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star-fcv-l - Re: [Star-fcv-l] FCV PWG meeting, 18/Nov/2020 (Wed) 9:30am (New York time zone)

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: "Wang, Fuqiang" <fqwang AT purdue.edu>
  • To: jagbir <jagbir AT rcf.rhic.bnl.gov>
  • Cc: "star-cme-focusgroup-l AT lists.bnl.gov" <star-cme-focusgroup-l AT lists.bnl.gov>, "levanfinch AT gmail.com" <levanfinch AT gmail.com>, "aggarwal AT pu.ac.in" <aggarwal AT pu.ac.in>, "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] FCV PWG meeting, 18/Nov/2020 (Wed) 9:30am (New York time zone)
  • Date: Sun, 16 May 2021 00:52:34 +0000

Jagbir,
 
See comments below.
 
Best regards,
Fuqiang
 
 
> -----Original Message-----
> From: jagbir <jagbir AT rcf.rhic.bnl.gov>
> Sent: Friday, May 14, 2021 3:01 PM
> To: Wang, Fuqiang <fqwang AT purdue.edu>
> Cc: esumi.shinichi.gn AT u.tsukuba.ac.jp; ptribedy AT rcf.rhic.bnl.gov;
> jiangyong.jia AT stonybrook.edu; levanfinch AT gmail.com; aihong AT bnl.gov;
> aggarwal AT pu.ac.in; STAR Flow, Chirality and Vorticity PWG <star-fcv-
> l AT lists.bnl.gov>; star-cme-focusgroup-l AT lists.bnl.gov
> Subject: Re: [Star-fcv-l] FCV PWG meeting, 18/Nov/2020 (Wed) 9:30am (New
> York time zone)
>
> Dear Fuqiang,
>
> Thank you for your nice reply with analogy. Please see my reply below:
>
> 1. These plots are simply Delta gamma, right? Then they are expected to be non-
> zero. I don't understand the statement here "the correlated background is zero".
> What do you mean?
>
> The correlated background is obtained by restoring the charges of shuffled and
> flipped charges in each event which in this case means one gets original default
> AMPT event in which delta gamma is zero. So, the correlated background is zero.
>
[Fuqiang Wang] I'm confused. Why does default AMPT give Delta gamma = 0?
 
> 2. How did you obtain the points on slide 25? Is it red-black and blue-black of
> some sort from slide 24? How were the black points on s25 obtained?
>
> All points on slide 25 are for different samples (i.e., Fix-1(Red),
> Fix-2(Blue) and AMPT(Black)) obtained from slide 24 as discussed earlier i.e.,
>
> (delta_gamma_data - delta_gamma_shuffle - delta_gamma_corr)/delta
> gamma_data
>
> delta_gamma_shuffle is not shown in slide 24. This presentation is regarding the
> comments.
> Black points are for default AMPT.
[Fuqiang Wang] Does the default AMPT have Delta gamma = 0 as you said above?
>
> 3(a). f_DbCs from events shuffled +/- particles <-> Nch from events shuffled
> charged/neutral particles
>
> We consider f_DbCS from data itself in different centrality bins not just from
> Shuffled.
>
> 3(b). We take difference between real signal and shuffled signal.
>
> We first take difference between gamma_OS and gamma_SS for data as well as
> for charge shuffled events. So we get two delta gamma, one for data (without
> shuffled) and other for charge shuffled events. Now the difference is taken
> between the delta gamma data and delta gamma charge shuffled to get f_CME.
> How do you take difference between real signal and shuffled signal?
>
> 3(c). You're seeing positive Delta gamma in large f_DbCs events;
>
> We see positive Delta gamma in large f_DbCs in data as well as in charge
> shuffled.
>
> 3(d). I'm seeing neutral/charged>1/2 in peripheral events and <1/2 in central
> events. I'll see this even when neutral/charged=1/3 is independent of centrality
> (not to say possibly centrality-dependent neutral/charged).This is called
> selection bias.
>
> Did you get these number from running AMPT and how many events were used?
> Are you seeing this in shuffled events? How it can happen let me understand this.
> I hope during shuffle you keep number of charged particles and neural particles
> same in each event. If it is so how this ratio of neutral/charged can change after
> shuffle. Centrality bin you define by the number of charged particle. So if
> number of charged particle in each event remain the same, as you keep Nch and
> neutral same during shuffle, so the centrality bin should remain the same. So this
> ratio of neutral/charged should remain the same in peripheral events as well as
> in central events you had before shuffle. You have wrote about neutral/charged
> for charge shuffled events. You did not write any thing about real events
> whereas we discussed both real data and charge shuffled.
>
> During shuffle I keep the number of positive and negative particle same in each
> event and also keep flow in. Alice collaboration used event shape engineering to
> probe CME signal (Phys. Lett. B777, 151 (2018)).
> Here, each centrality is divided into 10 bins depending on Q value. Is this
> selection bias?
