WEBVTT

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Yeah, I think now was successful, but I know you hear me you see me and you see my slides.

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All work and actually you managed to go for what I might worry because sometimes this crashes, so I think we're probably ready to start building the people.

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So, this is what was needed. This is a green light to start. Okay, so we start the next session of the workshop, and we'll start with the young trying to demystify the mother is fed by media channels so police younger is a prime and the Ester.

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Exactly.

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You're already looked into my slides. Yeah, thanks a lot for having me here.

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I will tell I mean, I will give you a bit of a logical perspective on dark matter and well try to motivate a little bit that if you're looking to teach Hello mediators met searches are probably not the way to go.

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At the LSC but that is very likely actually that we might see along with particles at the LSC when we talk about dark matter now. Yeah, exactly. This is the channel entity channel mediator models.

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Now I think in general, dark matter is one of the main motivations I think for for looking for new physics. And although they are of course plenty of ways to couple dark matter to the standard model.

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The way these searches word interpreted by the OC collaborations were mainly in terms of simplified models where you really look into the low energy.

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degrees of freedom of certain theory. And look, and they're basically these two options and as channel and teach no mediator, and a teacher the mediator in particular is very interesting because it has a quite rich phenomenology.

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And although you typically might think of it as I said as some low energy.

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degrees of freedom have a more complete theory and principles these models are consistent in the way that they are normalized double gage series where you can write down a master of and everything is fine principle.

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Now in the emphasis of what what you basically do is to introduce a documented particle and some, some partner that is also on the xe to a cemetery that stabilizes dark matter and here we have the Susie example where you

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think earlier, come as a s dark matter and a scalar cool partner as the mediator that you would have this you call the type of direction that you see down here in in in the MSM this coupling would be given by the gauge coupling which is of course not

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the case in general, also in the extension to the MSM. This might be free parameter.

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Now, some time ago, people started to study these kind of moles and more systematic way, for instance collaborators mine, who really went out and studied all the different spin assignments and coupling to the various generations, of course, and studied

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the constraints on such models.

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If you really take these low energy degrees of freedom, as all that there is relevant for the cinema algae and do the reluctance to computation indirect and direct detection constraints.

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And look what actually remains, and it's surprisingly little that remains so here's the case.

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Off the Susie like teacher mediator model, where you have this Marianna fermion talk met her, and a scalar mediator and this is promised space in terms of the Dark Matter mass and the relative mass but in between that mediator, and dark matter and the

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gray shading is here the coupling that you would need to get the right Radek density, um, and you have several constraints, do you see shockingly few little spot that are still allowed and these unfortunately are not ready, very much in the reach of LSC

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so yeah so you might think it's a good idea to look for these models at the OC at all. And it's even worse if you look into other choices for instance if you're looking to non self conjugate dogma, better, then you see actually that all of the parameter

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space was the size of a coupling so in the wimp region is actually excluded by all the searches. Without the LSC already.

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However, there's this white spot. Down here which for all, all of these models is actually untouched by all these constraints. And you might wonder what happens there so technically the couplings should be very small in this region so let's see what happens

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there and to understand this let us very briefly just review. I mean, what what happens what what what is actually the dependence of the relic density on this coupling Lambda Chi that I introduced.

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So in the usual freeze out scenario that all of you probably know where you have large couplings.

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You have just this animation of dark matter that governs erratic density so the reg densities, just inversely proportional to some power of the coupling.

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However, depending on the mass splitting between the mediator and that dark matter particle.

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Actually significant contribution for media to pan elation or this coalition.

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Can, can play a role in in the freezer so this could have actually bounced down and in the case of sufficiently small couplings. It's just a mediator panel ation that is important in the early universe and in this case, the rate of density is actually

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not dependent on the coupling anymore. However, if you reach a certain smallness of this coupling another process is actually important, which typically is assumed to be efficient but it's not for very small companies, namely the conversions between dark

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matter and this mediator particle. And once these conversions are not efficient anymore or at the edge of being efficient, they can actually initiate the breakdown of chemical even so they can actually govern the freeze out and that's a distinct freeze

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up mode which we call convergent or freeze out or co scattering.

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And that's another film illogical distinct region. And if you want to know where they sit so I mean, you can have probably already guess.

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But let me just just show you this this curve again for some particular mass point and the density that we measured Oh point one two, If they end up like this.

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You clearly find this wimp solution for the dentist so you were basically sitting here. However, if the curve looks like this so for another point in the mass parameter plane.

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You may find a region here and this is exactly in this white region down here with a get or solution for the roof is density for this conversion.

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And you might also be at this plateau which is which corresponds basically to this boundary here whether coupling actually drops by orders of magnitude.

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Why is it important for the LSC now, because it this converter and frees up really predicts long with particles at the LSC with typical life times or decay links of, basically.

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Wow. millimeters two meters so roughly a few centimeters typically, and that's because if conversions should be up the order of the huddle rate, which means that they are in the edge of being efficient, and the decay is, which are just one part of the

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conversions should be of the order of the Hubble rate or smaller. That means the decay length is off the order or larger than the inverse have a rate which you can translate actually into a centimeters for typical freezer temperature so for these test

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scale particles that we can prob at the LSC we naturally have these particles and that's why you know all these white spots.

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The way to look into is long as particles. So there's one more thing to the story, namely, there's been recent progress in the radio testing computer, meaning that we further look into bounce data effects that are I mean, known to be potentially important

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in these sorts of models because you have this colored mediated particle and they can form bound states however for this very small mass gaps so in this converting them from that region, you have a prolonged freezer process, so it's not an instantaneous

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so this bounce state effects are actually super important there. And while you can, of course, read, read our papers is very interesting but I mean the upshot and what is important for us here is that the region where you have this basically this this

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And this is the dark matter, mass. So this region here is actually pretty much enhance so this is the just performative computation for this boundary between the wind bridge and the convergence room freeze up region.

