1 gaskelld 1.1 From Omar.Benhar@roma1.infn.it Fri Jun 1 11:03:18 2001
2 Date: Fri, 1 Jun 2001 13:35:36 +0200 (MET DST)
3 From: "Omar Benhar - INFN, Roma - ++39-06-49914298"
4 <Omar.Benhar@roma1.infn.it>
5 To: John R. Arrington <johna@cedar.phy.anl.gov>
6 Cc: Omar Benhar <benhar@roma1.infn.it>
7
8 John:
9
10 the tabulated 4He spectral function that I sent a while ago looks
11 allright to me.
12 The spectral function consists of two contributions: the two body
13 breakup contribution, whose energy dependence is a delta-function, and the
14 background, giving rise to a continuum starting at the three-body breakup
15 threshold.
16 The first bin in the table is indeed 1 MeV wide. It represents the
17 delta-function contribution. The following bins, starting at 28.2 MeV,
18 give the background.
19 I have also checked that the normalization is correct to fractions of
20 a percent.
21
22 gaskelld 1.1 Attached are the files with the A=3 spectral functions, whose structure
23 is explained below.
24
25 Best
26 Omar
27
28
29 *******************************************************************************
30
31 The files are organized as follows
32
33 *** 3He: Paris potential, Faddeev calculations of the Hannover
34 group (see H. Meier-Hajduk, Ch. Hajduk, P.U. Sauer and W. Theis,
35 Nucl. Phys. A395(1983)332). file 'spec3he_paris.data' ***
36
37 - the first line gives the number of momentum and energy bins (65 and 15,
38 respectively)
39
40 - the central values of momentum bins (MeV) are given in lines 2-66 (GeV)
41
42 - lines 67-81 give central values and size of the energy bins (GeV)
43 gaskelld 1.1
44 - then follow 15 blocks of 34 lines each, giving the proton and neutron spectral
45 functions as a function of momentum for each energy. The first 17 lines give the
46 proton spectral function, while the next 17 lines give the neutron spectral
47 function. For example, lines 82 iand 99 gives the proton and neutron spectral
48 functions corresponding to the first energy bin and the first four momentum bins,
49 respectively.
50
51 - the spectral functions are given in units of GeV^-4
52
53 - the normalizations of the proton and neutron spectral functions are
54
55 4 \pi \int dE dk k^2*P_p(k,E) = 1
56
57 4 \pi \int dE dk k^2*P_n(k,E) = 1
58
59
60 *** 3He: Argonne v_14 + Urbana VII three-body force. Calculation carried
61 out using the model described in O. Benhar and V.R. Pandharipande, Phys. Rev.
62 C 47(1993)2218. file 'spec3he_mod.dat' ***
63
64 gaskelld 1.1 - the file is organized in exactly the same way as that containing the Hannover
65 spectral function. The only difference is that the proton and neutron spectral
66 functions are normalized according to
67
68 4 \pi \int dE dk k^2*P_p(k,E) = 2
69
70 4 \pi \int dE dk k^2*P_n(k,E) = 1
71
72 ********************************************************************************
73
74 ++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
75 Omar Benhar phone ++39-06-49914298
76 INFN, Sezione Roma 1 fax ++39-06-4454749
77 Piazzale Aldo Moro, 2 e-mail benhar@roma1.infn.it
78 I-00185 Rome, Italy
79 ++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
80
81 [ Part 2, "" Text/PLAIN (Name: "spec3he_paris.data") 703 lines. ]
82 [ Unable to print this part. ]
83
84
85 gaskelld 1.1 [ Part 3, "" Text/PLAIN (Name: "spec3he_mod.dat") 1,247 lines. ]
86 [ Unable to print this part. ]
87
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