>
[Fuqiang Wang] Because you brought up the analogy of f_DbCs to centrality, so I was using neutral/charged to tell you that your enhanced f_DbCs events are mostly, if not all, selection bias. The neutral/charged in my example serves different purpose from the +/- in your analysis. Please think about it.
 
> Thank you,
>
> With Best Regards,
> Jagbir Singh
> Panjab University
> Chandigarh
>
>
> On 2021-05-11 20:53, Wang, Fuqiang wrote:
> > Jagbir,
> >
> > Please see my comments below.
> >
> > Best regards,
> > Fuqiang
> >
> >> -----Original Message-----
> >> From: jagbir <jagbir AT rcf.rhic.bnl.gov>
> >> Sent: Tuesday, May 11, 2021 7:44 AM
> >> To: esumi.shinichi.gn AT u.tsukuba.ac.jp; ptribedy AT rcf.rhic.bnl.gov;
> >> jiangyong.jia AT stonybrook.edu; levanfinch AT gmail.com; aihong AT bnl.gov;
> >> aggarwal AT pu.ac.in; Wang, Fuqiang <fqwang AT purdue.edu>
> >> Cc: STAR Flow, Chirality and Vorticity PWG
> > <star-fcv-l AT lists.bnl.gov>; star-cme-
> >> focusgroup-l AT lists.bnl.gov
> >> Subject: Re: [Star-fcv-l] FCV PWG meeting, 18/Nov/2020 (Wed) 9:30am
> > (New
> >> York time zone)
> >>
> >> Dear Fuqiang,
> >>
> >> Thanks for your nice comments. Please find below my reply to your
> > comments.
> >>
> >> 1. Effectively, your signal after subtraction of correlated
> > background will
> >> average to zero within a centrality bin.
> >>
> >> Not true, In case of Fix-1 and Fix-2 substracting the correlated
> > background
> >> which is obtained from default AMPT, signal is not zero within
> > centrality bin as
> >> the correlated background is zero (Slide 18 & 19).
> >>
> > [Fuqiang Wang] These plots are simply Delta gamma, right? Then they
> > are expected to be non-zero. I don't understand the statement here
> > "the correlated background is zero". What do you mean?
> >
> >> 2. You divide this centrality bin into 10 bins according to your
> > dumbbell variable,
> >> in real event and in shuffled event. You take the difference of two,
> > so you're
> >> deemed to have some bins positive and other bins negative. You are
> > always
> >> going to have CME signal no matter what (except the rare case where
> > all bins
> >> are zero).
> >>
> >> Not true, In slide 24 (slide 25 for f_{CME}) we do not see any CME
> > signal for
> >> default AMPT.
> >>
> > [Fuqiang Wang] How did you obtain the points on slide 25? Is it red -
> > black and blue - black of some sort from slide 24? How were the black
> > points on s25 obtained?
> >
> >> 3. I don't think you can take such a liberty to claim positive bins
> > as CME signal
> >> and ignore negative bins.
> >>
> >> We are categorising events depending on the back-to-back charge
> > separation as
> >> one divides events in to different collision centralities depending
> > on the impact
> >> parameter or event multiplicity. The positive bin corresponds to
> > gamma positive
> >> for opposite-sign charge pairs and gamma negative for same-sign
> > charge pairs
> >> which means same sign charge pairs are strongly correlated whereas
> > opposite-
> >> sign charge pairs are weekly correlated which is considered as the
> > CME signal.
> >> The negative bin corresponds to opposite-sign charge pairs strongly
> > correlated
> >> (negative gamma) and same-sign charge pairs weekly correlated
> > (positive
> >> gamma) those evens look
> >> like normal events i.e, no CME signal.
> >>
> > [Fuqiang Wang] Let me use your analogy of f_DbCs binning ßà centrality
> > binning:
> > Your selection is f_DbCs ßà my selection is Nch f_DbCs from events
> > shuffled +/- particlesßà Nch from events shuffled charged/neutral
> > particles Delta gamma ßà neutral/charged ratio We take difference
> > between real signal and shuffled signal.
> > You're seeing positive Delta gamma in large f_DbCs events; I'm seeing
> > neutral/charged>1/2 in peripheral events and <1/2 in central events.
> > I'll see this even when neutral/charged=1/3 is independent of
> > centrality (not to say possibly centrality-dependent neutral/charged).
> > This is called selection bias.
> > I cannot claim those neutral/charged>1/2 events as some exotic
> > physics, and ignore the neutral/charged<1/2 events (or vice versa).
> >
> >> Thanking you,
> >>
> >> With best regards,
> >> Jagbir Singh
> >> Panjab University
> >> Chandigarh
> >>
> >> On 2021-05-06 13:23, jagbir wrote:
> >> > Dear all,
> >> >
> >> > These are our email exchange from December last year. We have
> > answered
> >> > all the comments earlier.
> >> > Please check.
