bfys-physics April 2013

bfys-physics@nikhef.nl

6 participants
9 discussions

[Bfys-physics] Bfys Meeting Friday 18 january at 9:30 in N328 and on EVO
by Tjeerd Ketel 09 Jun '14

09 Jun '14

Bfys Meeting Friday 18 january at 9:30 in N328 and on EVO* Paper introduction and discussion: 9:30 "A search for D+(s) to pi+mu+mu- and D+(s) to pi-mu+mu+ decays" by Francesco Dettori http://cds.cern.ch/record/1504407 Veldhoven rehearsals: 10:30 "A new window for new physics in Bs decays to two muons" by Rob Knegjens 11:00 "The Bs meson decay in two muons: a search for rare beauty" by Serena Oggero 11:30 "Measurement of the angle gamma in the unitary triangle in time-dependent Bs to DsK decays at the LHCb experiment" by Manuel Schiller The presentations will be available (protected under lhcb, etc.) on the Nikhef agenda page and comments can be directly mailed to the speakers. Best regards, Tjeerd *)Today Vidyo could not provide the same service as EVO in our meeting room at Nikhef, therefore I decided to book this meeting again on EVO. Universe is the community, as LHCb has been removed. As a test we can open a room in Vidyo on Friday at 12:00. ========================================================= http://agenda.nikhef.nl/conferenceDisplay.py?confId=2361 ========================================================= You have BOOKED a meeting in SeeVogh Research Network (http://research.seevogh.com). Title: Nikhef Description: Bfys Meeting 9:30-12:00 Community: Universe Password: n328 Meeting Access Information: - Meeting URL SeeVogh R.N. http://research.seevogh.com/join?meeting=MsMiMI2u2IDnDe999aDt9s EVO International http://evo.caltech.edu/evoNext/koala.jnlp?meeting=MsMiMI2u2IDnDe999aDt9s - Password: n328 - Phone Bridge ID: 627 7875 Password: 6287 =========================================================

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[Bfys-physics] Thesis colloquium
by Jacco de Vries 23 May '13

23 May '13

Dear all, I am glad to announce the date of the colloquium of my master thesis. You can (hopefully) see the results of all the questions I have been bothering you with in the last few months at 9:30, May 23, in room N328 (Nikhef). The title will be "Search for the decay Bc -> Bs Pi". Your presence will be highly appreciated! Until then, Jacco

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[Bfys-physics] Fwd: LHCB-PAPER-2013-012-001-COMMENT-008 (a comment has been made on your comment)
by Wouter Hulsbergen 26 Apr '13

