Level densities and gamma-ray strength functions

 

The data are extracted according to the Oslo-method (A. Schiller et al., Nucl. Instrum. Methods A 447 (2000) 498). For the present data set, both the (3He,3He) and (3He,4He) reactions have been used. A comparison between the two reactions is performed in Ref.: A. Schiller et al., Phys. Rev. C61, 044324 (2000).

Some papers show, together with new data, also previously published data. These may be identical, however, in some cases small adjustments have been made from more recent information, e.g. new (n,g) neutron resonance spacing data. Therefore, the data from the most recent paper should be adopted.

You may download these data and pdf figures. If you publish them, please give references to the method and the journal where the data were published (see below).

If you have comments or questions, please contact magne.guttormsen[]fys.uio.no


Level densities

You may download pdf figures for some of these data here:
SmDyErYb, Dy, Yb, Mo, Fe, V, new 96Mo, Sc, new 56,57Fe, 116,117Sn

A. Schiller et al., Phys. Rev. C63, 021306(R) (2001): (3He,4He)161Dy
A. Schiller et al., Phys. Rev. C63, 021306(R) (2001): (3He,4He)162Dy

E. Melby et al., Phys. Rev. C63, 044309 (2001): (3He,4He)166Er
E. Melby et al., Phys. Rev. C63, 044309 (2001): (3He,3He)167Er

A. Schiller et al., Phys. Rev. C63, 021306(R) (2001): (3He,4He)171Yb
A. Schiller et al., Phys. Rev. C63, 021306(R) (2001): (3He,4He)172Yb

S. Siem et al., Phys. Rev. C65, 044318 (2002): (3He,4He)148Sm
S. Siem et al., Phys. Rev. C65, 044318 (2002): (3He,3He)149Sm

M. Guttormsen et al., Phys. Rev. C68, 064306 (2003): (3He,4He)160Dy
M. Guttormsen et al., Phys. Rev. C68, 064306 (2003): (3He,3He)161Dy
M. Guttormsen et al., Phys. Rev. C68, 064306 (2003): (3He,4He)161Dy
M. Guttormsen et al., Phys. Rev. C68, 064306 (2003): (3He,3He)162Dy
M. Guttormsen et al., Phys. Rev. C68, 064306 (2003): (3He,4He)162Dy

A. Schiller et al., Phys. Rev. C68, 054326 (2003): (3He,4He)56Fe
A. Schiller et al., Phys. Rev. C68, 054326 (2003): (3He,3He)57Fe

A. Schiller et al., Phys. Rev. C68, 054326 (2003): (3He,4He)96Mo
A. Schiller et al., Phys. Rev. C68, 054326 (2003): (3He,4He)97Mo

U. Agvaanluvsan et al., Phys. Rev. C70, 054611 (2004): (3He,4He)170Yb
U. Agvaanluvsan et al., Phys. Rev. C70, 054611 (2004): (3He,3He)171Yb
U. Agvaanluvsan et al., Phys. Rev. C70, 054611 (2004): (3He,4He)171Yb
U. Agvaanluvsan et al., Phys. Rev. C70, 054611 (2004): (3He,3He)172Yb
U. Agvaanluvsan et al., Phys. Rev. C70, 054611 (2004): (3He,4He)172Yb

R. Chankova et al., Phys. Rev. C73, 034311 (2006): (3He,4He)93Mo
R. Chankova et al., Phys. Rev. C73, 034311 (2006): (3He,3He)94Mo
R. Chankova et al., Phys. Rev. C73, 034311 (2006): (3He,4He)95Mo
R. Chankova et al., Phys. Rev. C73, 034311 (2006): (3He,3He)96Mo
R. Chankova et al., Phys. Rev. C73, 034311 (2006): (3He,4He)96Mo
R. Chankova et al., Phys. Rev. C73, 034311 (2006): (3He,3He)97Mo
R. Chankova et al., Phys. Rev. C73, 034311 (2006): (3He,4He)97Mo
R. Chankova et al., Phys. Rev. C73, 034311 (2006): (3He,3He)98Mo