> >> >
> >> > Thank you,
> >> > Jagbir Singh
> >> > Panjab University
> >> > Chandigarh
> >> >
> >> >
> >> > On 2020-12-17 16:40, jagbir wrote:
> >> >> Dear Fuqiang,
> >> >>
> >> >> Please find my replies here below:
> >> >>
> >> >> In the rightmost data points, the f_cme signals appear negative
> >> >> beacuse of substracting the correlated background. But we
> > interpret
> >> >> CME-like signal if gamma_ss is negative and gamma_os is positive
> >> >> which is the case for leftmost data points whereas for the
> > rightmost
> >> >> data points gamma_ss is positive and gamma_os is negative, so
> > these
> >> >> rightmost points do not correspond to CME-like.
> >> >> So, for the rightmost data points, we can not interpret it as
> >> >> negative f_cme signal.
> >> >> The rightmost points correspond to normal behavior where opposite
> >
> >> >> sign charged particles are correlated and same sign charged
> > particles
> >> >> are uncorrelated.
> >> >>
> >> >> Thank you,
> >> >>
> >> >> With regards,
> >> >> Jagbir Singh
> >> >>
> >> >> On 2020-12-16 03:40, Wang, Fuqiang wrote:
> >> >>> Jagbir,
> >> >>>
> >> >>> Thanks for the plot. So you interpret the leftmost points as
> > from
> >> >>> CME and extract a CME fraction from it. What physics would you
> >> >>> interpret the rightmost data points where the signals appear
> > negative?
> >> >>>
> >> >>> Best regards,
> >> >>> Fuqiang
> >> >>>
> >> >>>
> >> >>>
> >> >>>> -----Original Message-----
> >> >>>> From: jagbir <jagbir AT rcf.rhic.bnl.gov>
> >> >>>> Sent: Tuesday, December 15, 2020 8:55 AM
> >> >>>> To: Wang, Fuqiang <fqwang AT purdue.edu>
> >> >>>> Cc: STAR Flow, Chirality and Vorticity PWG
> >> >>>> <star-fcv-l AT lists.bnl.gov>; star-cme-
> > focusgroup-l AT lists.bnl.gov;
> >> >>>> aggarwal AT pu.ac.in
> >> >>>> Subject: Re: [Star-fcv-l] FCV PWG meeting, 18/Nov/2020 (Wed)
> > 9:30am
> >> >>>> (New York time zone)
> >> >>>>
> >> >>>> Dear Fuqiang,
> >> >>>>
> >> >>>> Please find my replies below:-
> >> >>>>
> >> >>>> ------------------------------
> >> >>>>
> >> >>>>       1. because your selection is predominated by statistical
> >> >>>> fluctuations yet
> >> >>>>       you're applying a cut on those statistical fluctuations.
> >> >>>>
> >> >>>>       Our selection is not by statistical fluctuations but
> > based on
> >> >>>> fractional
> >> >>>>       Dumbbell charge separation in the data. However, similar
> > type
> >> >>>> of charge
> >> >>>>       separation can be due to statistical fluctuations, to
> > account
> >> >>>> for that
> >> >>>>       we are using charge reshuffle. Now we are having about
> > 160M
> >> >>>> events.
> >> >>>> It is
> >> >>>>       seen that observed delta gamma in the data is large
> > beyond
> >> >>>> statistical
> >> >>>>       fluctuations than those of charge reshuffle for  the top
> >> >>>> 0-20%
> >> >>>> Db+-max
> >> >>>>       bins. The plot you asked is attached here with email.
> >> >>>>
> >> >>>> ------------------------------
> >> >>>>
> >> >>>>       2. I mean the max Dbmax_shuffle bin is a random
> > collection of
> >> >>>> events from
> >> >>>>       this centrality bin.
> >> >>>>
> >> >>>>       The max Dbmax_shuffle bin is not a random collection of
> >> >>>> events from
> >> >>>>       this centrality bin. As explained earlier we generated
> > charge
> >> >>>> reshuffle
> >> >>>>       events by reshuffling charges of partices in the real
> > data in
> >> >>>> a given
> >> >>>>       collision centrality. So, charge reshuffle events are
> >> >>>> completely independent
> >> >>>>       sample from real data sample in  given centrality though
> >> >>>> number of
> >> >>>>       positive/negative charged partciles are kept same in each
> >
> >> >>>> reshuffle event
> >> >>>>       corresponding to real data event. Again  Dbmax_shuffle
> > bins
> >> >>>> are made
> >> >>>>       according to the fractional Dumbbell charge separation in
> > the
> >> >>>> charged
> >> >>>>       reshuffle event sample for a given collision centrality.
> >> >>>>
> >> >>>> ------------------------------
> >> >>>>
> >> >>>> Thank you,
> >> >>>> Jagbir Singh
> >> >>>>
> >> >>>>
> >> >>>> On 2020-12-14 22:46, Wang, Fuqiang wrote:
> >> >>>> > Jagbir,
> >> >>>> >
> >> >>>> > Please see my replies below.
