We present the model published in [Mat17a]
concerning th beam asymmetry of η and η′ beam asymmetries.
We report here only the main features of the model.
The code can be downloaded in Resources section and simulated
in the Simulation section.
Denoting η and η′ quantities by bare and primed symbols respectively, the beam asymmetry is defined by
Σ(′)=dσ(′)⊥−dσ(′)∥dσ(′)⊥+dσ(′)∥,
with dσ⊥ and dσ∥ denoting the differential cross section
with a photon polarization parallel and perpendicular to the reaction plane.
Natural exchanges ρ,ω and ϕ contribute to dσ⊥ and
unnatural exchanges b,h and h′ contribute to dσ∥.
The other unnatural exchanges ρ2,ω2 and ϕ2 also contribute to dσ∥.
We separate the contribution from natural and unnatural exchanges
kN=dσ′⊥dσ⊥,kU=dσ′∥dσ∥.
and rewrite the ratio of η′ and η beam asymmetries as
Σ′Σ=1+1−Σ2Σ⋅kN−kU(1+Σ)kN+(1−Σ)kU,≡1+ϵ
We use the CGLN invariant amplitudes Ai defined in [Chew57a].
The scalar amplitudes Ai=∑V,A,EAVi+AAi+AEi receive contribution
from V=ρ,ω,ϕ, A=b,h,h′ and E=ρ2,ω2,ϕ2.
For the natural Regge poles V=ρ,ω,ϕ (with s expressed in GeV2):
A(′)V1(s,t)=tβ(′)V1(t)1−e−iπαV(t)sinπαV(t)sαV(t)−1A(′)V2(s,t)=(−1/t)A(′)V1(s,t)A(′)V4(s,t)=tβ(′)V4(t)1−e−iπαV(t)sinπαV(t)sαV(t)−1A(′)V3(s,t)=0
The factor t in A(′)V1 comes from the factorization of the Regge pole residues and conservation of angular momentum.
The unnatural exchange contribution are A=b,h,h′ and E=ρ2,ω2,ϕ2
A(′)A2(s,t)=β(′)A2(t)1−e−iπαA(t)sinπαA(t)sαA(t)−1A(′)A1(s,t)=A(′)A3(s,t)=A(′)A4(s,t)=0A(′)E3(s,t)=β(′)E2(t)1−e−iπαE(t)sinπαE(t)sαE(t)−1A(′)E1(s,t)=A(′)E2(s,t)=A(′)E4(s,t)=0
In this webpage we propose the following flexible parametrization for the residues and trajectories
(ommitting the index V,A,E)
β(′)i(t)=g(′)iγgiNebit(1−γi,1t)(1−γi,2t)α(t)=α0+α1t
The observables are expressed with the scalar amplitudes (K is an irrelevant kinematical factor):
dσ(′)⊥(s,t)=K[|A(′)1|2−t|A(′)4|2],dσ(′)∥(s,t)=K[|A(′)1+tA(′)2|2−t|A(′)3|2]
so that the relevant quantities are
kN=|A′1|2−t|A′4|2|A1|2−t|A4|2,kU=|A′1+tA′2|2−t|A′3|2|A1+tA2|2−t|A3|2.
References
[Chew57a]
G.F. Chew, M.L. Goldberger, F.E. Low and Y. Nambu,
``Relativistic dispersion relation approach to photomeson production,''
Phys. Rev. 106, (1957) 1345.
[Mat17a]
V. Mathieu, J. Nys, C. Fernandez-Ramirez, A. Jackura, M. Mikhasenko, A. Pilloni, A. P. Szczepaniak and G. Fox (JPAC),
``On the η and η′ Photoproduction Beam Asymmetries,''
arXiv:1704.07684 [hep-ph],
Resources
- Publications: [Mat17a]
- C/C++: C/C++ file
- Input file: param.txt , EtaBA.txt .
- Output files: EtaP-BA.txt .
- Contact person: Vincent Mathieu
- Last update: May 2017
- param.txt:
The first line is the beam energy (in the lab frame) in GeV
The next 3x3 lines corresponds to the ρ,ω and ϕ exhchanges.
There are 3 lines for each exchange with the format:- gηγ gη′γ α0 α1
- g1 b1 g4 b4
- γ1,1 γ1,2 γ4,1 γ4,2
There are 2 lines for each exchanges with the format:- gηγ gη′γ α0 α1
- g2(3) b2(3) γ2(3),1 γ2(3),2
- EtaBA.txt: The data for γp→ηp t(GeV2)cosθdσdt(μb/GeV2)dσdΩ(μb)Σ The total cross sections σ(π±p) are in milli barns.
- EtaP-BA.txt: The results of the simulations in the format t(GeV2)Σ(η)kVkA104∗ϵΣ(η′)1+ϵ