Hello everyone,
After a never-ending discussion to set the date of our new JC, we decided to organize the first one on Tuesday 21/02 at 2PM.
I will be talking about the recent proposal for the formation of PBH from FOPTs discussed in https://arxiv.org/abs/2106.05637 and https://arxiv.org/pdf/2212.14037.pdf.
I hope to see you,
Best,
Miguel
> Begin forwarded message:
>
> From: Juan Garcia-Bellido <juan.garciabellido(a)gmail.com>
> Subject: [Et-all] First Announcement COSMO 23
> Date: 21 February 2023 at 18:04:32 GMT+1
> To: et-all(a)ego-gw.it
> Resent-From: <alberto.mariotti(a)vub.be>
>
>
> Dear Colleagues,
>
> We are delighted to announce that from September 11th to 15th, 2023, we will host the COSMO’23 conference at the Instituto de Física Teórica (IFT UAM-CSIC) in Madrid, Spain.
>
> Confirmed invited speakers and the topics they will cover include:
>
> Alex Amon (Weak Lensing)
> Raul Angulo (Cosmological Simulations)
> Phil Bull (21cm Surveys)
> Clare Burrage (Dark Energy & Modified Gravity)
> Sebastien Clesse (Dark Matter)
> Paolo Creminelli (Early Universe)
> Eleonora Di Valentino (Tensions in Cosmology)
> Daniel Figueroa (Early Universe Gravitational Waves)
> Kiyotomo Ichiki (Status of CMB Observations)
> Isobel Romero-Shaw (Simulations for Black Hole Populations)
> Eva-Maria Muller (Galaxy Clustering)
> Samaya Nissanke (Gravitational Wave Observations)
> Enrico Pajer (Cosmological Correlators)
> Paolo Pani (Strong Gravity)
> Rafael Porto (Analytical Approaches for Black Hole Coalescence)
> Arman Shafieloo (Statistical Methods)
> Francisco Villaescusa-Navarro (Machine Learning Techniques)
> Gabrijela Zaharijas (Cosmic and Gamma Rays + Dark Matter Detection)
>
> Registration will open in March 2023, the registration fee is expected to be around €350, and limited support will be available upon request.
>
> The webpage is:
> https://workshops.ift.uam-csic.es/COSMO23
>
> <https://workshops.ift.uam-csic.es/COSMO23>
> Best wishes,
>
> The COSMO’23 SOC
> Yashar Akrami, George Alestas, Santiago Ávila, David Cerdeño, Matteo Fasiello, Juan García-Bellido (Chair), Violeta Gonzalez-Pérez, Sachiko Kuroyanagi, Carlos Muñoz, Savvas Nesseris, Ogan Özsoy, Lucas Pinol, Miguel A. Sánchez-Conde
>
> P.S. Apologies if you receive this more than once.
>
> ==========================
> Prof. Dr. Juan García-Bellido RAC
> Instituto de Física Teórica
> c/ Nicolás Cabrera 13-15
> Universidad Autónoma de Madrid
> Cantoblanco 28049 Madrid, Spain
> Tel: + 34 912999812
> juan.garciabellido(a)uam.es <mailto:juan.garciabellido@uam.es>_______________________________________________
> Et-all mailing list
> Et-all(a)ego-gw.it
> https://mail.ego-gw.it/mailman/listinfo/et-all
FYI
> Begin forwarded message:
>
> From: HUFNAGEL Marco <marco.hufnagel(a)ulb.be <mailto:marco.hufnagel@ulb.be>>
> Subject: JC 16.02.2023
> Date: 15 February 2023 at 16:47:57 GMT+1
> To: GRP_ULB_PhysTh <GRP_phys_th(a)ulb.be <mailto:GRP_phys_th@ulb.be>>, GRP_ULB_JC_Add <GRP_physth_jc(a)ulb.be <mailto:GRP_physth_jc@ulb.be>>
> Resent-From: <alberto.mariotti(a)vub.be <mailto:alberto.mariotti@vub.be>>
>
> Dear all,
>
> we will have our next JC tomorrow at 12:30 in room 2NO.708.
