Analysis of $\gamma\gamma\to ZH$ within the CSM concept
Fernand M. Renard

TL;DR
This paper investigates how Higgs and top quark compositeness within the CSM framework affect the amplitudes and cross sections of gamma-gamma to ZH processes, emphasizing the role of photon polarization in distinguishing different compositeness scenarios.
Contribution
It introduces a detailed analysis of polarization effects in gamma-gamma collisions to identify signatures of Higgs and top quark compositeness within the CSM model.
Findings
Polarized photon collisions reveal large differences between CSM conserving and violating scenarios.
Modifications in amplitudes and cross sections depend on the compositeness nature.
Photon polarization is crucial for identifying the origin of observable differences.
Abstract
We study the modifications of the amplitudes and cross sections generated by Higgs and top quark compositeness in particular within the CSM concept. We insist on the particular interest of polarized photon-photon collisions which should allow to identify the origin of the large observable differences between various, CSM conserving or CSM violating, compositeness possibilities.
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Taxonomy
TopicsTraditional Chinese Medicine Studies
March 14, 2017
Analysis of within the CSM concept.
F.M. Renard
Laboratoire Univers et Particules de Montpellier, UMR 5299
Université Montpellier II, Place Eugène Bataillon CC072
F-34095 Montpellier Cedex 5, France.
Abstract
We study the modifications of the amplitudes and cross sections generated by Higgs and top quark compositeness in particular within the CSM concept. We insist on the particular interest of polarized photon-photon collisions which should allow to identify the origin of the large observable differences between various, CSM conserving or CSM violating, compositeness possibilities.
PACS numbers: 12.15.-y, 12.60.-i, 14.80.-j; Composite models
1 INTRODUCTION
In previous papers we have studied the effect of Higgs boson and top quark compositeness on production in gluon-gluon collision, [1], [2]. We have introduced the concept of Composite Standard Model (CSM) which should preserve the structure and the main properties of the Standard Model (SM), at least at low energy. No anomalous coupling modifying the SM structures should be present, but form factors (for example due to substructures) would affect the Higgs boson and top quark couplings at high energy. We had not based our analyzes on a specific compositeness model, for example one of those mentioned in ref. [3, 4, 5, 6, 7, 8], but on the dependence of the observables on form factor effects.
We had noticed that the process is particularly sensitive to the presence of form factors, because they could destroy a peculiar SM cancellation between diagrams involving Higgs boson and top quark couplings. But we had also shown that this cancellation can be recovered provided that a special relation between form factors is satisfied. We considered this relation as a specific CSM property.
This process is therefore very interesting for revealing a violation of the SM prediction but an amplitude analysis confirming the origin of such an effect seems difficult to do in hadronic collisions.
This is why, in the present paper, we make an analysis of , the similar process appearing in photon-photon collisions.
The possibility of high energy photon-photon collisions has been considered since a long time, [9]; for a recent review see [10].
Its very interesting feature for our purpose is the possibility of working with polarized beams; this would allow to make an amplitude analysis and to check what happens with the above mentioned cancellation.
This will be essential for choosing among the various compositeness possibilities, for example either with only or with both and compositeness, and with or without the CSM constraint relating it to Higgs compositeness.
Contents: In Section 2 we recall the definitions and the SM properties of the amplitudes and observables of the process with polarized beams. In Section 3 we define the form factors, with or without the CSM constraint, that would affect the amplitudes. Illustrations showing their effect on the observables are given in Section 4, and the conclusion and outlook in Section 5.
2 AMPLITUDES AND OBSERVABLES OF THE PROCESS
At one loop order the SM amplitudes of the process arise from the charged fermion (leptons and quarks) loop diagrams depicted in Fig.1; triangle diagrams (a),(b) and box diagrams (c), (with gluon-gluon symmetrization); see [11] and older references therein.
With CP conservation and Bose statistics the helicity amplitudes for helicities and satisfy the following relations
[TABLE]
[TABLE]
[TABLE]
The polarized cross section has the following structure
[TABLE]
where , and describe respectively the average helicities, transverse polarizations and azimuthal angles of the two photons with their density matrices
[TABLE]
Using the above CP conservation relations the -quantities in (4) are defined as
[TABLE]
[TABLE]
[TABLE]
[TABLE]
[TABLE]
[TABLE]
[TABLE]
[TABLE]
with
[TABLE]
Note that , , and are symmetric under the interchange
[TABLE]
whereas
[TABLE]
As in the case the leading contributions come from top quark loops in (a) and (c) whereas the (b) contribution is much smaller. This smallness arises from the mass suppressed coupling appearing in (b) as compared to the one in (a) which has in addition the () enhancement due to the coupling.
The triangle diagrams (a) and (b) only contribute to the amplitudes whereas the boxes (c) contribute to all amplitudes.
The real and imaginary parts of the resulting SM amplitudes are shown in Fig.2a,b.
One can see that the helicity concerving (HC) amplitudes finally dominate over the helicity violating (HV) ones at high energy in agreement with the HC rule [12].
The remarkable cancellation between contributions of diagrams (a) and (c) is illustrated in Fig.3a,b.
The energy and angular dependences of the various elements of the polarized cross section are shown in Fig.4-5. As in the case the rate of longitudinal Z production is always very large, apart from local energy and angular fluctuations. We only illustrate its shapes for when looking at the form factor effects in Fig.8a,b.
All these behaviours are globally similar to those of the process. Only small differences appear at low energy where the effect of light lepton and quark loops is not totally negligible.