> >> >>>> >
> >> >>>> > Best regards,
> >> >>>> > Fuqiang
> >> >>>> >
> >> >>>> >
> >> >>>> >
> >> >>>> >> -----Original Message-----
> >> >>>> >> From: jagbir <jagbir AT rcf.rhic.bnl.gov>
> >> >>>> >> Sent: Monday, December 14, 2020 11:18 AM
> >> >>>> >> To: Wang, Fuqiang <fqwang AT purdue.edu>
> >> >>>> >> Cc: STAR Flow, Chirality and Vorticity PWG
> >> >>>> >> <star-fcv-l AT lists.bnl.gov>;
> >> >>>> >> star-cme-
> >> >>>> >> focusgroup-l AT lists.bnl.gov; aggarwal AT pu.ac.in
> >> >>>> >> Subject: Re: [Star-fcv-l] FCV PWG meeting, 18/Nov/2020 (Wed)
> >
> >> >>>> >> 9:30am (New York time zone)
> >> >>>> >>
> >> >>>> >> Dear Fuqiang,
> >> >>>> >>
> >> >>>> >>     Please find my replies below:-
> >> >>>> >>
> >> >>>> >> 1.   I understand your motivation doing that but I don't
> > agree this is
> >> >>>> >> the right approach
> >> >>>> >>     (I think it causes biases).
> >> >>>> >>
> >> >>>> >>     Please let me know why this is not the right approach
> > and
> >> >>>> >> what kind of biases you meant.
> >> >>>> > [Fuqiang Wang] because your selection is predominated by
> >> >>>> > statistical fluctuations yet you're applying a cut on those
> >> >>>> > statistical fluctuations.
> >> >>>> >
> >> >>>> > Can you plot (data-chrgR. Bkg) and (Correlated bkg) vs (Dbmax
> >
> >> >>>> > bin) on slide 25 so we can see the details better?
> >> >>>> >
> >> >>>> >>
> >> >>>> >>
> >> >>>> >> 2.   you have only one point left. Your f_cme is basically
> > the
> >> >>>> >>       (Delta gamma of those events in that Dbmax bin)
> >> >>>> >>       - (Delta gamma of a random collection of events in the
> >
> >> >>>> >> same centrality bin which happen
> >> >>>> >>       to have the same Dbmax_shuffle bin)
> >> >>>> >>       - (Delta gamma of those same random events calculated
> >> >>>> >> after the charges are shuffled)
> >> >>>> >>       Do I understand it correctly?
> >> >>>> >>
> >> >>>> >>     If only one point is left as you wrote, please see the
> >> >>>> >> explanation
> >> >>>> >> below:
> >> >>>> >>
> >> >>>> >>     Here, there is nothing like random collection of events
> > in
> >> >>>> >> the same centrality bin.
> >> >>>> > [Fuqiang Wang] I mean the max Dbmax_shuffle bin is a random
> >> >>>> > collection of events from this centrality bin.
> >> >>>> >
> >> >>>> >>     We select events depending on Db+-max i.e., depending on
> > the
> >> >>>> >> back-to-back charge
> >> >>>> >>     separation fDbCS = Db+-max-1. As you wrote only one
> > point,
> >> >>>> >> in that case it is the
> >> >>>> >>     top 10% Db+-max events corresponding to maximum
> > back-to-back
> >> >>>> >> charge separation events.
> >> >>>> >>     It is similar to selecting events in particular
> > collision
> >> >>>> >> centrality depending on
> >> >>>> >>     the impact parameter or event multiplicity. As we have
> >> >>>> >> selected in the data top 10%
> >> >>>> >>     Db+-max corresponding to maximum back-to-back charge
> >> >>>> >> separation events, in  same way
> >> >>>> >>     we select events from charge reshuffle in the same
> > collision
> >> >>>> >> centrality for top 10%
> >> >>>> >>     Db+-max(here Db+-max of charge reshuffle) corresponding
> > to
> >> >>>> >> maximum
> >> >>>> >> back-
> >> >>>> >> to-back
> >> >>>> >>     separation. Now we get delta_gamma_data of real data
> > events
> >> >>>> >> corresponding to top
> >> >>>> >>     10% Db+-max of data and delta_gamma_sta of charge
> > reshuffle
> >> >>>> >> events corresponding to top
> >> >>>> >>     10% Db+-max of charge reshuffle for a given collision
> >> >>>> >> centrality which gives
> >> >>>> >>     us delta_gamma due to statistical fluctuations. Now for
> >> >>>> >> correlated background we
> >> >>>> >>     look for real events in the data corresponding to the
> > top
> >> >>>> >> 10%
> >> >>>> >> Db+-max
> >> >>>> >>   of charge
> >> >>>> >>     reshuffle in a given centrality and get delta_gamma_cor
> > from
> >> >>>> >> those real
> >> >>>> >>     data events.
