55Fe) Gas +0±6±2 eV
SIDDHARTA (New) Gas +5±3±4 eV
Comparison of results
Target Shift [eV]
SIDDHARTA Gas -2±2±4 eV
J-PARC E17 Liquid planned
..exp2 mep EEE
Kaonic 4He 2p level shift
Kaonic 3He 2p level shift
shift),"repulsive("0
),"attractive("0
2
2
shiftE
shiftE
p
p
Conclusions (2)Conclusions (2)
Confirmed the small shift obtained by recent experiment E570 for Kaonic 4Helium
The “kaonic helium puzzle” for Kaonic 4Helium is now solved
The preliminary analysis of the 3d2p transitions for Kaonic 3Helium, indicate that the statistic error shift is less than 3 eV.
e e
SDDs
Ti/Cu foil
X-ray tube
Data taking scheme at DAFNE
calibration data
e e
K
K
SDDs
degrader
Scintillators
Production data
Instead of Fe source, “X-ray tube” data taken
Estimated systematic error ~ 5 eV
- rebuilding of the sdds mounts: gain of solid angle of X ray detectors- replacement of sdd modules: 144 cm2 detectors operational- new upper kaon detector: less material in vicinity of target, clean trigger- improved shielding: new multimaterial and more narrow collimator
Setup improvements during summer 2009 shutdownSetup improvements during summer 2009 shutdown
Recent theoretical calculation for the Recent theoretical calculation for the width of kaonic helium atomswidth of kaonic helium atoms
theoretical calculations ofphenomenological optical
potential model by Friedman
Akaishi-Yamazaki model of deeply-bound kaon-nucleus states
Small width(E2p 2 eV)
Possible large width 5eV
K-4He K-3He
Contamination of K-O peakContamination of K-O peak
Several small peaks were observed in all the spectram which originated from kaonic atom X-rays produced in the target window material (C22H10N2O5)
The X-rays peaks are: (K-C) 6→5
(K-O) 7→6,(K-C) 6→5
(K-N) 6→5
(K-C) 8→6
Kaonic Helium atomsKaonic Helium atoms
p d f
3d 2p X ray
E2p (exp.)
n
4
3
2
Strong Interaction causes:energy shift
of the last energy levels form their purely electromagnetic
values AND
level width finite lifetime of the state
corresponding to an increase in the observed
level width
electromagnetic cascade
K- stopped in He
Repulsive type
Attractive type
Kaonic Helium atom: last orbit 2p
E2p (e.m.)