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Formalismus in helicity and invariant amplitudes

4. Polarized nucleon Compton scattering 31

4.2. Polarization observables

4.2.2. Formalismus in helicity and invariant amplitudes

With the help of the T-matrix of Eq. (2.13) represented by the helicity amplitudes or of the relation between the amplitudes Hi and Ai of Eq. (D.1), one can get the observables in terms of the helicityHi or the invariantAi amplitudes.

4. Polarized nucleon Compton scattering

The c.m. unpolarized differential cross section d¯σ/dΩ reads then d¯σ As shown in Eq. (4.38) an unpolarized differential cross section is simply given as the sum of a squares of the individual helicity amplitude |Hi|2, and is then averaged over the four possible initial states. The |Hi|2 is not measurable directly because the polarizations in a final state are determined by the interaction between the particles.

Thus, it is allowed to measure only the different linear combinations of them, i.e dif-ferential cross sections or asymmetries. The explicite expressions of the single and double polarization observables are as follows:

dσ¯

4. Polarized nucleon Compton scattering

4. Polarized nucleon Compton scattering

As said, H3 = H4 = H5 = H6 = 0 at θ = 0 (t = 0) and H1 = H2 = H3 = H4 = 0 at θ = π(η = 0). In Eqs. (4.38)-(4.53), it is hence simply recognizable that all observables, excepting the c.m. unpolarized differential cross section, Σ1z and Σ2z, are equal to zero at these two extreme angles. Notice also that below the pion threshold (ω= 150 MeV) there are only three asymmetries, Σ3, Σ2x, and Σ2z, which are different from zero. Indeed, Σ2z is the only measurable quantity in this region of energy and at the anglesθ = 0 andπ. From

On the other hand, the cross section d¯σ/dΩ and the asymmetry Σ2z are also deter-mined by the amplitudes A3,4 and A6 at the angle θ = 0 and by the amplitudes A1,2

4. Polarized nucleon Compton scattering In order to investigate the sensitivity of the observables to the invariant amplitudes, we turn the strength of the each invariant amplitude Ai from 100% to 101% and illustrate the difference between the results by using the invariant amplitude with the unchanged strength and that obtained from the amplitudes Ai having increased strength in Fig. 4.1-4.6 by means of the solid (θ = 300), dashed (θ = 600), dot-ted (θ = 1200) and dashed-dotted lines (θ= 1500), respectively.

At the small angles (θ= 300 and 600) the maximum respone to a change of A3,4 and A6 is, as expected, shown in the asymmetry Σ2z. Furthermore, the effects of the am-plitudesA3 and A6 on Σ2z are most visible just above and below the pion threshold, i.e. ω '130 MeV as well as about ω ' 170 MeV. Since the sum of the A3 and A6 is connected with theα+β at the angleθ = 0, the measurment of the asymmetry Σ2z in this kinematical region could offer important information on the electromagnetic po-larizability. On the other hand, the influence of changing theA4 amplitude is seen not only for Σ2z at higher energies, but also for Σ1x at the large angleθ = 1200 and above the energy of the second resonance (ω '750 MeV). The sensitivity of the amplitudes A3 and A6 are generally observed in the low energy region and at the small angles in nearly all asymmetries. In the case of the unpolarized differential cross section, the dependence on the amplitudes A3,4 and A6 is specifically large at ω ' 320 MeV and around the energies ω '750 MeV, respectively.

At the large backward angles of θ = 1200 and 1500 the change of the strength of the amplitudes A2 and A5 has the largest influence on Σ2z at the energy ω ' 730 MeV.

This means that the measurment of the asymmetry Σ2z in this high energy region and at the larger angles is appropriate to get more knowledge on the proton backward spin polarizability γπp. In the case of the amplitude A1, the asymmetry Σ2z as well as Σ3 are sensitive to a change of the strength of this amplitude, in particular below the one-pion threshold and in the region of ∆-resonance, respectively. Among the three amplitudes A1, A2 and A5, the amplitude A1 affects mostly the unpolarizaed differential cross sectionsd¯σ/dΩ.

As a result, the experiment using the circularly polarized photon and the proton-target polarized inz direction is mostly adequate to determine the value of the polarizabili-ties.

