Observation of a charged (DD*bar)- mass peak in e+e- --> pi+ (DD*bar)- at Ecm=4.26 GeV

We use a second-order QED calculation and unpublished BESIII energy-dependent measurements of σ ⁡ ( e + ​ e − → π ​ D ​ D ∗ ¯ ) \sigma(e^{+}e^{-}\rightarrow\pi D\bar{D^{*}}) to compute the radiative correction; see E. A. Kuraev and V. S. Fadin, Yad. Fiz. 41

Original

1985

Earlier work this paper cites.

D.J. Lange, Nucl. Istrum. and Methods Phys. Res., Sect. A 462

2001

Earlier work this paper cites.

S. Jadach, B.F.L. Ward, and Z. Was, Comput. Phys. Commun. 130

2001

Earlier work this paper cites.

S. Agostinelli et al

2003

Earlier work this paper cites.

See, for example, M.B. Voloshin and L.B. Okun, JETP Lett. 23

2004

Earlier work this paper cites.

B. Aubert et al

2005

Earlier work this paper cites.

C.Z. Yuan et al

2005

Earlier work this paper cites.

Q. He et al

2006

Earlier work this paper cites.

X.H. Mo et al

2006

Cited alongside, same era.

Z.Y. Deng, et al

2006

Cited alongside, same era.

T. Sjöstrand, S. Mrenna and P. Skands, JHEP 026

2006

Cited alongside, same era.

K.-F. Chen et al

2008

Cited alongside, same era.

R.G. Ping et al

2008

Cited alongside, same era.

G. Pakhlova et al

2009

Cited alongside, same era.

M. Ablikim et al

2010

Cited alongside, same era.

A.E. Bondar et al

Original

J. Beringer et al

2012

Later among the works it cites.

A. Bondar et al

2012

Later among the works it cites.

R. Faccini et al

2012

Later among the works it cites.

M. Ablikim et al

2012

Later among the works it cites.

M. Ablikim et al

2013

Closest in time.

Z.Q. Liu et al

2013

Closest in time.

Q. Wang, C. Hanhart and Q. Zhao, Phys. Rev. Lett. 111

2013

Closest in time.

N. Mahajan, arXiv:1304.1301 [hep-ph], M.B. Voloshin, Phys.Rev. D 87