A.C. Larsen et al., Phys. Rev. C 73, 064301 (2006): (3He,4He)50V
A.C. Larsen et al., Phys. Rev. C 73, 064301 (2006): (3He,3He)51V

Reanalyzed 2008, R. Chankova et al., Phys. Rev. C73, 034311 (2006): (3He,3He)96Mo
Reanalyzed 2008, R. Chankova et al., Phys. Rev. C73, 034311 (2006): (3He,4He)96Mo

A.C. Larsen et al., Phys. Rev. C 76, 044303 (2007): (3He,4He)44Sc
A.C. Larsen et al., Phys. Rev. C 76, 044303 (2007): (3He,3He)45Sc

E. Algin et al., Phys. Rev. C 78, 054321 (2008): (3He,4He)56Fe
E. Algin et al., Phys. Rev. C 78, 054321 (2008): (3He,3He)57Fe

U. Agvaanluvsan et al., Phys. Rev. C79, 014320 (2009): (3He,4He)116Sn
U. Agvaanluvsan et al., Phys. Rev. C79, 014320 (2009): (3He,3He)117Sn

N.U.H. Syed et al., Phys. Rev. C79, 024316 (2009): (3He,4He)205Pb
N.U.H. Syed et al., Phys. Rev. C79, 024316 (2009): (3He,3He)206Pb
N.U.H. Syed et al., Phys. Rev. C79, 024316 (2009): (3He,4He)207Pb
N.U.H. Syed et al., Phys. Rev. C79, 024316 (2009): (3He,3He)208Pb

N.U.H. Syed et al., Phys. Rev. C80, 044309 (2009): (p,d)45Ti

H.K. Toft et al., Phys. Rev. C81, 064311 (2010): (3He,4He)118Sn
H.K. Toft et al., Phys. Rev. C81, 064311 (2010): (3He,3He)119Sn

M. Guttormsen et al., Phys. Rev. C83, 014312 (2011): (p,p)46Ti

H.K. Toft et al., Phys. Rev. C83, 044320 (2011): (3He,4He)121Sn
H.K. Toft et al., Phys. Rev. C83, 044320 (2011): (3He,3He)122Sn

H.T. Nyhus et al., Phys. Rev. C85, 014323 (2012): (3He,4He)163Dy
H.T. Nyhus et al., Phys. Rev. C85, 014323 (2012):  (3He,3He)164Dy

A. Bürger et al., Phys. Rev. C85, 064328(2012): (p,4He)43Sc

A.C. Larsen et al., Phys. Rev. C85, 014320 (2012), CT-norm.: (p,t)44Ti
A.C. Larsen et al., Phys. Rev. C85, 014320 (2012), GHK-norm.: (p,t)44Ti

Normalisation with E&B 2005 (see paper):

A.C. Larsen et al., Phys. Rev. C87, 014319 (2013): (3He,4He)105Cd
A.C. Larsen et al., Phys. Rev. C87, 014319 (2013): (3He,3He)106Cd
A.C. Larsen et al., Phys. Rev. C87, 014319 (2013): (3He,4He)111Cd
A.C. Larsen et al., Phys. Rev. C87, 014319 (2013): (3He,3He)112Cd

M. Guttormsen et al., Phys. Rev. C88, 024307 (2013): (3He,4He)231Th
M. Guttormsen et al., Phys. Rev. C88, 024307 (2013)(3He,3He)232Th
M. Guttormsen et al., Phys. Rev. C88, 024307 (2013)(d,p)233Th
M. Guttormsen et al., Phys. Rev. C88, 024307 (2013): (d,t)237U
M. Guttormsen et al., Phys. Rev. C88, 024307 (2013): (d,d)238U
M. Guttormsen et al., Phys. Rev. C88, 024307 (2013): (d,p)239U

M. Guttormsen et al., Phys. Rev. C89,014302 (2014): (3He,t)232Pa
M. Guttormsen et al., Phys. Rev. C89,014302 (2014): (3He,d)233Pa