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And this is actually the, the solution if we take into account bounce states and even excited bout states.

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So, this endpoint in particular, goes from to one point say three or so TV two for TV. So, yeah, there's quite large rate.

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Yeah, the minutes, three minutes. Okay, thank you. So how would you look into these long with particles at the LSE so here in this case it's called a park that could be produced.

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They could typically decay inside the detector into a soft jet engine in dark matter. And here I would like to highlight that this is a soft ish jet, that, that, and the signature somehow falls a little bit into the between the typical targets that I'll

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look for it the OC so typically you either look into something like splits to see where you have a heart and from from us a gluey know that then the case and to read to lead hard jets in a displaced vertex, or you look into something like a charge you

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know that the case into a super soft Python like hundreds of MeV just and missing energy, but this is something like the soft chat has something like typical energy of this delta and so say 2040, maybe 50 GV.

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So this actually found that neither the displaced vertices search nor the disappearing track searches really tired to this kind of scenario those This is.

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Well, this is basically what comes out if you look into this teach animals and of course once in a while, depending on the lifetime It could also trigger us all off the detector and so gives us, highly ionizing tracks, and this is the current LP constraints

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that we examined here for. I mean, for very small mass lettings, so this is the bottom partment so if it's below the bottom threshold there this too buddy the case of press so here we really have detect a stable particles, we can directly integrate the

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art and searches for these kind of searches, here we had to reinterpret them and this is

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what we would call disappearing tracks. And today's vertices searches actually suffered a lot from an invariant mascot that was a post that experimental setup that basically killed our sensitivity for this rather softish jets.

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Yeah, so there's still quite some room to be explored here.

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Okay, I think my time is up, I just want to flesh of course I mean this this pain, this this this 1.4 TV.

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Heavy saver chock full particle access, with a mass 1.4 most likely, which of course fits very well here principle and you see also the importance of these effects.

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But I mean, we have discussed this on Tuesday.

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Clearly there's something that that points to maybe something more weird than that but I just wanted to flesh her, I mean that that in principle from from the cross section that we expect here, this would fit very well, if only one would see it in the

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time of flight measurement so very, very briefly my summary so the abstract is really that teach have a mediator models.

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The wind per hour to space almost excluded the remaining region is to convert from freeze up region which is less explored, but gives us really as a prediction, not just in some corner of it, along with particles that the IC, which can be looked for,

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and we've seen that these bounced at factor, actually, largely enhance this region, where we expect LPs and the kinematics differ from the one that is currently looked into it so the targets, either split Suzy, or charge he knows that he came to a very

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soft pie on this. This may be something that could be looked looked into more dedicated. Okay, thank you very much for your attention.

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And sorry for being probably going over time.

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Thanks again for they started say I think one means pay, and then we open the floor for questions.

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Okay, so let me ask Michael something so you said that they, although they signature wise, you would say ladies are beaten track should work. There's a cut in there where they say making the search not very effective for your setup.

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And now they've you look into the separate track before because probably the cat is removing some unwanted background so it somehow clear from a naive estimation that if you remove this card, then you will gain sensitivity or is really the way the recipient

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that can give you know this this is this place purchases, so the the game here. This is the displays versus surgery and while we made this exercise, maybe you even remember that because we discuss it at some point.

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So the thing is that actually both our signal is in that region below this TMGV.

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Cut.

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So we, I mean if you we were able to completely remove this cut, we would actually gain I think two or three artists of magnitude in our signal. So this is, I think worth looking to of course there's a reason why it was placed in the first place.

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However, as far as we could see, there's not really much background so you can easily put it down to five gv as far as I understand you could of course also play, because I mean you put it there because you want to get rid of background from be the demons

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and stuff like that but you could of course play around with having a slum what tighter cut on on the displacement so require slightly larger displacement but reduce that delta that variant mascot I think this is some things worse playing around with

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so what what we've seen from Sigma point of view, this is really what kills the signal in this case.

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And I don't have the plot here but I mean the the sensitivity was really I mean, if you would remove it. I think that the sensitivity would be something like here.

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And without it's basically, it's hidden here.

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And I get it. Okay, okay. Thank you very much.

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So, in the off time, move to our next speaker, we send you again. Thank you.

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We have under.

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Hi, can you hear me. Yes loud and clear. Can you try to share your screen. Absolutely.

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While when you can stop sharing yeah I just have to get them because I got rid of the, I think, here, here it is right.

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Here we go.

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Can you try now. Yes, I can.

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There we go. Can we all see this looks fine yep perfect so can you try to go back and forth One. One. Perfect.

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Okay so without further ado, now are the different to take that tell us about the elastic that mother, delicious. Please go ahead. I let you know when you have two minutes list.

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Perfect. Thank you, so I'll be discussing recent study we've just completed regarding inelastic dark matter in the context of future propose experiments are the NFC.

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So brief overview, basically we try and do our best to survey the landscape.

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Basically utilizing a few of the proposed to take the geometries, some of which have been discussed this week.

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In the context of a standard inelastic. Dr. setup will be extinct some work. That's previously done by Felix clean and collaborators in the sense of a beta detector parameters as well as just new experiments, being proposed as they come online.

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And so, he was saying that this sort of setup led to suppress Dark Matter nuclear couplings.

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And so this can help us start to evade detection expect direct detection constraints which are currently getting very strong for the war coronations in the early universe can determine and set the relic abundance, which is then at later times suppressed.