> >> >>>> >>
> >> >>>> >>     Now the f_CME is obtained as
> >> >>>> >>
> >> >>>> >>     f_CME = N1*(delta_gamma_data - delta_gamma_sta -
> >> >>>> >> delta_gamma_cor)/(delta_gamma_data * N)
> >> >>>> >>
> >> >>>> >>     Where N1 is number of events in top 10% Db+-max and
> >> >>>> >>     N is total number of events in a given collision
> > centrality.
> >> >>>> >>
> >> >>>> >> Thank you,
> >> >>>> >> With regards,
> >> >>>> >> Jagbir Singh
> >> >>>> >>
> >> >>>> >> On 2020-12-14 10:32, Wang, Fuqiang wrote:
> >> >>>> >> > Jagbir,
> >> >>>> >> >
> >> >>>> >> > Thanks for your answers.
> >> >>>> >> >
> >> >>>> >> > To your questions:
> >> >>>> >> >> Please clarify the following
> >> >>>> >> >>       Of course you've also removed the large
> > charge-shuffle
> >> >>>> >> >> background which is basically
> >> >>>> >> >>       an autocorrelation effect (sort to speak) due to
> > the
> >> >>>> >> >> Dbmax (and
> >> >>>> >> >> Dbmax_shuffle)
> >> >>>> >> >>       selection bias.
> >> >>>> >> > I was just saying it in passing, referring to the fact
> > that
> >> >>>> >> > you're largely selecting on statistical fluctuations and
> >> >>>> >> > trying to remove the auto-correlation effect by shuffling.
> > It wasn't a
> >> question.
> >> >>>> >> >
> >> >>>> >> >>       Please explain the following:
> >> >>>> >> >>       So is your finite signal really due to the
> > difference
> >> >>>> >> >> between the average of ratios
> >> >>>> >> >>       and the ratio of averages (or perhaps also due to
> >> >>>> >> >> residual effect from shuffling)?
> >> >>>> >> > I was referring to the fact that if you had a single Dbmax
> > bin (i.e.
> >> >>>> >> > taking average first and then ratio) then you'd get zero
> >> >>>> >> > signal by definition. You now have 10 bins and take ratios
> >
> >> >>>> >> > first in each bin and then take average of the ratios, and
> > get a positive
> >> signal.
> >> >>>> >> > During the focus meeting discussion, it was made clear
> > that
> >> >>>> >> > your analysis required multiple Dbmax bins, not taking
> > average
> >> >>>> >> > of all bins, but only those with Delta gamma > 0. So now I
> >
> >> >>>> >> > think I understand technically how you did it. I
> > understand
> >> >>>> >> > your motivation doing that but I don't agree this is the
> > right
> >> >>>> >> > approach (I think it causes
> >> >>>> biases).
> >> >>>> >> > So let me try to understand better:
> >> >>>> >> > On slide 9 of your focus meeting presentation
> >> >>>> >> >
> > https://drupal.star.bnl.gov/STAR/system/files/CME_FOCUS.pdf,
> >> >>>> >> > you
> >> >>>> >> > state:
> >> >>>> >> > (1) If Delta gamma_bkg. is negative then it is taken as
> > zero.
> >> >>>> >> > (2) If gamma_SS is not negative and gamma_OS is not
> > positive
> >> >>>> >> > then delta gamma = 0.
> >> >>>> >> > Now to slide 25, let's take one centrality say 40-50%, you
> >
> >> >>>> >> > have the blue points (signal) and red+green points (bkg).
> > The
> >> >>>> >> > 8 points to the right of this centrality: all of them have
> >
> >> >>>> >> > negative bkg and negative Delta gamma, so they are not
> > counted
> >> >>>> >> > in your calculation of CME fraction. Now you're left with
> > the
> >> >>>> >> > two leftmost points. Do both points satisfy (2) above? I
> > know
> >> >>>> >> > both points seem to have
> >> >>>> >> > bkg>0 & Delta
> >> >>>> >> > gamma>0 but it's unclear if they satisfy SS<0 & OS>0.
> > Assume
> >> >>>> >> > gamma>they do,
> >> >>>> >> > then you're taking average of these two data points. For
> > the
> >> >>>> >> > sake of simplicity, let me say you have only one point
> > left.
> >> >>>> >> > Your f_cme is basically the (Delta gamma of those events
> > in
> >> >>>> >> > that Dbmax bin)
> >> >>>> >> > - (Delta gamma of a random collection of events in the
> > same
> >> >>>> >> > centrality bin which happen to have the same Dbmax_shuffle
> >
> >> >>>> >> > bin)
> >> >>>> >> > - (Delta gamma of those same random events calculated
> > after
> >> >>>> >> > the charges are shuffled) Do I understand it correctly?