H. Utsunomiya et al., Phys. Rev. C88, 015805 (2013): (3He,3He)94Mo
H. Utsunomiya et al., Phys. Rev. C88, 015805 (2013): (3He,4He)95Mo
H. Utsunomiya et al., Phys. Rev. C88, 015805 (2013): (3He,3He)96Mo
H. Utsunomiya et al., Phys. Rev. C88, 015805 (2013): (3He,3He)97Mo
H. Utsunomiya et al., Phys. Rev. C88, 015805 (2013): (3He,3He)98Mo

M. Guttormsen et al., Phys. Rev. C90,044309 (2014): (p,p)89Y
M. Guttormsen et al., Phys. Rev. C90,044309 (2014): (d,p)90Y

T.K. Eriksen et al., Phys. Rev. C90, 044311 (2014): (3He,4He)105Pd
T.K. Eriksen et al., Phys. Rev. C90, 044311 (2014): (3He,3He)106Pd
T.K. Eriksen et al., Phys. Rev. C90, 044311 (2014): (3He,4He)107Pd
T.K. Eriksen et al., Phys. Rev. C90, 044311 (2014): (3He,3He)108Pd

B.V. Kheswa et al., Phys. Lett. B744, 268 (2015): (3He,4He)138La
B.V. Kheswa et al., Phys. Lett. B744, 268 (2015): (3He,3He)139La

A. Spyrou et al., Phys. Rev. Lett. 113, 232502 (2014): beta-76Ge_withGHK
A. Spyrou et al., Phys. Rev. Lett. 113, 232502 (2014): beta-76Ge_withEB

T.G.Tornyi et al., Phys. Rev. C89, 044323 (2014): (d,p)238Np

A. Simon et al., Phys. Rev. C93,034303 (2016): (p,d)151Sm
A. Simon et al., Phys. Rev. C93,034303 (2016): (p,d)153Sm

A.C. Larsen et al., Phys. Rev. C93, 045810 (2016), low: (p,p)89Y
A.C. Larsen et al., Phys. Rev. C93, 045810 (2016), middle: (p,p)89Y
A.C. Larsen et al., Phys. Rev. C93, 045810 (2016), high: (p,p)89Y

G.M. Tveten  et al., Phys. Rev. C94, 025804 (2016), low: (p,p)92Mo
G.M. Tveten  et al., Phys. Rev. C94, 025804 (2016), rec: (p,p)92Mo
G.M. Tveten  et al., Phys. Rev. C94, 025804 (2016), high: (p,p)92Mo

T.A.Laplace et al., Phys. Rev. C93, 014323 (2016): (d,p)243Pu

S. Bassauer et al. , Phys. Rev. C94, 054313 (2016) (reanalyzed N.U.H. Syed et al., Phys. Rev. C79, 024316 (2009)): (3He,3He)208Pb

M. Guttormsen et al., Phys. Rev. C96, 024313 (2017): (d,p)91ZrCT
M. Guttormsen et al., Phys. Rev. C96, 024313 (2017): (d,p)91ZrHFB
M. Guttormsen et al., Phys. Rev. C96, 024313 (2017): (p,p)92ZrCT
M. Guttormsen et al., Phys. Rev. C96, 024313 (2017): (p,p)92ZrHFB

A.C.Larsen et al., J. Phys. G: Nucl. Part. Phys. 44, 064005 (2017): (p,p)56Fe_NaI_FG05
A.C.Larsen et al., J. Phys. G: Nucl. Part. Phys. 44, 064005 (2017): (p,p)56Fe_LaBr_FG09​​​​
A.C.Larsen et al., J. Phys. G: Nucl. Part. Phys. 44, 064005 (2017): (p,p)57Fe_NaI_FG05
A.C.Larsen et al., J. Phys. G: Nucl. Part. Phys. 44, 064005 (2017): (p,p)57Fe_LaBr_FG09

F. Giacoppo et al., Phys. Rev. C90, 054330 (2014): (p,d)194Pt
F. Giacoppo et al., Phys. Rev. C90, 054330 (2014): (d,d)195Pt
F. Giacoppo et al., Phys. Rev. C90, 054330 (2014): (p,p)195Pt
F. Giacoppo et al., Phys. Rev. C90, 054330 (2014): (d,p)196Pt
F. Giacoppo et al., Phys. Rev. C90, 054330 (2014): (3he,3he)197Au
F. Giacoppo et al., Phys. Rev. C90, 054330 (2014): (d,d)197Au
F. Giacoppo et al., Phys. Rev. C90, 054330 (2014): (d,p)198Au