26 Apr '13

Dear all, Please see this link http://cds.cern.ch/record/1543516 for answers to our comments on the B->phiK* paper. Cheers, Wouter -------- Original Message -------- Return-Path: <cds.support(a)cern.ch> Received: from ambleve.nikhef.nl (ambleve.nikhef.nl [192.16.199.208]) by correze (Cyrus v2.3.7-Invoca-RPM-2.3.7-12.el5_7.2) with LMTPA; Tue, 23 Apr 2013 15:30:30 +0200 X-Sieve: CMU Sieve 2.3 Received: from localhost (localhost.localdomain [127.0.0.1]) by ambleve.nikhef.nl (Postfix) with ESMTP id 7D16078217 for <wouterh(a)nikhef.nl>; Tue, 23 Apr 2013 15:31:18 +0200 (CEST) X-Virus-Scanned: amavisd-new at nikhef.nl Received: from ambleve.nikhef.nl ([127.0.0.1]) by localhost (ambleve.nikhef.nl [127.0.0.1]) (amavisd-new, port 10024) with LMTP id HYuipx0v2-tF for <wouterh(a)nikhef.nl>; Tue, 23 Apr 2013 15:31:18 +0200 (CEST) Received: from filter5-til.mf.surf.net (filter5-til.mf.surf.net [194.171.167.221]) by ambleve.nikhef.nl (Postfix) with ESMTP id 6042378216 for <wouterh(a)nikhef.nl>; Tue, 23 Apr 2013 15:31:18 +0200 (CEST) Received: from CERNMX33.cern.ch (cernmx33.cern.ch [137.138.144.181]) by filter5-til.mf.surf.net (8.14.3/8.14.3/Debian-9.4) with ESMTP id r3NDVHMe022125 for <wouterh(a)nikhef.nl>; Tue, 23 Apr 2013 15:31:17 +0200 Received: from pcudssx1502.cern.ch (137.138.198.205) by cernmxlb2.cern.ch (137.138.144.184) with Microsoft SMTP Server (TLS) id 14.2.318.1; Tue, 23 Apr 2013 15:31:17 +0200 Received: from pcudssx1502.cern.ch (localhost.localdomain [127.0.0.1]) by pcudssx1502.cern.ch (8.13.8/8.13.8) with ESMTP id r3NDVG1v017678 for <wouterh(a)nikhef.nl>; Tue, 23 Apr 2013 15:31:16 +0200 Date: Tue, 23 Apr 2013 15:31:16 +0200 Message-ID: <201304231331.r3NDVG1v017678(a)pcudssx1502.cern.ch> MIME-Version: 1.0 Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 7bit From: CERN Document Server Submission Engine <cds.support(a)cern.ch> To: <wouterh(a)nikhef.nl> Subject: LHCB-PAPER-2013-012-001-COMMENT-008 (a comment has been made on your comment) User-Agent: Invenio 1.1.0.156-1d5a9 at http://cds.cern.ch X-Bayes-Prob: 0.0001 (Score 0, tokens from: @@RPTN) X-Spam-Score: -2.70 () [Tag at 5.00] T_RP_MATCHES_RCVD,SPF(pass:-1),RBL(RPRL-ham:-1.0),RBL(DNSWL-high-medium:-0.7) X-CanIt-Geo: ip=137.138.144.181; country=CH; region=07; city=Geneva; latitude=46.1956; longitude=6.1481; http://maps.google.com/maps?q=46.1956,6.1481&z=6 X-CanItPRO-Stream: nikhef:wouterh@nikhef.nl (inherits from nikhef:default,base:default) X-Canit-Stats-ID: 0WJrpvhpG - f425d68a374a - 20130423 (trained as not-spam) X-Antispam-Training-Forget: https://www.mf.surf.net/canit/b.php?i=0WJrpvhpG&m=f425d68a374a&t=20130423&c… X-Antispam-Training-Nonspam: https://www.mf.surf.net/canit/b.php?i=0WJrpvhpG&m=f425d68a374a&t=20130423&c… X-Antispam-Training-Spam: https://www.mf.surf.net/canit/b.php?i=0WJrpvhpG&m=f425d68a374a&t=20130423&c… X-Scanned-By: CanIt (www . roaringpenguin . com) on 194.171.167.221 Dear LHCb Colleague, The comment (LHCB-PAPER-2013-012-001-COMMENT-005) that you made on LHCB-PAPER-2013-012-001 (entitled: 'First observation of the decay $B_s^0 \to\phi\bar{K}^{*0}$') has itself been commented on by Cibran Santamarina Rios [CERN - PH/ULB] (cibran.santamarina.rios(a)cern.ch). This new comment (LHCB-PAPER-2013-012-001-COMMENT-008) may be seen at http://cds.cern.ch/record/1543516 Best regards, The CERN Document Server Server support Team

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[Bfys-physics] K*mumu review
by Patrick Koppenburg 09 Apr '13

09 Apr '13

Hi all, The K*mumu people were very fast in replying to our review. See https://cds.cern.ch/record/1537911 I have not digested all of that yet. One cookie goes to Jeroen for having spotted a mistake in a formula. Cheers, Patrick -- ======================================================================== Patrick Koppenburg Nikhef, Amsterdam http://www.koppenburg.org/address.html

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[Bfys-physics] Fwd: LHCb-UK Student Meeting Next Week: The DecayTreeFitter Tool
by Wouter Hulsbergen 09 Apr '13