3 CSM CONSTRAINTS
Let us first recall the procedure used in [2] for introducing this CSM concept in the previous analysis of the process.
We affect form factors to each coupling appearing in the one loop diagrams of this process (see Fig.1) and involving an Higgs boson and/or a top quark. This means five arbitrary form factors chosen as .
Incidently we note that photon- form factors (similarly to gluon- form factors) may also appear, but as they would occur exactly in the same way in the triangles and in the boxes, they would not affect the structures of the amplitudes (in particular the special cancellation mentioned in the previous section); they would only modify the total result by a pure normalization factor. So we do not discuss them more.
With the five arbitrary form factors listed above large effects are in general observed due to the destruction of the cancellation appearing for the amplitude between its contribution from triangle (a) and the one from boxes (c) (see Fig.8 of [2]). But this cancellation can be recovered provided that the following CSM constraint is satisfied:
[TABLE]
We now look at the process and the effect of such form factors, with and without the CSM constraint, on the observables defined in the previous section.
For the illustrations, as simple examples, we will use simple ”test” expressions of the type
[TABLE]
with the new physics scale taken for example with the value of 5 TeV.
We use this expression for different form factors and we treat separately the following cases:
The two CSM conserving cases will be
— (a) denoted CSMtLR, refering to both and compositeness, with , and satisfying (15),
— (b) denoted CSMtR, for pure compositeness, and , and, in order to satisfy (15), either
and
or
and ,
and the 2 CSM violating cases:
— (c) denoted CSMvt, where with TeV, with TeV and with TeV,
— (d) denoted CSMvH, no top form factor and only one form factor affecting the and vertices.
In the next Section and Figures 6-8, we illustrate the consequences of such choices for the observables.
4 ILLUSTRATIONS
Fig.6a-f and 7a-f respectively illustrate the effects of the choices (a-d) of form factors on the energy and angular dependences of the cross sections corresponding to the unpolarized or to specific polarization cases. Fig.8a,b illustrate similarly the behaviour of the rate in the cross section.
As in the gluon-gluon case we can first check that the unpolarized cross section is very sensitive to the CSM violation cases CSMvt and CSMvH. The corresponding rates tend also to be closer to 1 at high energy.
Similar effects can be seen in the longitudinal polarization term .
The transverse polarization terms (related to ) and are also very sensitive with spectacular changes of signs.
On the opposite the double transverse term, only controlled by HC amplitudes, is not affected by the CSMvH case, but gets some effects in the other cases.
The mixed longitudinal and transverse term (related to ) involving both HV and HC amplitudes get also notably modified by the CSM violating terms.
Globally the CSM conserving terms lead to weaker effects in these various cross section elements.
Quantitatively the above effects obviously depend on the precise expression used for the ”test” form factor and on the value of ; our simple choice has no physical meaning but was only chosen in order to show the sensitivity of each observable.
Note also that the CSM violating cases producing large differences with the pure SM prediction due to the destruction of the special cancellation in amplitudes could nevertheless satisfy unitarity owing to the decrease of the form factors above the new physics scale (chosen at 5 TeV in the illustrations).
5 CONCLUSIONS
We have shown that the process, especially with polarized photon beams, should be particularly interesting for analyzing a possible departure from SM predictions with the aim of testing the CSM concept.
Indeed the observables of the process with photon polarizations and the associated dependences should allow to make an amplitude analysis and to identify the form factor structure, CSM conserving or CSM violating.
As in the case, the biggest effect should be found in the amplitude whose internal cancellation property is preserved or violated by the corresponding form factors.
We have illustrated with a simple ”test” shape how the various observables react to the presence of a form factor in the involved couplings.
We can conclude, in the case a departure from SM prediction would be observed in , that the process would be very fruitful for revealing the nature of a possible compositeness interpretation.
Along this line of thought further works could be carried with phenomenological analyzes of other processes sensitive to such compositeness effects, with or without CSM constraint; see for example and ref.[14]. Independently, possible theoretical studies could be done about the meaning of the CSM concept.
The reference list from the paper itself. Each links out to its DOI / PubMed record.
- 1[1] F.M. Renard, ar Xiv: 1701.04571.
- 2[2] F.M. Renard, ar Xiv: 1701.09116, 1702.08853.
- 3[3] G. Panico and A. Wulzer, Lect.Notes Phys. 913 ,1(2016).
- 4[4] H. Terazawa, Y. Chikashige and K. Akama, Phys. Rev. 𝐃𝟏𝟓 𝐃𝟏𝟓 {\bf{D 15}} , 480 (1977); for other references see H. Terazawa and M. Yasue, Nonlin.Phenom.Complex Syst. 19 ,1(2016); J. Mod. Phys. 𝟓 5 {\bf{5}} , 205 (2014).
- 5[5] D.B. Kaplan and H. Georgi, Phys. Lett. 𝟏𝟑𝟔 𝐁 136 𝐁 {\bf{136B}} , 183 (1984).
- 6[6] K. Agashe, R. Contino and A. Pomarol, Nucl. Phys. 𝐁𝟕𝟏𝟗 𝐁𝟕𝟏𝟗 {\bf{B 719}} , 165 (2005); hep/ph 0412089.
- 7[7] R. Contino, T. Kramer, M. Son and R. Sundrum, J. High Energy Physics 05 (2007)074.
- 8[8] G. Panico and A. Wulzer, Lect.Notes Phys. 913 ,1(2016).