T. Renstrøm et al., Phys. Rev. C93, 064302 (2016), (3he,3he)74Ge: HFB, lower, rec, upper
T. Renstrøm et al., Phys. Rev. C93, 064302 (2016), (3he,4he)73Ge: HFB, lower, rec

T. Renstrøm et al., Phys. Rev. C98, 054310 (2018): (3he,4he)160Dy  (3he,3he)161Dy    (3he,4he)161Dy  (3he,3he)162Dy   (3he,4he)Dy162  (3he,4he)163Dy (3he,3he)164Dy  

M.Guttormsen et al., Phys. Lett. B816, 136206 (2021): (p,p)142Nd  (p,p)144Nd  (d,p)145Nd (p,p)146Nd  (d,p)147Nd  (p,p)148Nd  (d,p)149Nd  (p,p)150Nd  (d,p)151Nd
 
M.Markova et al., PRL 127, 182501 (2021): renormalised (3he,4he)116Sn
M.Markova et al., PRC 106, 034322 (2022): (p,p)120Sn (p,p)124Sn
 
F. Pogliano et al., Phys. Rev. C106, 015804 (2022): (alpha,p)127Sb
F. Pogliano et al., Phys. Rev. C107, 034605 (2023): (alpha,p)166Ho
F. Pogliano et al., Phys. Rev. C107, 064614 (2023): (alpha,p)167Ho

M. Markova et al., arXiv:2311.08864v1 (2023):  112Sn(p,d)111Sn 112Sn(p,p)112Sn 112Sn(d,p)113Sn 117Sn(3he,4he)116Sn 117Sn(p,p)117Sn 119Sn(3he,4he)118Sn 119Sn(p,p)119Sn 120Sn(p,p)120Sn 122Sn(3he,4he)121Sn 122Sn(3he,3he)122Sn 124Sn(p,p)124Sn

Gamma-ray strength functions (Oslo method)

You may download pdf figures for some of these data here:
SmDyErYb, Dy, Yb, Mo, Fe, 50V, 51V, new 96Mo, Sc, new 56,57Fe

A. Voinov et al., Phys. Rev. C63, 044313 (2001): (3He,4He)161Dy
A. Voinov et al., Phys. Rev. C63, 044313 (2001): (3He,4He)162Dy

E. Melby et al., Phys. Rev. C63, 044309 (2001): (3He,4He)166Er
E. Melby et al., Phys. Rev. C63, 044309 (2001): (3He,3He)167Er

A. Voinov et al., Phys. Rev. C63, 044313 (2001): (3He,4He)171Yb
A. Voinov et al., Phys. Rev. C63, 044313 (2001): (3He,4He)172Yb

S. Siem et al., Phys. Rev. C65, 044318 (2002): (3He,4He)148Sm
S. Siem et al., Phys. Rev. C65, 044318 (2002): (3He,3He)149Sm

M. Guttormsen et al., Phys. Rev. C68, 064306 (2003): (3He,4He)160Dy
M. Guttormsen et al., Phys. Rev. C68, 064306 (2003): (3He,3He)161Dy
M. Guttormsen et al., Phys. Rev. C68, 064306 (2003): (3He,4He)161Dy
M. Guttormsen et al., Phys. Rev. C68, 064306 (2003): (3He,3He)162Dy
M. Guttormsen et al., Phys. Rev. C68, 064306 (2003): (3He,4He)162Dy

U. Agvaanluvsan et al., Phys. Rev. C70, 054611 (2004): (3He,4He)170Yb
U. Agvaanluvsan et al., Phys. Rev. C70, 054611 (2004): (3He,3He)171Yb
U. Agvaanluvsan et al., Phys. Rev. C70, 054611 (2004): (3He,4He)171Yb
U. Agvaanluvsan et al., Phys. Rev. C70, 054611 (2004): (3He,3He)172Yb
U. Agvaanluvsan et al., Phys. Rev. C70, 054611 (2004): (3He,4He)172Yb