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And so we can seem to tenuously evade stringent SMB constraints while also producing a stable thermal thermal relic which we denote.

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One other inventively.

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And so they're relatively like me later. He's been required to explain that the dark matter abundance by a standard thermal freeze up processes.

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And when we choose is the course I suppose the standard duck photon.

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And so, to set up our model we consider a Dark Sector containing, as I mentioned, to almost a generic mistakes coupled through a dark photon mediator, the strength of which is given this term here by a kinetic mixing parameter epsilon.

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And so, we consider a couple of cases, first week to the fermion iq states, and so we have majorana fermion with a vertex coupling to that point on like this, we consider a staircase.

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And of course, the relevant vertex for a phenomenology is going to be how our states couple through this stock photo to the standard model, given Mike so and so, I've highlighted.

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Our kinetic mixing here which will be eventually what we can stream, as a model parameter.

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The next parameter of interest is going to be this term delta which is basically proportional to the mass bling, where I've hired the mass of the ledger state, so I'll stay we'll talk about a candidate.

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And this is going to be the other model prominent we can strength. Okay. So, epsilon. And one of the premise of interesting.

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Okay so production. The dominant production, because through drug in through some, is it bows on order photon into our elastic states here.

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This heavier state Chi to then propagate off, and then probably the case through, you know not show on shell.

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Duck photon into some semiotic final states which should hopefully be picked up by our detector.

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Okay, just going into the, into some detail here about how we conduct the analysis, it's a very straightforward analysis. Of course the main ingredient is going to be the expected number of signal events, we expect to see.

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And this is of course proportional to the production cross section of our colon cartoon states from Protein Protein collisions, multiplied by some integrated luminosity.

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And some parameter, which is called f signal, which is basically the expectation of detector efficiency multiplied by the probability of our heavy inelastic state decaying within the detect the volume.

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And so functionally we. This is computed by averaging over all of the possible kinematic configurations of our heavier state using my graph.

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So, again, getting slightly more into this. The, the piece of interest here this probability is given by this combination of exponential terms here.

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Of note is this Elba, which is just the expected expected decay length, which is of course inversely proportional to the decay with the process.

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This entry and exit here are just simply the entry and exit points of our detective volume, assuming the longest particle, basically, travels from the interaction point straight to the detector doesn't again.

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And so schematically, the little picture here.

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We calculate this entry and exit by simulating Monte Carlo realizations about decay process and then determining the three momentum trajectories, like so.

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Furthermore, the other kind of important thing to note is we impose them a detective dependent energy cut on these final state fermion here, which is just the total cut on the total visible energy of the particles.

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Basically, preparing for any, you know, detect energy thresholds that we might have in the future, and discuss a little bit about that later.

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So that's a schematic set up.

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Okay, so as far as the experiments we consider, he's a cartoon.

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So, a bunch of these as I mentioned have been discussed at length this week, so facet could xB map map one and two fazer a nervous and Alex here.

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Matt one and two fazer a nervous and Alex here. As far as the numerical input implementation of these geometries we took.

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Basically the most recent and up to date values we could find in the proposals in the literature and implemented as best implemented them as best we can.

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Okay, keeping things. Moving on to some results. So here we have the forecasted 95% confidence interval limits on the Munich case.

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Basically these contours correspond to Apple for some fluctuation of three events.

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In the absence of any significant background contribution.

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We have four benchmarks, corresponding to different values of the escalating parameter Delta, and the ratio of the photon last to the latter.

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The particle mass here.

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And so, as we can see, the colored contours correspond to the predictive sensitivities in each of these experiments, we can carve out quite a significant chunk of the currently on unexplored premier space yet, which is nice.

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The Alex detector being, especially

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good, which was interesting to see some things to notice the focus and sensitivities move to higher valleys of the kinetic mixing and the mess. When we decrease our message letting him by an order of magnitude.

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This is basically due to the fact that the decay with goes as basically this delta to power five and so to produce the same number of particles, we need to increase the coupling strength and the mass.

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So this was expected.

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The gray regions correspond to current experimental constraints on the dark photon.

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And finally, just for completeness we include a contour, this black line here and each of these plots that correspond to the case where the staple dogmatic candidate the sky one saturates the observed from the commandments.

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So, for the scalar case, we found, basically the same result. And so, just for demonstration we we plot the first benchmark here.

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This could pretty much be explained by the fact that the decay length for the scale and the firm on a case were observed to be approximately the same.

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And so this was somewhat interesting, but pretty much expected.

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Somebody else we observed was the effect of changing this energy cut that we imposed for stage detector.

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And so what we've done here on this plot is we show the case for, who's learned and phase two.

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And this is just basically done to demonstrate examples of an off axis, compared with a foreword detector.

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And so we can see that changing the energy threshold by gv and the food labs and off axis type proposal could actually significantly change the forecasted sensitivity, something that we certainly didn't appreciate before doing this.

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And that's it short, sharp and shiny thank you very much and we open the floor for questions.

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Okay, if another will I will use my chair by was to ask you something so it's just a curiosity maybe they look into it. I think you have a guide to the K two k one FF bar for interesting moto certain quality or whatever, they should differ from the let's

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the let's say normal range bar of a scalar became to FX bar because of the city very gay so you will see one of these guys, but they will look not really looking like this scalar the game, so I don't know if you look into sort of some body levels of the

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Barbie case in case you say, if there's a signal I should be able to say, this looks more like an elastic their mother ran a scalar became or no no we didn't, but this is certainly a good idea, and a good proposal to look at.

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Now I was just curious, you know, because at some point we will see things and we need to correct the horizon so not keep doing. We is crucial blocks.