> >> >>>> >> >
> >> >>>> >> > Best regards,
> >> >>>> >> > Fuqiang
> >> >>>> >> >
> >> >>>> >> >
> >> >>>> >> >
> >> >>>> >> >> -----Original Message-----
> >> >>>> >> >> From: jagbir <jagbir AT rcf.rhic.bnl.gov>
> >> >>>> >> >> Sent: Sunday, December 13, 2020 10:12 AM
> >> >>>> >> >> To: Wang, Fuqiang <fqwang AT purdue.edu>
> >> >>>> >> >> Cc: STAR Flow, Chirality and Vorticity PWG
> >> >>>> >> >> <star-fcv-l AT lists.bnl.gov>;
> >> >>>> >> >> star-cme-
> >> >>>> >> >> focusgroup-l AT lists.bnl.gov; aggarwal AT pu.ac.in
> >> >>>> >> >> Subject: Re: [Star-fcv-l] FCV PWG meeting, 18/Nov/2020
> > (Wed)
> >> >>>> >> >> 9:30am (New York time zone)
> >> >>>> >> >>
> >> >>>> >> >> Dear Fuqiang, all,
> >> >>>> >> >>
> >> >>>> >> >>    Sorry for not answering your email. Infact, I did not
> > look this
> >> >>>> >> >>    email. Please go through my replies below:
> >> >>>> >> >> ------------------------
> >> >>>> >> >>
> >> >>>> >> >>   1. A few events do not satisfy this cut so not
> > including in
> >> >>>> >> >> it
> >> >>>> >> >> Db+-max
> >> >>>> >> >>      but in overall calculations all events are included.
> >
> >> >>>> >> >>
> >> >>>> >> >>   2. Yes
> >> >>>> >> >>
> >> >>>> >> >>   3. We reshuffle charges in each event. We donot
> > randomize
> >> charges
> >> >>>> >> >>      according to the positive/negative charge ratio of
> > the
> >> >>>> >> >> given event.
> >> >>>> >> >>      In fact, we pick up one event and reshuffle
> >> >>>> >> >> positive/negative charges
> >> >>>> >> >>      keeping theta,  phi, number of postive charges and
> >> >>>> >> >> number of negative
> >> >>>> >> >>      charges as such. After this we calculate gamma
> > correlator.
> >> >>>> >> >> This procedure
> >> >>>> >> >>      is repeated for each event. The Db+-max of reshuffle
> >  is
> >> >>>> >> >> a bit bit wider
> >> >>>> >> >>      than the  real distribution which may be due to some
> >
> >> >>>> >> >> correlations in the
> >> >>>> >> >>      real data whereas reshuffle is purely randomize.
> > Db+-max
> >> >>>> >> >> binning is
> >> >>>> >> >>      done on the basis of same fractions.
> >> >>>> >> >>
> >> >>>> >> >>   4. Let me explain this point
> >> >>>> >> >>
> >> >>>> >> >>      We pick up a real data event and calculate following
> >
> >> >>>> >> >>      i)  Dbmax+- of real data event
> >> >>>> >> >>      ii) reshuffle charges in an event
> >> >>>> >> >>
> >> >>>> >> >>      iii) again calculate Dbmax+- and termed it Db+-max
> > of
> >> >>>> >> >> charge reshuffle
> >> >>>> >> >>      iv)  calculate gamma of real data event
> >> >>>> >> >>      v)   calculate gamma of reshuffle event
> >> >>>> >> >>
> >> >>>> >> >>      Now for a given centrality
> >> >>>> >> >>      Steps i) to v) repeated for each event. Db+-max
> > (data)
> >> >>>> >> >> and
> >> >>>> >> >> Db+-max(reshuffle)
> >> >>>> >> >>      sliced into ten percentile bins.
> >> >>>> >> >>      Now average gamma is found in every sliced Db+-max
> >> >>>> >> >> (data) and
> >> >>>> >> >> Db+-max(reshuffle)
> >> >>>> >> >>      from the respective event samples. It should be
> > noted
> >> >>>> >> >> that events in the top
> >> >>>> >> >>      say 10% Db+-max(data) are not the same as in the top
> > 10%
> >> >>>> >> >> Db+-max(reshuffle) i.e,
> >> >>>> >> >>      real events in the top 10% Db+-max(data) are
> > different
> >> >>>> >> >> from those top 10%
> >> >>>> >> >>      Db+-max(reshuffle). Now the correlated background is
> >
> >> >>>> >> >> caculated from the real events
> >> >>>> >> >>      corresponding to the top 10% Db+-max(reshuffle)
> > events.
> >> >>>> >> >>
> >> >>>> >> >>       Please clarify the following
> >> >>>> >> >>
> >> >>>> >> >>       Of course you've also removed the large
> > charge-shuffle
> >> >>>> >> >> background which is basically
> >> >>>> >> >>       an autocorrelation effect (sort to speak) due to
> > the
> >> >>>> >> >> Dbmax (and
> >> >>>> >> >> Dbmax_shuffle)
> >> >>>> >> >>       selection bias.
> >> >>>> >> >>
> >> >>>> >> >>   5.  Db+-max distribution is sliced in to ten percentile
> >
> >> >>>> >> >> bins which represent
> >> >>>> >> >>       different amount of charge separation in each
> > sliced
> >> >>>> >> >> db+-max bin.
