[Clas_hadron] APS Meeting abstract

[Viktor Mokeev]

Dear Valery,

Previously, the N* region was frequently determined as W<2.0 GeV. However, the extension in the exclusive photoproduction analyses of the last decade increases the value for this limit.

D.G. Ireland, et al., Prog.Part.Nucl.Phys. 111 (2020) 103752e-Print: 1906.04228<https://arxiv.org/abs/1906.04228> [nucl-ex]


Another factor which defines this limit is imposed by the capabilities for the credible treatment of the rad correction effects.

Best Regards,
                            Victor

________________________________
From: Clas_hadron <clas_hadron-bounces at jlab.org> on behalf of Valery Kubarovsky <vpk at jlab.org>
Sent: Monday, January 4, 2021 2:06 PM
To: Nikolay Markov <markov at jlab.org>; CLAS Hadron <clas_hadron at jlab.org>; Bryan McKinnon <Bryan.McKinnon at glasgow.ac.uk>; Latifa Elouadrhiri <latifa at jlab.org>
Subject: Re: [Clas_hadron] APS Meeting abstract

Dear Nick,
Where is W<2.5 GeV limit coming from?
I am not sure that $\gamma_vpN^*$ is the commonly used.
Best,
Valery

________________________________
From: Clas_hadron <clas_hadron-bounces at jlab.org> on behalf of Nikolay Markov <markov at jlab.org>
Sent: Monday, January 4, 2021 13:15
To: CLAS Hadron <clas_hadron at jlab.org>; Bryan McKinnon <Bryan.McKinnon at glasgow.ac.uk>; Latifa Elouadrhiri <latifa at jlab.org>
Subject: [Clas_hadron] APS Meeting abstract

Dear all,
attached is my draft for a contributed talk during the upcoming APS meeting at the
E8 Mini-Symposium: Early Science Results from Jefferson Lab 12 GeV Program.
I will really appreciate your comments and suggestions.
Best regards, Nick.
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