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Okay, so let me see someone else. In the meantime, God inspired to ask a question since it doesn't seem to be the case.

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We think Andre again and now we move to Nathan going to tell us about some quirky stuff.

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Yes. Hello.

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Hello. Can you try to share your slides. Yes.

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Okay, perfect. So, please go ahead and I will let you know when you have three minutes left.

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All right.

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All right.

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Hello, my name is Nathan Sorry, I am a student Caltech, I am currently working at the Lauridsen laboratory for high energy physics and today I'll be talking about my work on a standalone search for court pair production with timing detector at the highly

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me la seat.

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Now, to begin let's actually go into what quirks are so quirks are actually heavy, they proposed heavy stable charged particle, a Dark Sector analog to standard model corks that are connected by flux tube of dark blue ones.

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Now they're actually probably understood quirks are let us go through a little thought experiment. So in the Standard Model q CD case, the mass of the cork is much less than the dark, sorry the confining skill of ci CD.

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However, in the dark or cork proposed juicy case, the mass of the work is much greater than the dark confining scale. So what are the actual implications of this.

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So in the Standard Model case as we all know, the flux tube of glue on breaks and the leads to radiation into lighter quirks. However, stable quirks do not have any lighter states that maintain quantum numbers, therefore the flux tube of dark gluons does

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not break. As you can see here at the bottom, and this actually causes macroscopic also little emotion and eventual annihilation so very striking signature in deep.

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So, the actual search regime that we are looking at is in this lambda dark or the dark confining scale between 100. electron volts to 10 kilo electron volts.

00:30:29.000 --> 00:30:44.000
This correlates to an oscillation amplitude on the order of point one to 10 centimeters. This is like search currently constrained by the Jets plus match search, but as we know, in general, any current searches are limited by standard trigger acceptances

00:30:44.000 --> 00:30:49.000
therefore, the use of any additional kinematic data may improve our reach. As we will see soon.

00:30:49.000 --> 00:31:04.000
So what actually are the court dynamics, or what is the nature of the kinematic nature is of the trajectories of these very unusual particles. See the alert, sorry the linked quirk anti four pairs oscillate while moving outward or from an initial collision,

00:31:04.000 --> 00:31:17.000
as we can see you're on the right now the interaction with the inner detector does not change the angular momentum of the court system. So this actually leads to the courts, having not only under solitary motion but a planar oscillation.

00:31:17.000 --> 00:31:26.000
And as we know, current reconstruction algorithms are designed to look for helical trajectories. However, with these planar oscillations with quirks.

00:31:26.000 --> 00:31:40.000
They don't really work that much that well so with the current reconstruction algorithms are not designed to handle this very striking signature. However, a full redesign of the current reconstruction algorithms do handle the his system is unfeasible,

00:31:40.000 --> 00:31:47.000
therefore we try to look for indirect methods of probing a, the court systems, and the cork signal.

00:31:47.000 --> 00:32:03.000
So this is what leads us to our first or third strategy of time delay. So, in this case time delay refers to the difference between a particle in this case that court, reaching a specific region of the detector.

00:32:03.000 --> 00:32:16.000
So difference between that and a liminal particle. So on the left we see a little schematic of the in black the course trajectory and an orange as a liberal particle going straight from the interest of the interaction point.

00:32:16.000 --> 00:32:23.000
Now the background the Standard Model background, generally have some distribution peak that zero with some small spread.

00:32:23.000 --> 00:32:34.000
But the quick signal is expected to have time delays, greater than or on the order of one nanosecond so already quite a distinct from the Standard Model background.

00:32:34.000 --> 00:32:43.000
And this is because quirks are as we mentioned earlier these oscillating heavy masses, which are going to travel slowly and reach the point in the detector.

00:32:43.000 --> 00:32:47.000
As you can see on left much slower than just.

00:32:47.000 --> 00:32:55.000
So how are we actually going to look at the timing layer, or how are we actually going to pro time delay as a discriminate.

00:32:55.000 --> 00:33:12.000
Fortunately, CMS of my law actually is a collaborator on this is designing a minimum ionizing particle timing detector layer, which is a four millimeter timing detector layer proposed between the tracker and he Cal region, designed for charged particles.

00:33:12.000 --> 00:33:27.000
It is currently currently both a proposed timing and resolution of 30 Pico seconds for note the BTL region or the barrel timing layer is using Lysol crystals activated with serum read out with silicone photo multipliers, and the ATL or the end cap timing

00:33:27.000 --> 00:33:34.000
layer uses radiation tolerant silicone sensors with game known as l guts.

00:33:34.000 --> 00:33:49.000
So, before we actually get into the, the time delay study we actually need to generate the cork Monte Carlo simulations. So to do that, as I mentioned earlier, there are two free parameters in the court model the mass of the cork and the dark confining

00:33:49.000 --> 00:34:00.000
scale so my simulations are done in a scan of this parameter space, the mass of the court going from 500 gb to 2500 gb and lend the dark going from 100.

00:34:00.000 --> 00:34:14.000
electron volts to three kilo electron volts, the actual model used with my graph is VOQ underscore UFO, which is an extension of standard model of the standard model with vector like top partners, as I mentioned earlier quirks, are these vector like for

00:34:14.000 --> 00:34:29.000
these PVC will charge particles, so we can actually use this T type court in this model as a proxy for quirks. Now the samples are generated with zero to one extra jets and the cork evolution is done through a self made code base, and at right we can

00:34:29.000 --> 00:34:46.000
Kirk sample Kirk trajectories from the simulations, showing the characteristic of dilatory motion. Now this actually gets us into the time delay investigation. So here we actually see the time delay distributions for the BTL region.