A. Voinov et al., Phys. Rev. Lett. 93, 142504 (2004): (3He,4He)56Fe
A. Voinov et al., Phys. Rev. Lett. 93, 142504 (2004): (3He,3He)57Fe

M. Guttormsen et al., Phys. Rev. C71, 044307 (2005): (3He,4He)93Mo
M. Guttormsen et al., Phys. Rev. C71, 044307 (2005): (3He,3He)94Mo
M. Guttormsen et al., Phys. Rev. C71, 044307 (2005): (3He,4He)95Mo
M. Guttormsen et al., Phys. Rev. C71, 044307 (2005): (3He,3He)96Mo
M. Guttormsen et al., Phys. Rev. C71, 044307 (2005): (3He,4He)96Mo
M. Guttormsen et al., Phys. Rev. C71, 044307 (2005): (3He,3He)97Mo
M. Guttormsen et al., Phys. Rev. C71, 044307 (2005): (3He,4He)97Mo
M. Guttormsen et al., Phys. Rev. C71, 044307 (2005): (3He,3He)98Mo

A.C. Larsen et al., Phys. Rev. C 73, 064301 (2006): (3He,4He)50V
A.C. Larsen et al., Phys. Rev. C 73, 064301 (2006): (3He,3He)51V

Reanalyzed 2008, M. Guttormsen et al., Phys. Rev. C71, 044307 (2005): (3He,3He)96Mo
Reanalyzed 2008, M. Guttormsen et al., Phys. Rev. C71, 044307 (2005): (3He,4He)96Mo

A.C. Larsen et al., Phys. Rev. C 76, 044303 (2007): (3He,4He)44Sc
A.C. Larsen et al., Phys. Rev. C 76, 044303 (2007): (3He,3He)45Sc

E. Algin et al., Phys. Rev. C 78, 054321 (2008): (3He,4He)56Fe
E. Algin et al., Phys. Rev. C 78, 054321 (2008): (3He,3He)57Fe

N.U.H. Syed et al., Phys. Rev. C79, 024316 (2009): (3He,4He)205Pb
N.U.H. Syed et al., Phys. Rev. C79, 024316 (2009): (3He,3He)206Pb
N.U.H. Syed et al., Phys. Rev. C79, 024316 (2009): (3He,4He)207Pb
N.U.H. Syed et al., Phys. Rev. C79, 024316 (2009): (3He,3He)208Pb

N.U.H. Syed et al., Phys. Rev. C80, 044309 (2009): (p,d)45Ti

H.T. Nyhus et al., Phys. Rev. C81, 024325 (2010): (3He,4He)163Dy
H.T. Nyhus et al., Phys. Rev. C81, 024325 (2010): (3He,3He)164Dy

H.K. Toft et al., Phys. Rev. C81, 064311 (2010): (3He,4He)116Sn
H.K. Toft et al., Phys. Rev. C81, 064311 (2010): (3He,3He)117Sn
H.K. Toft et al., Phys. Rev. C81, 064311 (2010): (3He,4He)118Sn
H.K. Toft et al., Phys. Rev. C81, 064311 (2010): (3He,3He)119Sn

M. Guttormsen et al., Phys. Rev. C83, 014312 (2011): (p,p)46Ti

H.K. Toft et al., Phys. Rev. C83, 044320 (2011): (3He,4He)121Sn
H.K. Toft et al., Phys. Rev. C83, 044320 (2011): (3He,3He)122Sn

A. Bürger et al., Phys. Rev. C85, 064328(2012): (p,4He)43Sc

A.C. Larsen et al., Phys. Rev. C85, 014320 (2012), CT-norm.: (p,t)44Ti
A.C. Larsen et al., Phys. Rev. C85, 014320 (2012), GHK-norm.: (p,t)44Ti
 
Normalisation with E&B 2005 (see paper):

A.C. Larsen et al., Phys. Rev. C87, 014319 (2013): (3He,4He)105Cd
A.C. Larsen et al., Phys. Rev. C87, 014319 (2013): (3He,3He)106Cd
A.C. Larsen et al., Phys. Rev. C87, 014319 (2013): (3He,4He)111Cd
A.C. Larsen et al., Phys. Rev. C87, 014319 (2013): (3He,3He)112Cd

