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Electroweak Penguin Decays
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Yes. Hi. It's a pleasure to talk to you about the latest results from
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the limits on the B to ee branching ratio. On slide four, what would be considered
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predictions also changed a bit. The form factor uncertainties actually
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decreased. But the sub-leading corrections to the interpolation, it
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actually became more conservative. Together with a small shift in central
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value of the observation, this results in just a slight decrease in discrepancy with
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the Standard Model. But the behaviour of all of our angular observables is now more
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consistent with a single change in C9 which is the vector boson coefficient.
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Speaking of Wilson coefficients, just one slide on effective theory. This is a
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tool that helps us write the process as a sum over effective operators, that
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describe the physics happening at this effective four point interaction on the
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bottom right block,
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as electroweak penguins are the B to sll transitions. So I'm not talking about
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and their Wilson coefficients. These parameterise the amount of which kind of
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physics happens at this vertex. The idea is that this allows for a model
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independent interpretation of which kind of new physics is happening here. But also
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it allows to combine different measurements of different processes which
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are sensitive to a subset of the same Wilson coefficients. Now, in this Q-
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squared region where these bins deviate, the C9 and the C10 - the vector and
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axial vector - are actually the most important ones. When we allow a freedom in C9
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and C10 in a fit, you can see on the bottom left that we have about 2.8
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sigma deviation from the Standard Model. But mostly this appears to be in the C9
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direction, so the vector direction. If we only allow to vary C9,
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where the gamma is on shell, I'm talking about the diagram shown on the right here.
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you see the middle plot, we are actually 3.3 standard deviations away with just
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this K*mumu measurement. And then on the right, for comparison, you see
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when we change C9 to minus one, which seems to be this preferred value, the
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Standard Model and the data - the theory and the data -
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match better by eye. So this is going from the solid line or the blue blocks to these
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blue dashed lines. Slide 14. I mentioned combinations of different
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measurements contributing to the same Wilson coefficients, so it's a natural
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moment to move on to the second analysis I wanted to highlight, which is the
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measurement of B to ee. This is also a b2sll transition, but it has a different
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decay topology, to leptons only. And because of helicity suppression, this is
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These are flavour changing and neutral. So these are forbidden at tree level in the
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even more suppressed. If you see this equation in the branching ratio here, the
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helicity suppression occurs in front of this C10 term, which is the same C10
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as we saw for this angular analysis. But there are also scalar and pseudo-scalar
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contributions which were not there. They contribute to the
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overall picture of the coefficients, of course, but the B to ee analysis is even
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more suppressed in C10. So this is a very good probe of scalar new physics. And even
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one observation, one event, would actually be a very significant hint for new physics
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already. In slide 15, the B to mumu results. Aiden already talked about it. So, I will
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not mention that now. But on the bottom left, you can see our results for the
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search of B to ee, which resulted in no observation, but a limit that is 30
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Standard Model. So they are very suppressed, and called rare decays. And
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times better than the previous CDF one. The global picture of those
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coefficients will help constrain which kinds of new physics
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might explain our other observations.
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In slide 16, I'm done with the LHCb measurements. But I just wanted
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to mention that there are many independent groups who do these models-independent
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fits to a lot of these measurements combined: in the order of 170. And they
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find somewhat consistently that C9 only, deviates from zero by four sigma to
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five sigma, depending on your assumptions and which group you ask. But
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it all seems to be consistent with a single change in a Wilson coefficient, this
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factor seems to be minus one, maybe. So this is a very interesting result, how all
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because of that, sensitive to new physics in the loops, or even at tree
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of these measurements somehow seem to point to a single explanation. I think
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that's fascinating. So any kind of vector new physics is very hot at the
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moment, of course, because of this. On slide 17, my conclusion. I showed you two
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new exciting results on b2sll transitions from LHCb: the angular analysis K*mumu,
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and this new rare decay, B to ee, where we have a limit. The discrepancy in this angular
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analysis with the Standard Model still stands, although it did not increase
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because of various reasons. And all of these results are not done with the full
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dataset yet: we’re still analysing the remaining data that we took in Run-2, so we
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can expect the what we call ‘Run-1+2 legacy results’ soon. This also
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goes for the new B to mumu analysis, which is coming out, hopefully,
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level, if that's the form that new physics takes. We can categorise these penguins
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very soon. The B to ee analysis, and on top of that, we actually have many other analysis
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ongoing. These are R(X) analyses that Miriam will talk about after me, but also we
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finally have enough statistics to measure the angular analysis of K*ee
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actually. So all kinds of very interesting new results will hopefully come out soon
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with that more data.
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And that's it. Thank you. Thank you for your attention.
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Question to Jacco, please raise your hand
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Yeah, my chemical yosity just started. Sure.
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So, you mentioned second edition and China is that you can start of course not but
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there is one missing I remember the visa are quite old the result from the bar
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in three classes: the ratios of different flavours of leptons, which we call R(X),
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about B plus C two three plus down that was about two or something time 10 to the
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minus three
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is quite interesting. I think c said
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should be sensitive to the effects massing and the the tweaks doubled more than
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So, do you think it is something that can be feasible in Italy should be a thing. So
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since you use already final stage without?
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Yeah, so
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I will I will not say it's not possible? Absolutely not. We've made an attempt at B
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to dow which is even more challenging. So it's definitely something we we studied,
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we can study I should say. But it is tricky at the LSE. Right? So these these
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but that's the subject of the talk by Miriam, which is right after mine. And the
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measurements with without, you have to make it takes time. I should say that,
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yeah, I would expect the result like that coming from LGB soon, but it doesn't mean
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it's not something maybe we can all do. And it adds to the to the full picture. So
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it's an interesting channel, I think.
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Thank you very much.
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Other question
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seems not so we can move to the third
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measurements of branching fractions and angular observables. We measure these
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last March actually, on electroweak penguin decays from LHCb. So on slide 2,
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as a function of the Q-squared which is the invariant mass of, in this case, the
End of preview. Expand in Data Studio