00:34:46.000 --> 00:35:02.000
So the BTL being the barrel timing layer on left we see the hundred electron volts case for lambda dark and mass of the work being 1000 GV and on right we see three kilo electron volts for the lambda Dart, and the 1000 jeebies for the mass of the cork.

00:35:02.000 --> 00:35:16.000
At the bottom we actually see the topology of the event. So for the hundred electron whole case, you have the larger versions of these oscillation amplitude, as the court kind of moves out from its original

00:35:16.000 --> 00:35:32.000
production point, and at right, we have actually interesting enough, the three kilometres from the highlands at our region has small oscillation amplitude, and to actually reach the BTL later you actually need to have the pair system recoil off of jet.

00:35:32.000 --> 00:35:50.000
So in the hundred EV case, you're going to have the time delay distribution peaked at two nanoseconds. And in the right case you see the time delay. Being approximately 17.5 nanoseconds again because courts are these heavy oscillating particles.

00:35:50.000 --> 00:35:54.000
That's why you have this larger time delay, even in the three kV region.

00:35:54.000 --> 00:35:57.000
When it's requiring have a job.

00:35:57.000 --> 00:36:09.000
So the BTL region actually yields greater time delay statistics in the low lambda dark region as we see compared to the hundred EV or the art sorry as, as you compared to the high.

00:36:09.000 --> 00:36:13.000
Sorry, the high lambda dark region of three kill electron volts.

00:36:13.000 --> 00:36:25.000
So to actually compare it to the ATL region. Here are the distributions at left again we have the hundred EV case, and it right the three kilo electron both case of the time delay is approximately the same order of magnitude.

00:36:25.000 --> 00:36:36.000
With time delay being a 2.5 nanoseconds on the left, 12 nanoseconds on the right. Note that the ATL yields greater timely stats in the high land the dark region.

00:36:36.000 --> 00:36:48.000
However, the overall time delay is, as you saw on the previous slide, higher in the, The, the right plot with the BTR region.

00:36:48.000 --> 00:36:57.000
So now that we actually understand or saw some timely distributions, we can go into the actual, the numbers and numeric the quantitative measurements.

00:36:57.000 --> 00:37:11.000
And here is the actual geometric cut. So these are the acceptance is used to make the previous slide, where we're requiring least one court to reach the specified layer I do the BTL or ATL after a center of mass on greater than 12.5 nanoseconds.

00:37:11.000 --> 00:37:23.000
So as we can see the general trend of this table is that higher court masses yield lower signal efficiencies, with the exception being the low lambda dark region and in general upholding the trends from the previous two slides.

00:37:23.000 --> 00:37:32.000
The BTL region is better for probing the lambda lambda dark region and the ATL is better for probing the high lambda darker region.

00:37:32.000 --> 00:37:46.000
Now, now that we actually understand the acceptances we can actually try to implement a kinematic cut here we apply a timing cut of three nanosecond time delay a cut off, apply to all events passing that geometric acceptance on the previous slide.

00:37:46.000 --> 00:37:55.000
So, here the BTL region, maintains more signal efficiency or sorry the general trend is that the BTL region maintains more signal efficiency, after the timing cut.

00:37:55.000 --> 00:38:09.000
But in general, we actually do achieve high efficiency, high signal efficiency greater than 95% for both the BTL and ATL regions for lambda dark being greater than or equal to a 25 ev a general.

00:38:09.000 --> 00:38:23.000
As I previously mentioned the ET the BTL region does maintain more signal efficiency, especially above masses of 1000 GV, but that's not to say the ATL is poorly performing.

00:38:23.000 --> 00:38:38.000
So, this search of actually looking at court systems, represents a departure of simply probing the electronic breaking scale, and moving towards looking at, unique, or striking signatures that are potentially observable at the Elysee, but are currently

00:38:38.000 --> 00:38:45.000
miserable because of differences in our workflow, especially in this case the reconstruction algorithms.

00:38:45.000 --> 00:38:59.000
Cork trajectories in this project were successfully simulated and the signal events were generated using mad graph time delay actually proved to be valuable discriminate for the court signal motivating the use of the MTD both the BTL on ATL separately,

00:38:59.000 --> 00:39:08.000
separately, as we saw the BTL proved more effective improving the low lambda dark regime, while the ATL proved more effective, improving the Highland the dark regime.

00:39:08.000 --> 00:39:21.000
Currently we are exploring plane fitting seated by timing hits as an additional discriminate. Playing fitting, naturally, is a pretty obvious idea, as I mentioned earlier court systems have these planar oscillations.

00:39:21.000 --> 00:39:36.000
Therefore, it is natural to try to consider a plane fitting aptitude approach. We are also currently determining and generating possible backgrounds to the court signal for the timing investigation that would most likely be a soft QCD simulation with

00:39:36.000 --> 00:39:51.000
a finite MTD timing resolution. And then we want also like to expand the analysis into investigating other court signatures. So currently we're only looking at courts produced through Julian processes, which allows us to have these center model electric

00:39:51.000 --> 00:39:53.000
charge.

00:39:53.000 --> 00:40:07.000
And that allows us to use the MTV which is requires us use charged particles, but if we are clever we can potentially expand the analysis, into other cases, maybe even using like plain fitting aptitude example to look at the other production methods such

00:40:07.000 --> 00:40:11.000
as the colored cases from CCD or even one charge one neutral.

00:40:11.000 --> 00:40:12.000
Thank you.

00:40:12.000 --> 00:40:13.000
Any questions.

00:40:13.000 --> 00:40:21.000
Thank you very much. Listen. So yes, actually we open the floor for questions so in James has a question. I know Mike has a question please mind go ahead.