> >> >>>> >> >> Let us
> >> >>>> >> >>       say we have Db+-max = 2, in this case fractional
> >> >>>> >> >> dumbbell charge separation
> >> >>>> >> >>       f_DbCS = Db+-max-1=1 i.e., 100% back-to-back charge
> >
> >> >>>> >> >> separation i.e.,
> >> >>>> >> >>       positive charged particles on one side of the
> > dumbbell
> >> >>>> >> >> and negative charge
> >> >>>> >> >>       particles on other side of the dumbbell. So,
> > computing
> >> >>>> >> >> gamma in different
> >> >>>> >> >>       Db+-max and calculating things is different from
> > just
> >> >>>> >> >> making a single wide
> >> >>>> >> >>       bin as you mentioned. This method is designed to
> > get
> >> >>>> >> >> CME-like enriched sample
> >> >>>> >> >>       in given collision centrality as one divides all
> > events
> >> >>>> >> >> into different collision
> >> >>>> >> >>       centralities depending on either the impact
> > parameter
> >> >>>> >> >> or event multiplicity but
> >> >>>> >> >>       one does not study all events taken together
> > without
> >> >>>> >> >> making different
> >> >>>> >> >>       collision centrality classes. However, for a single
> >
> >> >>>> >> >> wide
> >> >>>> >> >> Db+-max bin as you
> >> >>>> >> >>       wrote we will get zero signal.
> >> >>>> >> >>
> >> >>>> >> >>       Please explain the following:
> >> >>>> >> >>
> >> >>>> >> >>       So is your finite signal really due to the
> > difference
> >> >>>> >> >> between the average of ratios
> >> >>>> >> >>       and the ratio of averages (or perhaps also due to
> >> >>>> >> >> residual effect from shuffling)?
> >> >>>> >> >>
> >> >>>> >> >>
> >> >>>> >> >> Thank you,
> >> >>>> >> >>
> >> >>>> >> >> with regards,
> >> >>>> >> >> Jagbir Singh
> >> >>>> >> >>
> >> >>>> >> >>
> >> >>>> >> >>
> >> >>>> >> >> On 2020-11-18 23:18, Wang, Fuqiang wrote:
> >> >>>> >> >> > Hi Jagbir,
> >> >>>> >> >> >
> >> >>>> >> >> > Your results are quite interesting. I have a few
> > further
> >> >>>> >> >> > questions about the details of your analysis:
> >> >>>> >> >> > 1. For each event you have Dbmax with the condition of
> >> |Dbasy|<0.25.
> >> >>>> >> >> > You bin events of each centrality in Dbmax. You use all
> >
> >> >>>> >> >> > events in your analysis (i.e. you're not throwing away
> >> >>>> >> >> > events based on Dbmax or Dbasy), right?
> >> >>>> >> >> > 2. In your calculation of gamma=<...>/v2c for a
> > particular
> >> >>>> >> >> > Dbmax bin of a given centrality, the v2c is calculated
> >> >>>> >> >> > using those events only, right?
> >> >>>> >> >> > 3. For the charge reshuffle, you reshuffle the charges
> > of
> >> >>>> >> >> > all events, and repeat your analysis from step 1 (i.e.
> > you
> >> >>>> >> >> > treat this as a completely separate "new" data sample),
> >
> >> >>>> >> >> > right? Did you "randomize" the charges according to the
> >
> >> >>>> >> >> > positive/negative charge ratio of the given event? On
> > s11,
> >> >>>> >> >> > the Dbmax_shuffle distribution is a bit wider than the
> > real
> >> >>>> >> >> > distribution, do you understand why? How do you bin the
> >
> >> >>>> >> >> > Dbmax and Dbmax_shuffle into
> >> >>>> >> >> > 10 bins, respectively (same bin edges or same
> > fractions)?
> >> >>>> >> >> > 4. Your correlated background gamma is calculated for
> > the
> >> >>>> >> >> > Dbmax bin where Dbmax is from the charge-shuffled
> > events,
> >> >>>> >> >> > but using restored charges, right? If so, then you're
> >> >>>> >> >> > effectively taking gamma difference between Dbmax_i
> > events
> >> >>>> >> >> > and Dbmax_shuffle_i events (which are different
> > events),
> >> >>>> >> >> > right? Of course you've also removed the large
> >> >>>> >> >> > charge-shuffle background which is basically an
> >> >>>> >> >> > autocorrelation effect (sort to
> >> >>>> >> >> > speak) due to the Dbmax (and Dbmax_shuffle) selection
> > bias.
> >> >>>> >> >> > 5. You divide Dbmax (and Dbmax_shuffle) into 10 bins
> > and do
> >> >>>> >> >> > your analysis in each bin separately, and then take the
> >
> >> >>>> >> >> > weighted average for your f_cme result. You could just
> > use
> >> >>>> >> >> > a single wide Dbmax (and
> >> >>>> >> >> > Dbmax_shuffle) bin, then in principle you should get
> > zero
> >> >>>> >> >> > signal because the correlated "background" is your real
> >
> >> >>>> >> >> > signal since they are now identical event sample. So is
> >
> >> >>>> >> >> > your finite signal really due to the difference between
> > the
> >> >>>> >> >> > average of ratios and the ratio of averages (or perhaps
> >
> >> >>>> >> >> > also due to residual effect from
> >> >>>> shuffling)?