LHCP-ASR Segments

This dataset is a segment-level distribution derived from mllp/LHCP-ASR (and the original LHCP-ASR repository), an English speech corpus for narrow-domain ASR benchmarking in high-energy particle physics.

Unlike previous versions, this repository provides audio directly at the segment level (<30 seconds each) for evaluation, adds talk-level metadata and cleans up transcription tags.

Differences from mllp/LHCP-ASR

  1. No subsets: Directly formatted as segments (<30s audio chunks). There is no longform configuration.
  2. Evaluation splits: Specifically contains the test partitions:
    • test.2020
    • test.2022
  3. Text normalization: Occurrences of <UNK> (used in manual transcriptions to mark unintelligible speech) have been removed.
  4. Metadata: Each sample now contains talk-level metadata fields (talk_id, segment_pos, title and speaker_id).

Metadata fields

  • talk_id (str): Identifier for the talk to which the segment belongs.
  • segment_pos (int): Sequential position of the segment within the talk.
  • title (str): Title of the plenary talk.
  • speaker_id (str): Identifier of the primary speaker of the talk. This field refers to the assigned presenter of the talk, not strictly the voice heard in every segment. Segments may contain speech from session chairs or Q&A audience members.

Usage

You can load the dataset directly using the Hugging Face datasets library:

from datasets import load_dataset

# Load the full dataset
dataset = load_dataset("mllp/LHCP-ASR-segments")

# Or load a specific test split
test_2020 = load_dataset("mllp/LHCP-ASR-segments", split="test.2020")
test_2022 = load_dataset("mllp/LHCP-ASR-segments", split="test.2022")

Citation

If you use this dataset, please cite the original work:

@inproceedings{santamariajorda25_interspeech,
  title     = {{LHCP-ASR: An English Speech Corpus of High-Energy Particle Physics Talks for Narrow-Domain ASR Benchmarking}},
  author    = {Jaume Santamaría-Jordà and Pablo Segovia-Martínez and Gonçal V. {Garcés Díaz-Munío} and Joan Albert Silvestre-Cerdà and Adrià Giménez and Rubén {Gaspar Aparicio} and René {Fernández Sánchez} and Jorge Civera and Albert Sanchis and Alfons Juan},
  year      = {2025},
  booktitle = {{Interspeech 2025}},
  pages     = {4033--4037},
  doi       = {10.21437/Interspeech.2025-2630},
  issn      = {2958-1796},
}

For more details on the original dataset, visit https://github.com/mllpresearch/LHCP-ASR.


Legal disclaimer

Speech and text data were provided by the European Organization for Nuclear Research (CERN) under PO OV9177345. The following disclaimers are those available in the CERN Document Server (CDS) repository on May 30th, 2025:

CERN Document Server - Terms and Conditions

DOI

Use of the CERN Document Server service (hereafter "CDS") denotes agreement with the following terms of use:

  • CDS is provided free of charge. It serves as a comprehensive institutional repository and dissemination platform for the research and historical output produced by CERN, the European Organization for Nuclear Research, and its members of personnel. See Content Policy [1] for more details.
  • By uploading content to CDS, the content provider affirms that such content complies with all applicable laws, licence conditions and third party rights, and shall hold CERN free and harmless from any related liability.
  • All content is provided "as is" and without warranty of any kind. The user shall hold CERN and individual content providers free and harmless from any related liability in connection with its use of such content.
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  • CERN bases CDS on leading technologies and architectures, operated within the limits of its financial and human resources and made available by CERN on an "as is" and "best efforts" basis. Access to, availability and use of CDS is not guaranteed nor can be expected.
  • CERN excludes and disclaims all liability for damage resulting from users' access, or inability to access, or use of CDS.
  • These terms and conditions of use are subject to change by CERN at any time and without notice, other than through posting the updated terms on the CDS website. Any revised terms and conditions of use shall become effective immediately upon posting.

If you have any questions or comments with respect to CDS, or if you are unsure whether your intended use is in line with these Terms and Conditions, or if you seek permission for a use that does not fall within these Terms and Conditions, please contact CDS support.

[1] CDS Content Policy DOI


License

This dataset is licenced under CC-BY-NC-ND 4.0. To view a copy of this licence, visit https://creativecommons.org/licenses/by-nc-nd/4.0/

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