00:40:21.000 --> 00:40:34.000
Yeah Hi, thanks very interesting, but I have a question, but presumably the quirks will they got electric charge and there'll be radiating photons right and and going.

00:40:34.000 --> 00:40:40.000
And if one is annihilated the other ones got benign at the same time, I don't quite understand what's going on there.

00:40:40.000 --> 00:41:00.000
Oh, I guess, so do you mean, are you asking about like the topology the event or. Well, as I understand it, the quicks charged the the end of the string of this string of dark clouds right right as Gosh, as they, as they are oscillating and turning around

00:41:00.000 --> 00:41:04.000
the end, there must be radiating photons because charged particles. Right.

00:41:04.000 --> 00:41:17.000
Right. So that will they will cascade down and then annihilate presumably on each other right. Okay, so I'm not, Mike, Mike, they don't need to let their photos they they so they could be elected.

00:41:17.000 --> 00:41:31.000
They could be St Charles where they could only be called or a chance if you will not under under a new, they could be totally cinema and neutral and charged under the new sort of dark QCD of model building if you want.

00:41:31.000 --> 00:41:32.000
Okay.

00:41:32.000 --> 00:41:43.000
Could they radiate not protons as their accelerated at the end of the day, could maybe not the most common model that because it's the next question, so I let him comments.

00:41:43.000 --> 00:41:58.000
I'm just gonna, I mean, there's a there's a whole slew of different types of objects here so I think there's no real one size fits all answer to my question but generally these particles take a long time to annihilate because the amount of radiation compared

00:41:58.000 --> 00:42:06.000
to the mass is so small. So, on the timescale that this speaker is worried about the annihilation it's not an issue.

00:42:06.000 --> 00:42:20.000
But, but I do think it's worth keeping in mind that because they're all these different types of objects that there are some risks with plain fitting in that, you know, that'll work for some models but a lot of models that won't.

00:42:20.000 --> 00:42:29.000
Whereas, you haven't mentioned ddx, which works for why classic models and I wonder whether you, whether you're planning to sort of incorporate that.

00:42:29.000 --> 00:42:30.000
Yes.

00:42:30.000 --> 00:42:38.000
Yeah. Yeah. I didn't mention it, but that is a potential direction that we are looking into.

00:42:38.000 --> 00:42:40.000
Thanks.

00:42:40.000 --> 00:42:43.000
So Simon.

00:42:43.000 --> 00:42:59.000
Yeah, I met just commenting on the ddx, this is something that when we were looking at the plane flooding back in the day.

00:42:59.000 --> 00:43:10.000
Because you end up picking up the particle at a particular point and a picture of velocity. And so you got a really wide distribution for these things at least for these sort of very broad trajectories.

00:43:10.000 --> 00:43:14.000
And it didn't end up sticking out much about the background.

00:43:14.000 --> 00:43:23.000
Now if the if the cork is very narrow right so then it should it should work very well.

00:43:23.000 --> 00:43:31.000
But that was just like, you know, theories level study back in the day so it might be worth revisiting.

00:43:31.000 --> 00:43:32.000
Makes sense.

00:43:32.000 --> 00:43:46.000
Hey thanks for the comment. I see no further questions or comments, or concepts or we stagnate, we move to fall.

00:43:46.000 --> 00:43:48.000
Yes. Hello.

00:43:48.000 --> 00:43:50.000
Hello.

00:43:50.000 --> 00:43:56.000
We see you, the time to share your slides.

00:43:56.000 --> 00:44:03.000
So, The words.

00:44:03.000 --> 00:44:17.000
And let's see if we can go one for what I want my work. Perfect. So without further you see them changing. Yes yes fantastic so please go ahead and tell us everything about just a little piece.

00:44:17.000 --> 00:44:21.000
They have been discussing meeting.

00:44:21.000 --> 00:44:23.000
Yes.

00:44:23.000 --> 00:44:40.000
So, hello everyone my name is Alma civic I'm a PhD student at the University was so. And today I would like to present you results of the recent study we did together Bahama Delta cash Korean Columbia, see Kimmy so in Kazuki saccharine if you'd be interested,

00:44:40.000 --> 00:44:44.000
then you can find the prep in an archive.

00:44:44.000 --> 00:44:58.000
In our study we wanted to answer the question whether LPs can be discovered that Elysee doing ground three and highlighting the case. And we decided to concentrate on longest particles that are moved to be charged by want to be charged, I mean that the

00:44:58.000 --> 00:45:05.000
electric that they are electrically charged, and the magnitude of the charge can be up to several times.

00:45:05.000 --> 00:45:10.000
Magnitude of protons charge or electrons.

00:45:10.000 --> 00:45:18.000
Now, In our study we requested analyzes for three experiments Atlas CMS and metal.

00:45:18.000 --> 00:45:31.000
And we considered to production most of both open and closed on a production, whereby close channel, I mean, formation of petroleum like bounce states.

00:45:31.000 --> 00:45:40.000
And we hope that aimed at obtaining lower must bounds, that these three experiments could provide and the at the end of the day that they can do it.

00:45:40.000 --> 00:45:49.000
So there are multiple scenarios that predict existence of multiple charged particles, and in some of them. These particles can be long lift.

00:45:49.000 --> 00:45:55.000
In our study we want it to be very general model independent.

00:45:55.000 --> 00:46:09.000
We considered particles with charges from one to eight times elementary charge that were four times, so we considered particles will spin zero and half that were either close singlet or triplets.

00:46:09.000 --> 00:46:12.000
They were always as you do single it.

