One of the challenges of the modern physics
is the description of the internal structure
of the baryons and mesons.
The electromagnetic structure
of the nucleon and the nucleon resonances can be accessed
through the reactions,
which deppend of the (photon) transfer momentum squared [1--4].
The data associated with those transitions
are represented in terms of helicity amplitudes and have been collected in the recent years at Jefferson Lab, with increasing .
The new data demands the development of theoretical models
based in the underlying structure
of quarks and mesons states [3,4].
Those models can be also very useful
to predict the results of the future
Jlab--12 GeV upgrade, particularly
for resonances in the second and third resonance region
(energy -- GeV) [4].
In that region there are several resonances
from the supermultiplet of ,
characterized by a negative parity [5].
According with the single quark transition model,
when the electromagnetic interaction
is the result of the photon coupling with just one quark,
the helicity amplitudes of the members
depend only of three independent functions of :
and [5,6].
In this work we use the
covariant spectator quark model [4,6,7]
developed for the
and transitions [8],
also members of ,
to calculate those functions.
With the knowledge of the functions , and
we predict the helicity amplitudes for the
transitions , ,
,
and [6].
To facilitate the comparison with
future experimental data at high ,
we provide also simple parametrizations
of the amplitudes and
for the different transitions, compatible with the expected
falloff at high [6].
[1] I.G. Aznauryan et al. [CLAS Collaboration],
Phys. Rev. C 80, 055203 (2009);
V.I. Mokeev et al. [CLAS Collaboration],
Phys. Rev. C 86, 035203 (2012).
[2] L. Tiator, D. Drechsel, S.S. Kamalov and M.Vanderhaeghen,
Eur. Phys. J. ST 198, 141 (2011).
[3] I.G. Aznauryan and V.D. Burkert,
Prog. Part. Nucl. Phys. 67, 1 (2012).
[4] I.G. Aznauryan et al.
Int. J. Mod. Phys. E 22, 1330015 (2013).
[5] V. D. Burkert, R. De Vita, M. Battaglieri, M. Ripani and V. Mokeev,
Phys. Rev. C 67, 035204 (2003).
[6] G. Ramalho,
Phys. Rev. D 90, 033010 (2014).
[7] F. Gross, G. Ramalho and M.T.~Peña,
Phys. Rev. C 77, 015202 (2008);
Phys. Rev. D 85, 093005 (2012).
[8] G. Ramalho and M.T. Peña,
Phys. Rev. D 89, 094016 (2014);
Phys. Rev. D 84, 033007 (2011);
G. Ramalho and K. Tsushima,
Phys. Rev. D 84, 051301 (2011).