09 Apr '13

Dear all, At 11am I'll give a short 'lecture' on decaytreefitter over Vidyo. It is for UK PhD students, but I guess everybody is welcome. You can find details below. Cheers. Wouter -------- Original Message -------- Return-Path: <Laurence.Carson(a)cern.ch> Received: from almonte.nikhef.nl (almonte.nikhef.nl [192.16.199.207]) by correze (Cyrus v2.3.7-Invoca-RPM-2.3.7-12.el5_7.2) with LMTPA; Thu, 04 Apr 2013 15:16:06 +0200 X-Sieve: CMU Sieve 2.3 Received: from localhost (localhost.localdomain [127.0.0.1]) by almonte.nikhef.nl (Postfix) with ESMTP id 79E3B68050 for <wouterh(a)nikhef.nl>; Thu, 4 Apr 2013 15:16:33 +0200 (CEST) X-Virus-Scanned: amavisd-new at nikhef.nl Received: from almonte.nikhef.nl ([127.0.0.1]) by localhost (almonte.nikhef.nl [127.0.0.1]) (amavisd-new, port 10024) with LMTP id MVpKwvnkoq7I for <wouterh(a)nikhef.nl>; Thu, 4 Apr 2013 15:16:33 +0200 (CEST) Received: from filter2-ams.mf.surf.net (filter2-ams.mf.surf.net [192.87.102.70]) by almonte.nikhef.nl (Postfix) with ESMTP id 48B6868051 for <wouterh(a)nikhef.nl>; Thu, 4 Apr 2013 15:16:33 +0200 (CEST) Received: from CERNMX31.cern.ch (cernmx31.cern.ch [137.138.144.179]) by filter2-ams.mf.surf.net (8.14.3/8.14.3/Debian-9.4) with ESMTP id r34DGWLr014026 for <wouterh(a)nikhef.nl>; Thu, 4 Apr 2013 15:16:32 +0200 Received: from CERNFE23.cern.ch (137.138.144.152) by cernmxgwlb2.cern.ch (137.138.144.179) with Microsoft SMTP Server (TLS) id 14.2.318.1; Thu, 4 Apr 2013 15:16:32 +0200 Received: from PLOXCHG24.cern.ch ([fe80::9864:103b:dbb5:decc]) by CERNFE23.cern.ch ([fe80::ecc5:abbf:62c:e03%10]) with mapi id 14.02.0318.004; Thu, 4 Apr 2013 15:16:31 +0200 From: Laurence Carson <Laurence.Carson(a)cern.ch> To: lhcb-uk (LHCb UK users) <lhcb-uk(a)cern.ch> CC: Wouter Hulsbergen <wouterh(a)nikhef.nl> Subject: LHCb-UK Student Meeting Next Week: The DecayTreeFitter Tool Thread-Topic: LHCb-UK Student Meeting Next Week: The DecayTreeFitter Tool Thread-Index: Ac4xNXC+Xbs4uMYSQjamrAqoj1njEA== Date: Thu, 4 Apr 2013 13:16:30 +0000 Message-ID: <8266323BCD326144A21F6334672B8932CDD839FF(a)PLOXCHG24.cern.ch> Accept-Language: en-GB, en-US Content-Language: en-GB X-MS-Has-Attach: X-MS-TNEF-Correlator: x-originating-ip: [128.141.155.239] Content-Type: multipart/alternative; boundary="_000_8266323BCD326144A21F6334672B8932CDD839FFPLOXCHG24cernch_" MIME-Version: 1.0 X-Bayes-Prob: 0.0001 (Score 0, tokens from: @@RPTN) X-Spam-Score: -2.70 () [Tag at 5.00] HTML_MESSAGE,T_RP_MATCHES_RCVD,SPF(pass:-1),RBL(RPRL-ham:-1.0),RBL(DNSWL-high-medium:-0.7) X-CanIt-Geo: ip=137.138.144.179; country=CH; region=07; city=Geneva; latitude=46.1956; longitude=6.1481; http://maps.google.com/maps?q=46.1956,6.1481&z=6 X-CanItPRO-Stream: nikhef:wouterh@nikhef.nl (inherits from nikhef:default,base:default) X-Canit-Stats-ID: 0QJjNgwMN - 16feac1036d8 - 20130404 (trained as not-spam) X-Antispam-Training-Forget: https://www.mf.surf.net/canit/b.php?i=0QJjNgwMN&m=16feac1036d8&t=20130404&c… X-Antispam-Training-Nonspam: https://www.mf.surf.net/canit/b.php?i=0QJjNgwMN&m=16feac1036d8&t=20130404&c… X-Antispam-Training-Spam: https://www.mf.surf.net/canit/b.php?i=0QJjNgwMN&m=16feac1036d8&t=20130404&c… X-Scanned-By: CanIt (www . roaringpenguin . com) on 192.87.102.70 Dear all, We are pleased to announce that there will be an LHCb-UK student meeting next Tuesday (April 9th), featuring a presentation by Wouter Hulsbergen discussing the DecayTreeFitter tool and its use in LHCb. This is a tool which is being used by an increasing number of analyses, so please come along to find out how it works and how it could be applied to your own analysis! Ahead of the meeting, Wouter asked us to circulate a couple of links that give some background information on DecayTreeFitter: 1) The original paper outlining the method http://arxiv.org/abs/physics/0503191 2) Some lectures from Wouter on tracking http://www.nikhef.nl/~wouterh/topicallectures/ (especially Parts 1 & 6) The meeting will start at 10am UK time (11am CERN time). The Indico page can be found here: https://indico.cern.ch/conferenceDisplay.py?confId=245278 There is a Vidyo booking attached to the meeting, the details are: Name of the room: LHCb_UK_Student_Meeting Extension: 9235227 PIN: 2924 For those at CERN, the meeting will be in the usual room, 32/S-C22. Coffee and pastries will be provided. We hope to see many of you there! Best Regards, Laurence, Steve, Thomas and Sam