00:46:12.000 --> 00:46:26.000
And we added them on top of the standard model, but since we wanted to stay as model independent and general as possible. We didn't like specify the, how they will will decay.

00:46:26.000 --> 00:46:36.000
Rather we treat them as collider stable. In case of adolescence TMS, or we parameters the decay length for metal.

00:46:36.000 --> 00:46:49.000
But how these particles can be produced. Well, there are several processes, there is an S channel on production there was a photon fusion fruity channel or four point interaction vertex.

00:46:49.000 --> 00:46:56.000
And in case of color tripping particles. We can also have a glue and glue on and gum my view on the fusion processes.

00:46:56.000 --> 00:47:09.000
On the next slide you can see the composition of the section for an example particle called family on with one TV mass. Here is on x axis you can see charge of the particle on y axis cross section.

00:47:09.000 --> 00:47:19.000
And from this broad, you can see that wire for small charges, we can blow on the vision for that.

00:47:19.000 --> 00:47:31.000
And its dominant.

00:47:31.000 --> 00:47:50.000
I speak about it because so far experimental searches interpret the results, only for Julian processes. However, I heard a very interesting talk by Mr Smirnoff two days ago, about an ongoing Atlas analyzes where they finally take into also photo photo

00:47:50.000 --> 00:48:04.000
fusion, in case of a color singlet effect is also very large at beryllium and gamma gamma is the green one like this for highly charged particles.

00:48:04.000 --> 00:48:13.000
On the next slide you can see production per section for all those four types of particles. I just want you to notice that.

00:48:13.000 --> 00:48:25.000
And the production costs section increases significantly. When we increase the charge in case of NGOs this mean orders of magnitude change.

00:48:25.000 --> 00:48:42.000
Besides of. I mean, in addition to considering pairs of particles particle antiparticle pairs produced that propagates through the detector. We also considered formation of joining like bounce states, made of those new particles.

00:48:42.000 --> 00:48:51.000
And we calculated this, the production costs section for these using another relativistic approximation.

00:48:51.000 --> 00:49:05.000
Potential within the Schrodinger equation, we were able to obtain hydrogen atom like solutions, then we use now with approximation to get cross section to produce us bound state that

00:49:05.000 --> 00:49:26.000
says I have very limited time, I will not explain in details how we requested this analyzes, I just want to say that for open channel searches, we use, we based our study on analyzes by CMS that look for large the dx.

00:49:26.000 --> 00:49:39.000
our analyzes on Atlas resonance default on search, and for, and we also did open channel searches for the middle experiment using our own simulation.

00:49:39.000 --> 00:49:44.000
Now I'll show you the results. So the results of a form of two dimensional planes.

00:49:44.000 --> 00:50:07.000
Is there is a charge of a particle on the y axis, there is a mass of new particle corresponds to the experiments will be able to provide at the end of data taking period, the gray, the gray should be already dead.

00:50:07.000 --> 00:50:23.000
Now, there are several curves, the red curve is the open channel search and CMS. And as you can see it changes mother it with the charge. The blue curve is the closed on the search.

00:50:23.000 --> 00:50:28.000
that is not give too low charges.

00:50:28.000 --> 00:50:32.000
The for larger charges can be the dominant one.

00:50:32.000 --> 00:50:35.000
Winters correspond to the middle experiment.

00:50:35.000 --> 00:50:48.000
It always increases with George and Jenny provides the immediate sensitivity. You can, because the most top one is responsible detection of one event, then two events.

00:50:48.000 --> 00:51:07.000
Events, we can speak about such low numbers because medal is background for the experiment. It's for those that maybe haven't heard about it, it's a mostly passive detector located in LA CBK burn two meters away from intersection point eight.

00:51:07.000 --> 00:51:17.000
It was primarily designed to search for magnetic monopoles but it can also detect. Long live particles if they are highly organized.

00:51:17.000 --> 00:51:25.000
So on the next slide. I'll provide you a results for colors scalars on the left for run three on the right for hi Lou me.

00:51:25.000 --> 00:51:28.000
And as you can see.

00:51:28.000 --> 00:51:53.000
On three, four charges from one of the large PBX searches are most dominant and for larger charges the search for diapers on, man. And we can expect limits like 550 GV for touch one for charge eight 2.2 TV or high luminosity the limits grow to be 600

00:51:53.000 --> 00:52:13.000
One, and at 2.5 TV for touch a something that I think happens for intermediate values of charges from three touch six medal becomes more sensitive than those not experiments like a mess.

00:52:13.000 --> 00:52:21.000
This is kind of surprising because metal is a small experiment, and it will operate at 10 times lower luminosity than those.

00:52:21.000 --> 00:52:31.000
However, metal is background free, so it doesn't suffer from increased background after going to hi Lou me, and it can become here.

00:52:31.000 --> 00:52:33.000
City.

00:52:33.000 --> 00:52:39.000
Large experiments which is kind of interesting. limits for the colors failures are stronger.

00:52:39.000 --> 00:52:51.000
So, for one week. 950 gV during grand three and four charge a 2.3 TV for high luminosity.

00:52:51.000 --> 00:53:08.000
For charge one it should be about one TV, and for charge eight point 60 being and again we see that for intermediate values that that becomes more sensitive than our class and CMS wire for called scholars limits or even stronger.

00:53:08.000 --> 00:53:26.000
So we have one TV 550 GV for touch one during at the end of round three, and then we're charged eight we have 2.6. tv. And for a high low me with one point 61, and four charged.

00:53:26.000 --> 00:53:32.000
We have 2.9 TV situation with Mandela similar.

00:53:32.000 --> 00:53:42.000
And finally colored females here the bounce our strongest, so we can expect for charge one at the end of run three.