> >> >>>> >> >> >
> >> >>>> >> >> > This is a complicated analysis. It would be really good
> > to
> >> >>>> >> >> > have more discussions so the details can flesh out
> > better.
> >> >>>> >> >> >
> >> >>>> >> >> > Thanks,
> >> >>>> >> >> > Fuqiang
> >> >>>> >> >> >
> >> >>>> >> >> >
> >> >>>> >> >> >
> >> >>>> >> >> >> -----Original Message-----
> >> >>>> >> >> >> From: Star-fcv-l <star-fcv-l-bounces AT lists.bnl.gov> On
> >
> >> >>>> >> >> >> Behalf Of jagbir via Star- fcv-l
> >> >>>> >> >> >> Sent: Tuesday, November 17, 2020 10:49 AM
> >> >>>> >> >> >> To: ShinIchi Esumi
> > <esumi.shinichi.gn AT u.tsukuba.ac.jp>;
> >> >>>> >> >> >> STAR Flow, Chirality and Vorticity PWG
> >> >>>> >> >> >> <star-fcv-l AT lists.bnl.gov>
> >> >>>> >> >> >> Subject: Re: [Star-fcv-l] FCV PWG meeting, 18/Nov/2020
> >
> >> >>>> >> >> >> (Wed) 9:30am (New York time zone)
> >> >>>> >> >> >>
> >> >>>> >> >> >> Dear ShinIchi, Prithwish and Jiangyong,
> >> >>>> >> >> >>
> >> >>>> >> >> >> I would like to give "Update on event by event charge
> >> >>>> >> >> >> separation in
> >> >>>> >> >> >> Au+Au collisions at 200GeV with STAR detector"
> >> >>>> >> >> >>
> >> >>>> >> >> >> Please add me to agenda.
> >> >>>> >> >> >> I will post my slides later.
> >> >>>> >> >> >>
> >> >>>> >> >> >> Thankyou,
> >> >>>> >> >> >> Jagbir Singh
> >> >>>> >> >> >>
> >> >>>> >> >> >> On 2020-11-16 15:57, ShinIchi Esumi via Star-fcv-l
> > wrote:
> >> >>>> >> >> >> > Dear FCV PWG colleagues We will have our weekly FCV
> >> >>>> >> >> >> > PWG meeting on coming Wednesday
> >> >>>> >> >> >> > 18/Nov/2020
> >> >>>> >> >> >> > 9:30AM (in BNL) at our usual time and place. So if
> > you
> >> >>>> >> >> >> > have anything to present, please let us know and
> > please
> >> >>>> >> >> >> > post your slide by
> >> >>>> >> >> Tuesday.
> >> >>>> >> >> >> > We'll talk about the "HLT express productions" in
> > the
> >> >>>> >> >> >> > beginning of the meeting as you see in the agenda
> > page.
> >> >>>> >> >> >> > Jiangyong, please send a link to your slide from
> > last week.
> >> >>>> >> >> >> >
> >> >>>> >> >> >> > The zoom room link, ID and password are in our usual
> >
> >> >>>> >> >> >> > drupal agenda page below.
> >> >>>> >> >> >> > Please also keep in mind that all the preliminary
> > plots
> >> >>>> >> >> >> > should have already been there in the summary area
> > below.
> >> >>>> >> >> >> > Best regards, Jiangyong, Prithwish and ShinIchi
> >> >>>> >> >> >> >
> >> >>>> >> >> >> > Meeting agenda page with zoom link :
> >> >>>> >> >> >> >
> > https://drupal.star.bnl.gov/STAR/blog/jjiastar/bulkcorr
> >> >>>> >> >> >> >
> >> >>>> >> >> >> > Preliminary page :
> >> >>>> >> >> >> >
> > https://drupal.star.bnl.gov/STAR/pwg/bulk-correlations/b
> >> >>>> >> >> >> > ulkco
> >> >>>> >> >> >> > rr-
> >> >>>> >> >> >> > pre
> >> >>>> >> >> >> > lim inary-summary
> >> >>>> >> >> _______________________________________________
> >> >>>> >> >> >> > Star-fcv-l mailing list Star-fcv-l AT lists.bnl.gov
> >> >>>> >> >> >> > https://lists.bnl.gov/mailman/listinfo/star-fcv-l
> >> >>>> >> >> >> _______________________________________________
> >> >>>> >> >> >> Star-fcv-l mailing list Star-fcv-l AT lists.bnl.gov
> >> >>>> >> >> >> https://lists.bnl.gov/mailman/listinfo/star-fcv-l
 



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