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[Bfys-physics] K*mumu comments
by Patrick Koppenburg 05 Apr '13

05 Apr '13

Hi all, I compiled Niels', Jeroen's and my comments and will paste this into CDS if I get no more comments before 2: ------------------------------------------------------------------------------------------------------- Dear Tom, Nicola and friends, Congratulations for that impressive result. We are getting close to the roadmap (the central values as well, unfortunately...) Here are the comments from the Nikhef group. A few general comments: It's a difficult analysis resulting in a difficult paper to understand and more so to write. You've done a great job but there are still some places that could be clarified, especially Section 7. We find the description of the phi folding a bit detailed for the introduction. We suggest to be more brief in the intro, and move more detail to Sec.7.1. Fig.2: There seems to be a hump in all 6 bins around 5600 MeV. That happens to be the end of your training window. Have you studied these events? Table 2: It's not clear to use why you need to give corrected and uncorrected numbers. They are consistent at the 1/10th of a sigma level. Why not just give a systematic? Eq.(7) is a bit vague. We wouldn't know where to plug in these terms. Why is there an or? Either say more or less. 372: phimumu is on the same timescale as your paper. You could refer to it (here I'm getting myself into trouble as I just recommended to Christoph to refer to your paper - PK). But can't these decays be trivially vetoed at no signal cost. The phi is so narrow it cannot eat into the K* signal. Some maths questions and comments: L. 17 / Eqs. 1+2: - Both sin(phi) and the sign of cos(phi) are needed to determine phi. - Is this the correct definition of sin(phi)? - sin(phi) = [ (p^_mu+ x p^_mu-) x (p^_K+ x p^_pi-) ] . p^_K* - cos(phi) = (p^_mu+ x p^_mu-) . (p^_K+ x p^_pi-) * L. 17 / Eqs. 1+2: Eq. 3: S_6 * cos^2(t_K) * cos(t_l) --> S_6 * sin^2(t_K) * cos(t_l) (cos^2(t_K) is for the longitudinal--scalar interference) L. 249: From the expressions of observables in terms of amplitudes, one would (naively) expect the boundaries of A_FB and A_9 to be: |A_FB| <= 3/2 * (1-F_L) and |A_9| <= 1 * (1-F_L) (without taking into account correlations between A_FB, A_9 and S_3). Where does the factor two difference come from? L. 29, 33, 36, 308, 309, 398, 500, Tab. 2, Fig. 4: "K* amplitudes"/"K* polarisations": This is a bit sloppy. In general, the K* polarization doesn't fully determine the state of the mumuK* system. For example, it is also longitudinal for the state in which the mumu polarization is timelike. Maybe "decay amplitudes" and "polarization states"? Sect. 7.3, App. A: It is not obvious how the q^2-dependent factors in Eqs. 7, 14 and 15 are obtained. The most general expressions for the observables in terms of amplitudes cannot be written in this form. Can you indicate which assumptions for form factors and Wilson coefficients were made to obtain the large-recoil dilution factors? Is it described somewhere how this was done? L. 400-408: It is not entirely clear how F_S can be determined with the measurements of A_S: - You explain the procedure for "the P-wave amplitude" and "the S-wave amplitude". For single (transversity) amplitudes one can see how the magnitude of the S-wave amplitude can be determined from the difference in this 0-S interference term above and below the resonance. However, it is not obvious that this works if all observables are sums of left- and right-handed and B and Bbar terms. Do you need to make assumptions here? - Are values for F_L needed for this estimate of F_S? How are these obtained? - Do you combine this estimate of F_S with the direct measurement from the F_S term in the differential decay rate? 460: As you claim the zero-crossing point is precisely known, can't we include a prediction with error? Purely textual comments: Abstract+L.457 [no brackets around result] 7: [specify: ] '... larger theoretical uncertainties form hadronic form factors.' 10: why "so"? 17: and 19: no colon Eq.(1) and (2) replace . by \cdot 22: use \CP everywhere 23: of the one for the B0 decay (it's the definition, not the B that is transformed) 26: corresponds to -> is (?) 