>
> Chandan kindly volunteered to talk about
>
> The disappearance of neutral current Lepton Flavour Universality violation in R_K and R_K* in the latest update (Dec 22) by LHCb
>
> based on LHCb-PAPER-2022-045 and LHCb-PAPER-2022-046.
>
> I am looking forward to seeing all of you there!
>
> Best,
> Marco
>
>
> You're receiving this message because you're a member of the GRP_ULB_JC_Add group from Université Libre de Bruxelles. To take part in this conversation, reply all to this message.
>
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Dear All,
tomorrow there will be construction works in front of the IIHE, on the side of the office of Kevin/Alba/Hannah.
The noise should be present only in the morning, but most probably it will go a bit on also in the afternoon.
The visitor Fabrizio Rompineve will be around all day and give us a talk about "GW signatures at PTA", blackboards plus slides, at 14:00
https://indico.iihe.ac.be/event/1716/ <https://indico.iihe.ac.be/event/1716/>
Given the constructions, there are two options:
1) If the noise on our side (esplanade) is ok, then I propose I can host Kevin/Alba/Hannah/Xander in our offices (and in our seminar room).
The seminar then will go on in the small seminar room (1G012) as planned.
2) If the noise is too strong also on our side (esplanade), than we will all move on the 9th floor, building F, where we will have access to some office common space. Thanks a lot to Nina and Alex for making this possible.
The seminar will then go on into the small seminar room of the 9F.
Tomorrow morning when I will arrive (9:30), I will see what will be the best option, either 1 or 2.
Best,
Alberto
#---------------------------------------------------------------------#
Alberto Mariotti
Vrije Universiteit Brussel (VUB)
https://we.vub.ac.be/HEPVUB <https://we.vub.ac.be/HEPVUB>
Phone: +32 (0) 2 629 32 15
E-mail: alberto.mariotti(a)vub.be
Address: Vrije Universiteit Brussel
Physics Department
Elementary Particles Research Group
Pleinlaan 2, 1050 Brussels, Belgium
#---------------------------------------------------------------------#
> Begin forwarded message:
>
> From: HUFNAGEL Marco <marco.hufnagel(a)ulb.be>
> Subject: JC/Seminar tomorrow by Fabrizio Rompineve
> Date: 8 February 2023 at 12:07:09 GMT+1
> To: GRP_ULB_PhysTh <GRP_phys_th(a)ulb.be>, GRP_ULB_JC_Add <GRP_physth_jc(a)ulb.be>, "fabrizio.rompineve(a)cern.ch" <fabrizio.rompineve(a)cern.ch>
> Resent-From: <alberto.mariotti(a)vub.be>
>
> Dear all,
>
> it is a pleasure to announce that tomorrow -- instead of our usual JC -- we will have a special seminar by Fabrizio Rompineve from CERN, who is visiting VUB at the moment. The seminar will take place at 12:30 in the room 2NO.708 on the 7th floor of the NO building at ULB.
>
> Fabrizio will talk about
>
> QCD axion production in the early Universe
>
> with the following abstract:
>
> A population of relativistic QCD axions can be produced in the early Universe, via scatterings with Standard Model particles. This can be searched for in cosmological datasets, which therefore provide the opportunity to discover/constrain the QCD axion, independently of astrophysical and/or laboratory probes.
> In this talk, after reviewing the subject, I present an improved calculation of the relic abundance of such “hot” axions from scatterings with pions below the QCD crossover, as well as the resulting upper bound on the QCD axion mass. I then discuss the exciting outlook of upcoming cosmological surveys, which may probe otherwise unexplored regions of the QCD axion parameter space. I highlight the need of a non-perturbative calculation of axion production rates throughout the QCD crossover, to fully exploit the reach of such datasets.
>
> I am very much looking forward to seeing you there!
>
> Best,
> Marco
>
>
> You're receiving this message because you're a member of the GRP_ULB_JC_Add group from Université Libre de Bruxelles. To take part in this conversation, reply all to this message.
>
> View group files <https://outlook.office365.com/owa/GRP_physth_jc@ulb.be/groupsubscription.as…> | Leave group <https://outlook.office365.com/owa/GRP_physth_jc@ulb.be/groupsubscription.as…> | Learn more about Microsoft 365 Groups <https://aka.ms/o365g>