A.C. Larsen et al., Phys. Rev. Lett. 111, 242504 (2013): (p,p)56Fe with NaI
A.C. Larsen et al., Phys. Rev. Lett. 111, 242504 (2013): (p,p)56Fe with LaBr
 
M.Guttormsen et al., Phys. Rev. C89, 014302 (2014): (3He,a)231Th
M.Guttormsen et al., Phys. Rev. C89, 014302 (2014): (d,d)232Th
M.Guttormsen et al., Phys. Rev. C89, 014302 (2014): (3He,3He)232Th
M.Guttormsen et al., Phys. Rev. C89, 014302 (2014): (d,p)233Th
M.Guttormsen et al., Phys. Rev. C89, 014302 (2014): (3He,t)232Pa
M.Guttormsen et al., Phys. Rev. C89, 014302 (2014): (3He,d)233Pa
M.Guttormsen et al., Phys. Rev. C89, 014302 (2014): (d,t)237U
M.Guttormsen et al., Phys. Rev. C89, 014302 (2014): (d,d)238U
M.Guttormsen et al., Phys. Rev. C89, 014302 (2014): (d,p)239U

H. Utsunomiya et al., Phys. Rev. C88, 015805 (2013): (3He,3He)94Mo
H. Utsunomiya et al., Phys. Rev. C88, 015805 (2013): (3He,4He)95Mo
H. Utsunomiya et al., Phys. Rev. C88, 015805 (2013): (3He,3He)96Mo
H. Utsunomiya et al., Phys. Rev. C88, 015805 (2013): (3He,3He)97Mo
H. Utsunomiya et al., Phys. Rev. C88, 015805 (2013): (3He,3He)98Mo

T.K. Eriksen et al., Phys. Rev. C90, 044311 (2014): (3He,4He)105Pd
T.K. Eriksen et al., Phys. Rev. C90, 044311 (2014): (3He,3He)106Pd
T.K. Eriksen et al., Phys. Rev. C90, 044311 (2014): (3He,4He)107Pd
T.K. Eriksen et al., Phys. Rev. C90, 044311 (2014): (3He,3He)108Pd

B.V. Kheswa et al., Phys. Lett. B744, 268 (2015): (3He,4He)138La
B.V. Kheswa et al., Phys. Lett. B744, 268 (2015): (3He,3He)139La

A. Spyrou et al., Phys. Rev. Lett. 113, 232502 (2014): beta-76Ge_withGHK
A. Spyrou et al., Phys. Rev. Lett. 113, 232502 (2014): beta-76Ge_withEB

T.G.Tornyi et al., Phys. Rev. C89, 044323 (2014): (d,p)238Np

A. Simon et al., Phys. Rev. C93,034303 (2016): (p,d)151Sm
A. Simon et al., Phys. Rev. C93,034303 (2016): (p,d)153Sm

A.C. Larsen et al., Phys. Rev. C93, 045810 (2016), low: (p,p)89Y
A.C. Larsen et al., Phys. Rev. C93, 045810 (2016), middle: (p,p)89Y
A.C. Larsen et al., Phys. Rev. C93, 045810 (2016), high: (p,p)89Y

G.M. Tveten  et al., Phys. Rev. C94, 025804 (2016), low: (p,p)92Mo
G.M. Tveten  et al., Phys. Rev. C94, 025804 (2016), rec: (p,p)92Mo
G.M. Tveten  et al., Phys. Rev. C94, 025804 (2016), high: (p,p)92Mo

T.A.Laplace et al., Phys. Rev. C93, 014323 (2016): (d,p)243Pu

S. Bassauer et al. , Phys. Rev. C94, 054313 (2016) (reanalyzed N.U.H. Syed et al., Phys. Rev. C79, 024316 (2009)): (3He,3He)208Pb
 