34: 3*S_2^s = 1-F_L --> 4*S_2^s = 1-F_L 34: S_6 is responsible for generating... S_6 and A_FB are just different parametrisation of the same thing. Please reword. e.g. Add the conversion factor between AFB and S6. 37: "not suppressed... involved". As opposed to what? 46: and _to_ provide (increases readability) 47: why don't you give the angular expression here? Isn't it equation 6? At least forward reference it. 49: {\rm Re} (we think) 50: [skip the colloquial sentence: ] 'Hence they are .. cleaner.' 56: Sections 4 and 5 are not mentioned. The backgrounds are in Section 4, not 3. 58: ', in terms of cos theta_l, ... ' 62: why [6] and not [44]? 71: do you need two citations of [10]? 90: which primary? 91: replace [18] by trigger paper [11]. 100: remove "consistent with that of the K*(892)" 122-123 [add commas:] ', and populates ... mass range, ' 133 'Psi(2S) mesons.' 136: "... are shown in Fig.~1." (not for reference) 146: Use template \Lb and \L. 148-151: rewrite that in 2 sentences. 149 'picking up' -> 'using' 153: and many other places. Why not J/psiK* instead of K*J/psi? It is much more common. 153: and a muon as a pion or a kaon (people outside LHCb do not know any track is a good pion). 156 Ref.[21] is old. Should be: arXiv:1301.5286] 157: [Why Yukawa??] 'SM Yukawa couplings' -> 'CKM elements' 160: SM simulation sounds like you're simulating the whole Standard Model. 162: the geometry cannot bias a distribution. Its acceptance does. 170: the K*0 decay. 176: What do you mean with 'normalised' and 'have the correct statistical power' ? 179: 2.0 -> two. 188: principle -> principal? 193: Is that really two CB or is one reversed? Fig.2 [x-axis more clear if:] m_Kpimumu -> m(Kpimumu) SetTitle("#font[12]{m}(K^{+}#pi^{#font[122]{-}}#mu^{+}#mu^{#font[122]{-}}) [MeV/#font[12]{c}^{2}]") Caption Table 1: Maybe mention what the second (and first) uncertainty is? 209 [don't repeat decay decsriptors] 'The values for the branching fractions are BR(.... ' 210: you should explain here why you use [24] and not [22] for J/psiK* 223 and 226: / -> and (or or) 251: "have an immediate correspondence to the transformations" rephrase 255: helicity _or_ transversity. BTW are they defined? If these relationships are not reproduced where, where can we find them? 256 and elsewhere: why put A^Re_T and A_T^2 in parentheses? You measure all of those. 260: uni-angular sounds like jargon. 261-264: How is the wrong-ID probability parameter omega treated in the fit? Is it fixed/constrained to the MC number from Section 4? 265: signal -> angular distribution, or model, or... 267: The angular observables vary... This is very important and should be mentioned the first time you explain you do fits in bins. 269: (1-F_L) why the parenthesis? 275 and 287: Feldman-Cousins 283: express? exhibit? 286: 'row' -> 'column' 302: We had to think a bit to realise that largest recoil was the lowest q^2 bin. Why not call it like that? 305: "dilute the impact of the observables" is also very vague. Footnote 2: Ref [31] is not the same as the gamma combination paper uses for the same method. We have no opinion on who's right, but one should agree if possible. 309 [missing 'meson' and 'be'; skip 'only one'; rewrite:] 'K*0 meson, FL, turns out to be the only observable that' L.310/311 [unclear, how about:] 'sensitivity to FL arises mainly from the shape of the costheta_k distribution, ' Fig.4 S_3 is bound to be less than 1/2(1-F_L). You could zoom in to at least -0.5<S_3<0.5. [caption] : 'prediction is included' -> 'prediction is shown' 316: S_3/A_FB : S_3 and A_FB. Or are you making a fraction? 333: SM _prediction_ 343: Can't you test the assumption of equal B and Bbar in your sample? 350: faithfully reproduce -> are in agreement with 369: You neglect 0.25? That should be explained. 421: A large sample. Not all? 424: by 7\% -> by up to 7\% Eq.12 would look better with: \left(1-F_{\rm L}(q^2)\right) [7] BELLE -> Belle [11] LHCb. There's an arxiv number. [18] Still needed? [21] There seems to be a space missing before TeV (to be replaced anyway) Cheers, Patrick, Jeroen, Niels for the Nikhef group -- ======================================================================== Patrick Koppenburg Nikhef, Amsterdam http://www.koppenburg.org/address.html

