A. Feliciello / IEEE Nuclear Science Symposium and Medical Imaging Conference, Honolulu, Hawaii, USA, October 27-November 3, 2007. Alessandro Feliciello I.N.F.N. - Sezione di Torino The new FINUDA challenge: γ-ray spectroscopy of hypernuclei at DAΦNE The new FINUDA challenge: γ-ray spectroscopy of hypernuclei at DAΦNE γ n n n n n p p p p p p Λ
16
Embed
Alessandro Feliciello - Istituto Nazionale di Fisica Nuclearepersonalpages.to.infn.it/~feliciel/pub/mySlides/IEEE-NSS... · A. Feliciello / IEEE Nuclear Science Symposium and Medical
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
A. F
elic
iello
/ IE
EE N
ucle
ar S
cien
ce S
ympo
sium
and
Med
ical
Imag
ing
Con
fere
nce,
Hon
olul
u, H
awai
i, U
SA, O
ctob
er 2
7-N
ovem
ber 3
, 200
7.
Alessandro FelicielloI.N.F.N. -
Sezione di Torino
The new FINUDA challenge: γ-ray spectroscopy of hypernuclei
at DAΦNE
The new FINUDA challenge: γ-ray spectroscopy of hypernuclei
at DAΦNE
γn
nnn
np
pp
p ppΛ
2A.
Fel
icie
llo /
IEEE
Nuc
lear
Sci
ence
Sym
posi
um a
nd M
edic
al Im
agin
g C
onfe
renc
e, H
onol
ulu,
Haw
aii,
USA
, Oct
ober
27-
Nov
embe
r 3, 2
007. Outline Outline
Discovery potential of the strangeness nuclear physics
Need of sub-MeV resolutionapparatuses
γ-ray spectroscopy
Ideas for FINUDA spectrometer upgrade at DAΦNE/DAΦNE2
3A.
Fel
icie
llo /
IEEE
Nuc
lear
Sci
ence
Sym
posi
um a
nd M
edic
al Im
agin
g C
onfe
renc
e, H
onol
ulu,
Haw
aii,
USA
, Oct
ober
27-
Nov
embe
r 3, 2
007.
(low-energy) YN interaction
detailed knowledge of the hypernuclear fine structure
→ evaluation of the spin dependent terms of the ΛN interaction
measurement of angular distribution of γ–rays
→ determination of spin and parity of each observed level
Impurity nuclear physicsmeasurement of transition probability B(E2)
→ information on the size and deformation of hypernuclei
→ measurement of nucleus core shrinking → glue-like role of Λ
Properties of hyperons in nuclear matter (medium effect)measurement of transition probability B(M1)→ g-factor value for Λ in nuclear matter
Open questionsOpen questions
4A.
Fel
icie
llo /
IEEE
Nuc
lear
Sci
ence
Sym
posi
um a
nd M
edic
al Im
agin
g C
onfe
renc
e, H
onol
ulu,
Haw
aii,
USA
, Oct
ober
27-
Nov
embe
r 3, 2
007.
energy 510 MeV
luminosity 5 1032
cm-2
s-1
σx (rms) 2.11 mm
σy (rms) 0.021 mm
σz (rms) 35 mm
bunch length 30 mm
crossing angle 12.5 mrad
frequency (max) 368.25 MHz
bunch/ring up to 120
part./bunch 8.9 1010
current/ring 5.2 A (max)
FINUDA @ DAΦNE FINUDA @ DAΦNE
−Λ
−
+−+−
+→+
→→+
π
φ
ZZΚΚΚee
AAstop
→Λ ZA
nnZnpZ
Z
A
A
A
++
++−
++
−
−
−
)2(
)2( )1()1( π
5A.
Fel
icie
llo /
IEEE
Nuc
lear
Sci
ence
Sym
posi
um a
nd M
edic
al Im
agin
g C
onfe
renc
e, H
onol
ulu,
Haw
aii,
USA
, Oct
ober
27-
Nov
embe
r 3, 2
007. The status of the artThe status of the art
ΔE ~
1.6
5 MeV
FW
HM
ΔE ~
1.6
5 MeV
FW
HM
ΔE ~
1.9
5 MeV
FWHM
ΔE ~
1.9
5 MeV
FWHM
ΔE ~ 1.29 MeV
FWHMΔE ~ 1.29 MeV
FWHM
−BΛ (MeV)
Cap
ture
rat
e/0.
25 M
eV x
10−
3
0
0.1
0.2
0.3
0.4
0.5
0.6
−25 −20 −15 −10 −5 10 150 5
#6
#4#3
#2
#1#5
#7
b)M. Agnello et al., Phys. Lett. B 622 (2005) 35 M. Agnello et al., Phys. Lett. B 622 (2005) 35
( ) CK,π 12Λ
++
ΔE ~
1.4
5 MeV
FWHM
ΔE ~
1.4
5 MeV
FWHM
f-orb
it sp
littin
g
into t
wo pea
ks ob
serve
d?
f-orb
it sp
littin
g
into t
wo pea
ks ob
serve
d?
6A.
Fel
icie
llo /
IEEE
Nuc
lear
Sci
ence
Sym
posi
um a
nd M
edic
al Im
agin
g C
onfe
renc
e, H
onol
ulu,
Haw
aii,
USA
, Oct
ober
27-
Nov
embe
r 3, 2
007. The status of the artThe status of the art
7Li(K-
,π-)12C7Li(K-
,π-)12C−stopK Li7
Λ
KEK E419
KEK E419
ΔE ~ 1.1 MeV FWHMΔE ~ 1.1 MeV FWHM
ΔE ~ 2 keV
FWHMΔE ~ 2 keV
FWHM
3
order of magnitude!!!3
order of magnitude!!!
7A.
Fel
icie
llo /
IEEE
Nuc
lear
Sci
ence
Sym
posi
um a
nd M
edic
al Im
agin
g C
onfe
renc
e, H
onol
ulu,
Haw
aii,
USA
, Oct
ober
27-
Nov
embe
r 3, 2
007. The γ-ray spectroscopy domain The γ-ray spectroscopy domain