M.Guttormsen et al., Phys. Rev. C96, 024313 (2017), low: (d,p)91Zr
M.Guttormsen et al., Phys. Rev. C96, 024313 (2017), rec: (d,p)91Zr
M.Guttormsen et al., Phys. Rev. C96, 024313 (2017), high: (d,p)91Zr
M.Guttormsen et al., Phys. Rev. C96, 024313 (2017), low: (p,p)92Zr
M.Guttormsen et al., Phys. Rev. C96, 024313 (2017), rec: (p,p)92Zr
M.Guttormsen et al., Phys. Rev. C96, 024313 (2017), high: (p,p)92Zr
 
A.C.Larsen et al., J. Phys. G: Nucl. Part. Phys. 44, 064005 (2017): (p,p)56Fe_NaI_FG05​​​​​​
A.C.Larsen et al., J. Phys. G: Nucl. Part. Phys. 44, 064005 (2017): (p,p)56Fe_LaBr_FG09​​​​
A.C.Larsen et al., J. Phys. G: Nucl. Part. Phys. 44, 064005 (2017): (p,p)57Fe_NaI_FG05
A.C.Larsen et al., J. Phys. G: Nucl. Part. Phys. 44, 064005 (2017): (p,p)57Fe_LaBr_FG09
 
F. Giacoppo et al., Phys. Rev. C91, 054327 (2015):  (3He,3He)197Au
F. Giacoppo et al., Phys. Rev. C91, 054327 (2015):  (d,p)198Au
 
T. Renstrøm et al., Phys. Rev. C93,064302 (2016), (3he,3he)74Ge: lower, rec, upper
T. Renstrøm et al., Phys. Rev. C93,064302 (2016), (3he,4he)73Ge: lower, rec
 
L. Crespo Campo et al., Phys. Rev.94, 044321 (2016):  (p,p)64Ni
 
T. Renstrøm et al., Phys. Rev. C98, 054310 (2018): (3he,4he)160Dy  (3he,3he)161Dy    (3he,4he)161Dy  (3he,3he)162Dy   (3he,4he)Dy162  (3he,4he)163Dy (3he,3he)164Dy  
 
M.Guttormsen et al., Phys. Rev. C106, 034314 (2022): (p,p)142Nd  (p,p)144Nd  (d,p)145Nd (p,p)146Nd  (d,p)147Nd  (p,p)148Nd  (d,p)149Nd  (p,p)150Nd  (d,p)151Nd
 
M.Markova et al., PRL 127, 182501 (2021): renormalised (3he,4he)116Sn
M.Markova et al., PRC 106, 034322 (2022): (p,p)120Sn (p,p)124Sn
 
F. Pogliano et al., Phys. Rev. C106, 015804 (2022): (alpha,p)127Sb
F. Pogliano et al., Phys. Rev. C107, 034605 (2023): (alpha,p)166Ho
F. Pogliano et al., Phys. Rev. C107, 064614 (2023): (alpha,p)167Ho
 

Gamma-ray strength functions (Shape method)

The shape method was published in 2021 by M.Wiedeking et al., Phys. Rev. C104, 014311 (2021). It is based on measuring the intensities (counts) of direct gamma-feeding to final excitation energy state(s) at a certain E_f. These counts are to be localised at a diagonal in the Oslo matrix P(E,E_g) for E = E_f = E_g . With two well-defined diagonals (D1 and D2) in the matrix, it is possible to sew together the g-ray strength function f(E_g). The slope of f(E_g) can then be extracted, but the scaling is unknown and has to be normalised to other data.

M. Wiedeking et al., Phys. Rev. C104, 014311 (2021):  (p,p)56Fe  (p,p)92Zr( D1D2 D1D3 D1D4 D2D3 D2D4 D3D4)   (3he,3he)164Dy

M. Guttormsen et al., Phys. Rev. C106, 034314 (2022):  (p,p)144Nd  (d,p)145Nd  (p,p)150Nd

S. Goriely et al., Phys. Rev. C106, 044315 (2022): (3he,3he')112Cd (ShapeIt, Diablo

M. Markova et al., arXiv:2311.08864v1 (2023):  (p,p)120Sn  (p,p)124Sn

Published Apr. 29, 2011 11:47 AM - Last modified Dec. 8, 2023 5:14 PM