Hello!
Thank You very much in advance!
My full postal mail address: Yakubovskogo str., 4, apt. 77 Kiev 03191 Ukraine
My full name: Oleksandr Okhrimenko
My place of birth and date of birth: Novhorod-Siverskyy, Ukraine, 03.03.1984
Just in case, My international passport number is EK939584, valid until 28.04.2020
Cheers, Sasha
On 06/07/2017 13:32, Mischke, A. (Andre) wrote:
Dear Sasha,
thanks for your email. Please send us the following information:
- your full postal mail address
- your full name
- your place of birth and date of birth
We will than send you the invitation letter as a pdf.
Best, Andre
============================================================== Dr. André Mischke Associate Professor, FYAE, MAE
Institute for Subatomic Physics Center for Extreme Matter and Emergent Phenomena Faculty of Science Utrecht UniversityRoom:Ornstein Laboratorium ONL 213A Princetonplein 1Phone: +31 (0)30 253 2330 3584 CC UtrechtEmail: a.mischke@uu.nl mailto:a.mischke@uu.nl the NetherlandsWebsite: http://amischke.home.cern.ch
On sabbatical from April-August 2017 at the School of Physics and Astronomy University of Birmingham Birmingham B15 2TT UK Phone: +44 121 414 4674 ==============================================================
On 6 Jul 2017, at 12:09, Sasha Okhrimenko <okhrimenko@kinr.kiev.ua mailto:okhrimenko@kinr.kiev.ua> wrote:
Dear Organizers!
My name is Oleksandr Okhrimenko.
Could You, please, send me by e-mail an copy of the invitation letter to manage documents for my business trip to SQM today. If it is not impossible to prepare invitation letter today, so, I think, e-mail with invitation to participate at SQM 2017 as well as information about accommodation and meals should be enough to begin documents preparation. But, invitation letter will be required later at institute as well as can be required in the border control.
Also, I hope that it is not a problem that I will come to conference in Tuesday (11.07) and will not participate in SQM school? due to lack of time I will not be able to prepare my trip early.
My personal information: Mr. Oleksandr Okhrimenko
Junior Scientific Researcher
Institute for Nuclear Research NAS of Ukraine
Prospekt Nauky, 47
Kiev 03680
Ukraine
Please, let me know if additional info is needed.
Many thanks in advance and for understanding!
And sorry for incontinence.
Cheers,
Sasha
On 06/07/2017 12:30, Igor Kostiuk wrote:
Dear Organizers,
I will unfortunately be unable to come to SQM2017. I would like to ask for my payment (190 Euro) to be transferred to Sasha Okrimenko who will present my talk. Forwarding the related correspondence. Thank you in advance and sorry for the inconvenience.
Sincerely, Igor Kostiuk
*From:* Marco Gersabeck *Sent:* 06 July 2017 11:47 *To:* valerii.pugach@gmail.com mailto:valerii.pugach@gmail.com *Cc:* Giacomo Graziani; Igor Kostiuk; Oleksandr Okhrimenko; Francesco Bossu *Subject:* Re: change of abstract
Dear Valerii, Sasha,
Yes, that’s OK. Apologies for the delayed response, but I was unwell the last few days (fine now). Please let me know if the organisers agree to the swap.
Best regards,
Marco
On 4 Jul 2017, at 14:29, Valerii Pugach <valerii.pugach@gmail.com mailto:valerii.pugach@gmail.com mailto:valerii.pugach@gmail.com> wrote:
Dear Marco,
May I ask you to confirm that the Speaker's Bureau agrees to change a speaker at SQM2017 (Sasha Okhrimenko instead of Igor Kostiuk) for presenting
" J/psi production in proton-lead collisions at 8 TeV with the LHCb detector"
Abstract: "We present new results on J/psi production in p-Pb collisions, using the data collected in 2016 by LHCb at 8 TeV nucleon-nucleon center-of-mass energy. The LHCb experiment has the unique property to study heavy-ion interactions in the forward region (pseudorapidity between 2 and 5) with a fully instrumented detector. Both forward and backward rapidities are covered thanks to the possibility of beam reversal. Cold Nuclear Matter (CNM) effects are probed through measurements of nuclear modification factors and forward-backward production of both prompt and displaced J/psi. With respect to the results based on the 5 TeV sample collected in 2013, an increase in luminosity by a factor 20, other than the larger charm production cross-section, allow a remarkable improvement of the experimental accuracy. Results are compared with theoretical predictions modeling different CNM effects."
Thank you in advance, Best wishes, Valery
Valery Pugatch High Energy Physics Department, Head Institute for Nuclear Research NASU Prospekt Nauki, 47 03680 Kiev
On Tue, Jul 4, 2017 at 3:18 PM, <Giacomo.Graziani@cern.ch mailto:Giacomo.Graziani@cern.ch mailto:Giacomo.Graziani@cern.ch> wrote:
Dear Valery, the abstract below has been already accepted by the organizaers. If also a change of speaker is needed, please be sure to agree this with the Speaker's Bureau (I added Marco in cc), other than the organizers. Best regards,
GiacomoOn Tue, 4 Jul 2017, Valerii Pugach wrote:
Dear Giacomo, Thank you very much for this positive for us arrangement. I have talked with Igor few minutes ago concerning the J/Psi talk at SQM2017. Igor is currently recovering from the illness, and, unfortunately, does not feel well for the forhcoming trip. We have agreed with Igor and Sasha that this talk might be presented by Sasha. We would appreciate if you agree too and negotiate the subject with the Organizers. With my best wishes, Valery Valery Pugatch High Energy Physics Department, Head Institute for Nuclear Research NASU Prospekt Nauki, 47 03680 Kiev On Mon, Jul 3, 2017 at 5:05 PM, <Giacomo.Graziani@cern.chmailto:Giacomo.Graziani@cern.ch mailto:Giacomo.Graziani@cern.ch> wrote:
Dear Igor, we confirm that the organizers are happy with the change of subject of your talk. The new abstract is below, please prepare your contribution on the new topic. Cheers, Francesco and Giacomo J/psi production in proton-lead collisions at 8 TeV with the LHCb detector We present new results on J/psi production in p-Pb collisions, using the data collected in 2016 by LHCb at 8 TeV nucleon-nucleon center-of-mass energy. The LHCb experiment has the unique property to study heavy-ion interactions in the forward region (pseudorapidity between 2 and 5) with a fully instrumented detector. Both forward and backward rapidities are covered thanks to the possibility of beam reversal. Cold Nuclear Matter (CNM) effects are probed through measurements of nuclear modification factors and forward-backward production of both prompt and displaced J/psi. With respect to the results based on the 5 TeV sample collected in 2013, an increase in luminosity by a factor 20, other than the larger charm production cross-section, allow a remarkable improvement of the experimental accuracy. Results are compared with theoretical predictions modeling different CNM effects.
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