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[Bfys-physics] Fwd: CORRECTION concerning reading institutions for PAPER-2013-016, Production of $J/\psi$~and $\Upsilon(1S)$, $\Upsilon(2S)$ and $\Upsilon(3S)$~mesons at $\sqrt{s}=$8~TeV
by Patrick Koppenburg 05 Apr '13

05 Apr '13

A new paper for Nikhef! -------- Original Message -------- Subject: CORRECTION concerning reading institutions for PAPER-2013-016, Production of $J/\psi$~and $\Upsilon(1S)$, $\Upsilon(2S)$ and $\Upsilon(3S)$~mesons at $\sqrt{s}=$8~TeV Date: Mon, 18 Mar 2013 15:37:51 +0100 From: Rolf Oldeman <rudolf.oldeman(a)cern.ch> To: lhcb-general (LHCb General mailing list) <lhcb-general(a)cern.ch> Apologies, I made a mistake with the assignment of the reading institutions. The correct assignment is below. Best regards, Rolf Dear Colleagues, A paper is available for your comments: Title : Production of $J/\psi$~and $\Upsilon(1S)$, $\Upsilon(2S)$ and $\Upsilon(3S)$~mesons at $\sqrt{s}=$8~TeV Journal : JHEP Contact authors : Monica Pepe-Altarelli, Giulia Manca Reviewers : Johannes Albrecht (chair), Chris Parkes EB reviewer : Raluca Muresan EB readers : Niels Tuning, Joerg Marks Analysis note : ANA-2012-058 Deadline : 30-Mar-2013 e-group : lhcb-paper-2013-016-reviewers Link : http://cds.cern.ch/record/1528576 Authors : LHCb Twiki : https://twiki.cern.ch/twiki/bin/viewauth/LHCbPhysics/JPsiUpsilon8TeVXsec The following institutes are requested to make institutional comments: Cambridge, United Kingdom CBPF, Rio de Janeiro, Brazil Moscow State University, Russia LPNHE, Paris, France, Cincinnati, United States EPFL, Lausanne, Switzerland NIKHEF, Netherlands Please send any comments via the CDS system. It is the responsibility of the contact authors to provide replies on all comments made. Subsequent modification to the publication are made in consultation with the referees and during the EB reading. Following this, there will be a final meeting of the editorial board with contact authors and reviewers present where final decisions are made. As the last step a short presentation is given to the collaboration and the paper is sent for publication. You can find all paper and conference report drafts open for comments via the EB web-page, by clicking on Current Drafts. http://lhcb.web.cern.ch/lhcb/lhcb_page/collaboration/organization/editorial… Regards, Rolf Oldeman On Mar 16, 2013, at 9:43 AM, Rolf Oldeman wrote: > > Dear Colleagues, > > A paper is available for your comments: > > Title : > Production of $J/\psi$~and $\Upsilon(1S)$, $\Upsilon(2S)$ and > $\Upsilon(3S)$~mesons at $\sqrt{s}=$8~TeV > > Journal : JHEP > Contact authors : Monica Pepe-Altarelli, Giulia Manca > Reviewers : Johannes Albrecht (chair), > Chris Parkes > EB reviewer : Raluca Muresan > EB readers : Niels Tuning, Joerg Marks > Analysis note : ANA-2012-058 > Deadline : 30-Mar-2013 > e-group : lhcb-paper-2013-016-reviewers > Link : http://cds.cern.ch/record/1528576 > Authors : LHCb > Twiki : > https://twiki.cern.ch/twiki/bin/viewauth/LHCbPhysics/JPsiUpsilon8TeVXsec > > The following institutes are requested to make institutional comments: > Frascati, Italy > MPIK, Heidelberg, Germany > STFC (RAL), United Kingdom > IHEP, Protvino, Russia > Imperial College London, United Kingdom > Ruprecht-Karls-Universitat Heidelberg, Germany > > > Please send any comments via the CDS system. It is the responsibility > of the contact authors to provide replies on all comments > made. Subsequent modification to the publication are made in > consultation with the referees and during the EB reading. Following > this, there will be a final meeting of the editorial board with > contact authors and reviewers present where final decisions are > made. As the last step a short presentation is given to the > collaboration and the paper is sent for publication. > > You can find all paper and conference report drafts open for comments > via the EB web-page, by clicking on Current Drafts. > > http://lhcb.web.cern.ch/lhcb/lhcb_page/collaboration/organization/editorial… > > Regards, > Rolf Oldeman >

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[Bfys-physics] K*mumu paper
by Patrick Koppenburg 04 Apr '13

04 Apr '13

Dear all, I am collecting the comments on the paper "Differential branching fraction and angular analysis of the decay B0?K?0?+?-:"" " https://cds.cern.ch/record/1530660?ln=en Please send me your comments by Thursday 4 April. Cheers, Patrick -- ======================================================================== Patrick Koppenburg Nikhef, Amsterdam http://www.koppenburg.org/address.html

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[Bfys-physics] phi K* paper
by Wouter Hulsbergen 03 Apr '13

03 Apr '13

Dear all, I have been volunteered to send in our institutional review of the B0s->phiK* paper. For details see below. If you would like me to include your comments, please send them to me by April 4th. (There is no reason to be bored in your Easter holidays!) Cheers, Wouter ----- Title : First observation of the decay $B_s^0 \to\phi\bar{K}^{*0}$ Journal : JHEP Contact authors : Antonio Romero, Cibran Santamarina Rios Reviewers : Alvaro Neto (chair), Steve Playfer EB reviewer : Steven Blusk EB readers : Tim Gershon, Frederic Machefert Analysis note : ANA-2012-030 Deadline : 05-Apr-2013 e-group : lhcb-paper-2013-012-reviewers Link : http://cds.cern.ch/record/1530549 Authors : LHCb Twiki : https://twiki.cern.ch/twiki/bin/viewauth/LHCbPhysics/BsToKstarKstar The following institutes are requested to make institutional comments: Ferrara, Italy Warwick, United Kingdom Dortmund, Germany EPFL, Lausanne, Switzerland NIKHEF, Netherlands

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bfys-physics April 2013