00:53:42.000 --> 00:53:51.000
Two TV, and the fourth charge eight, it would be 2.8. tv. And for high luminosity.

00:53:51.000 --> 00:54:06.000
Expect over to TV for charge one and four charged eight people in one TV, more sensitive Atlas are in for charges from three to six.

00:54:06.000 --> 00:54:26.000
So to conclude, we can detect want to be charged heavy Longley particles, Adelaide see for open and close Jonathan searches and but if we want to correctly interpret our findings, we need to include, we need to consider photon photon, and photon gamma

00:54:26.000 --> 00:54:33.000
fusion processes to an appropriate PDF to calculate costs section accurately.

00:54:33.000 --> 00:54:46.000
Now, when it comes to large experiments like Atlas and CMS, then generally open channels such they're more sensitive for charges from one to five. Why for larger charges the default on the resonance searches become more sensitive.

00:54:46.000 --> 00:54:56.000
And when it comes to metal. It provides a completely different methods, then Atlassian CMS, because its background free and passive.

00:54:56.000 --> 00:55:04.000
And for around three, it provides intermediate sensitivity for all charges. While what is interesting for a high lumen.

00:55:04.000 --> 00:55:17.000
We expect that metal can become more sensitive than Atlassian CMS for intermediate value of charges from three to six, he. Because, mainly because it's big on experiments.

00:55:17.000 --> 00:55:31.000
And, as you might have noticed I showed you, limits from those three analyzes I didn't show me like a combined limit. And I think none of the experiments, provided that but my I might be wrong.

00:55:31.000 --> 00:55:40.000
I'm seeing something like a combined image from different searches open and close channel would be very, very interesting.

00:55:40.000 --> 00:56:02.000
And before I finish, just wanted to mention that there has been a very recent very recent resolved by Atlas and you large ddx search was published in May, and an excess with 3.3 sigma significance has been observed that is interpreted as a longer particle.

00:56:02.000 --> 00:56:08.000
There was a talk about it and discussion, two days ago at this workshop.

00:56:08.000 --> 00:56:10.000
Thank you.

00:56:10.000 --> 00:56:20.000
Thank you very much for these nice talk, and we open the floor for questions.

00:56:20.000 --> 00:56:36.000
Because if not, I had to ask you, okay, Mike is going to say yeah, just okay and such a high charged particles could affect g minus to Milan is that been calculated or does it neon t minus to give limits on these particles,

00:56:36.000 --> 00:56:39.000
minus two.

00:56:39.000 --> 00:56:49.000
For any any charged particles especially highly charged ones in the loop diagram can can affect p minus to neon, but it probably is. They're really heavy.

00:56:49.000 --> 00:56:52.000
that would be

00:56:52.000 --> 00:57:07.000
simplified modern life okay yes yes it's model. It's model, we wanted to be as general as possible. So we basically we only assume in our studies the quantum numbers of particles.

00:57:07.000 --> 00:57:18.000
And we've already there mass, and we are the collider stable or in case of Madeley Parma tries to be killing so that became depends, I think, on the concrete model.

00:57:18.000 --> 00:57:28.000
We wanted. Instead, give like a rough estimate what can be measured around relate see and hi to me.

00:57:28.000 --> 00:57:35.000
Then if you have like a concrete model you can kind of like, know what to expect.

00:57:35.000 --> 00:57:48.000
Does that answer your question or yeah pretty well I guess yeah but I don't know if it's been calculated p minus two things so maybe he wants to say something about this, or something different I don't know.

00:57:48.000 --> 00:58:15.000
I will draw something different. Just as a follow up on the, on the sexuality. Yes, we have two days ago, we would metal be sensitive to what's possibly atlases seeing the luminosity still low but for metal because we have only been nearly as a signature.

00:58:15.000 --> 00:58:20.000
When you see that in your plastic.

00:58:20.000 --> 00:58:31.000
In order for me to be sensitive, the particle has to be really long lived, it has to traverse at least two meters, the detector is two meters away from the section point.

00:58:31.000 --> 00:58:34.000
And it has to be highly organized.

00:58:34.000 --> 00:58:42.000
Now, maybe I would be, this has to be checked

00:58:42.000 --> 00:58:55.000
yet yes I think it has a chat, there's a chance but like, there's still ongoing discussion with actually how to interpret this result, there was this thing.

00:58:55.000 --> 00:58:58.000
But

00:58:58.000 --> 00:59:07.000
apparently not that they're supposed to be faithful one or so and that probably would not not.

00:59:07.000 --> 00:59:12.000
Yes, yes, you're right you're right, you're right. So, uh, yeah, you're right.

00:59:12.000 --> 00:59:21.000
So, okay, I have to look at it maybe once within the collaboration.

00:59:21.000 --> 00:59:26.000
No, actually I wanted to show you this, this book, it's in the backup.

00:59:26.000 --> 00:59:39.000
Actually Actually you're right so mentally sensitive, only to slowly moving particles. So if you did this data suggests this particles, black, brown charge one or touch to

00:59:39.000 --> 00:59:48.000
touch to the particle has to move low, not more than 30% of speed of light, to be detectable at that not meddle.

00:59:48.000 --> 00:59:54.000
So if their data suggests.

00:59:54.000 --> 01:00:09.000
Also this other measurement that's said, 0.6, if I remember correctly, and it's still like beyond Mandela switch. And that has this big

01:00:09.000 --> 01:00:18.000
property that it's sensitive, only to slowly moving particles.

01:00:18.000 --> 01:00:48.000
Okay, thank you, thank you very much for this estimation I think for for more refined estimates estimates, you can always use the matter most channel.