4. Polarized nucleon Compton scattering

Deviations Θcm =30

o

Θcm =60o Θcm =120o Θcm =150o dσ/dΩ

Σy

Σ3 Σ3y

Σ2x

Σ1x

Eγ(MeV)

Σ2z

Eγ(MeV)

Σ1z -100

-50 0 50

-0.1 -0.05 0 0.05 0.1

-0.2 0 0.2

-0.2 0

-0.2 0

-0.1 0 0.1 0.2 0.3

-0.5 0

0 150 300 450 600 750 900 -0.2 -0.1 0

150 300 450 600 750 900

Figure 4.1.:The relative difference between the results for the observables of proton Compton scattering obtained from the invariant amplitude A3 with the unchanged strength and that obtained from the amplitudes A3 with the strength increased by 1% at four different angles θcm = 30o (solid lines), 60o (dashed lines), 120o (dotted lines) and 150o (dashed-dotted lines).

4. Polarized nucleon Compton scattering

Deviations Θcm =30oΘ

cm =60o Θcm =120o Θcm =150o dσ/dΩ

Σy

Σ3

Σ3y

Σ2x Σ1x

Eγ(MeV)

Σ2z

Eγ(MeV)

Σ1z -15

-10 -5 0

0 0.02

-0.02 -0.01 0 0.01

-0.04 -0.02 0 0.02 0.04

-0.04 -0.02 0 0.02 0.04

-0.025 0 0.025 0.05

-0.1 -0.05 0 0.05

0 150 300 450 600 750 900

-0.01 0 0.01 0.02

150 300 450 600 750 900

Figure 4.2.:The relative difference between the results for the observables of pro-ton Comppro-ton scattering obtained from the invariant amplitude A4 with the unchanged strength and that obtained from the amplitudes A4 with the strength increased by 1% at four different angles θcm = 30o, 60o 120o and 150o. The notations are the same as in Fig. 4.1.

4. Polarized nucleon Compton scattering

Deviations

Θcm =150o Θcm =120o Θcm =60o Θcm =30o dσ/dΩ

Σy

Σ3

Σ3y

Σ2x Σ1x

Eγ(MeV)

Σ2z

Eγ(MeV)

Σ1z -100

-50 0

-0.05 0 0.05

-0.2 0 0.2

-0.1 0 0.1

-0.1 0 0.1 0.2

-0.2 -0.1 0 0.1

-0.5 0 0.5

0 150 300 450 600 750 900

-0.1 0 0.1

150 300 450 600 750 900

Figure 4.3.:The relative difference between the results for the observables of pro-ton Comppro-ton scattering obtained from the invariant amplitude A6 with the unchanged strength and that obtained from the amplitudes A6 with the strength increased by 1% at four different angles θcm = 30o, 60o 120o and 150o. The notations are the same as in Fig. 4.1.

4. Polarized nucleon Compton scattering

Deviations

dσ/dΩ

Θcm =30o Θcm =60o Θcm =120o Θcm =150o

Σy

Σ3 Σ3y

Σ2x Σ1x

Eγ(MeV)

Σ2z

Eγ(MeV)

Σ1z -40

-30 -20 -10 0

-0.02 0 0.02

-0.05 -0.025 0 0.025 0.05

-0.02 0 0.02

-0.04 -0.02 0 0.02

-0.04 -0.02 0 0.02

-0.05 0 0.05

0 150 300 450 600 750 900

-0.01 0 0.01 0.02

150 300 450 600 750 900

Figure 4.4.:The relative difference between the results for the observables of pro-ton Comppro-ton scattering obtained from the invariant amplitude A1 with the unchanged strength and that obtained from the amplitudes A1 with the strength increased by 1% at four different angles θcm = 30o, 60o 120o and 150o. The notations are the same as in Fig. 4.1.

4. Polarized nucleon Compton scattering

150 300 450 600 750 900

Figure 4.5.:The relative difference between the results for the observables of pro-ton Comppro-ton scattering obtained from the invariant amplitude A2 with the unchanged strength and that obtained from the amplitudes A2 with the strength increased by 1% at four different angles θcm = 30o, 60o 120o and 150o. The notations are the same as in Fig. 4.1.

4. Polarized nucleon Compton scattering

150 300 450 600 750 900

Figure 4.6.:The relative difference between the results for the observables of pro-ton Comppro-ton scattering obtained from the invariant amplitude A5 with the unchanged strength and that obtained from the amplitudes A5 with the strength increased by 1% at four different angles θcm = 30o, 60o 120o and 150o. The notations are the same as in Fig. 4.1.

4. Polarized nucleon Compton scattering