- Hep-pheno - listserv.vub.be

Fwd: ULB PhysTH Seminar by Jeesun Sk - 23/09/2024 at 11 am
by Alberto Mariotti 17 Sep '24

17 Sep '24

#---------------------------------------------------------------------# Alberto Mariotti Vrije Universiteit Brussel (VUB) https://hep.research.vub.be Phone: +32 (0) 2 629 32 15 E-mail: alberto.mariotti(a)vub.be Address: Vrije Universiteit Brussel Physics Department Pleinlaan 2, 1050 Brussels, Belgium #---------------------------------------------------------------------# > Begin forwarded message: > > From: FACCHINETTI Gaëtan <gaetan.facchinetti(a)ulb.be> > Subject: Re: ULB PhysTH Seminar by Jeesun Sk - 23/09/2024 at 11 am > Date: 17 September 2024 at 08:29:05 CEST > To: GRP_ULB_PhysTh <GRP_phys_th(a)ulb.be>, GRP_ULB_Sem_Add <GRP_physth_sem(a)ulb.be> > Resent-From: <alberto.mariotti(a)vub.be> > > Dear All, > > Please find below the title and abstract for next-week seminar (Monday 23/09/2024 at 11 am). > > Studying dark sector imprints in cosmology and ground based experiments > Relativistic degrees of freedom or N_eff is one of the crucial cosmological parameters and is sensitive to extra radiation energy density at the time of neutrino decoupling. The precise measurement of $N_eff$ at the time of CMB formation by Planck 2018 can be used to understand fundamental interactions and to shed light on beyond standard model (BSM) scenarios. In this talk I will explain how N_eff can probe light (MeV) freeze in dark matter models which contain additional neutrino injection at late time. We propose a scenario where a long lived scalar decays to a dark matter and active neutrinos after BBN. Despite the feeble coupling of DM the parameter space can be probed via N_eff. I will also talk about how N_eff at CMB can constrain light Z' gauge boson realized in generic BSM U(1)_X scenarios. Finally, from the perspective of ground based experiments, I will show how table top experiments like optically trapped nanospheres can shed light on MeV scale dark matter and other BSM particles like ALP. > > Best regards, > > Gaétan > >> Le 16 sept. 2024 à 13:23, FACCHINETTI Gaëtan <gaetan.facchinetti(a)ulb.be> a écrit : >> >> Dear All, >> >> I am happy to announce our first seminar of this academic year. Jesus Sk (IACS, Kolkata) will give us a seminar next Monday, the 23rd of September, at 11am in room 2.N7.110 (building NO, campus Plaine). Please note the unusual time slot! In case 11am is inconvenient for too many of you, please let me know and we can try to move it later that day (if it suits the speaker too). The title and abstract will be sent as soon as possible. >> >> Best regards, >> >> Gaétan > > > > You're receiving this message because you're a member of the GRP_ULB_Sem_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_sem@ulb.be/groupsubscription.a…> | Leave group <https://outlook.office365.com/owa/GRP_physth_sem@ulb.be/groupsubscription.a…> | Learn more about Microsoft 365 Groups <https://aka.ms/o365g> > >

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Fwd: 2024 Jacques Solvay International Chair in Physics (Professor Samaya Nissanke) - Tuesday 1 October at 4:00 pm
by Alberto 16 Sep '24

16 Sep '24

Sent from my iPhone, please excuse brevity and typos Begin forwarded message: > From: Isabelle Van Geet <Isabelle.vanGeet(a)solvayinstitutes.be> > Date: 16 September 2024 at 14:29:12 CEST > To: Isabelle Van Geet <Isabelle.vanGeet(a)solvayinstitutes.be> > Subject: 2024 Jacques Solvay International Chair in Physics (Professor Samaya Nissanke) - Tuesday 1 October at 4:00 pm > > Dear Colleagues, > > We are pleased to announce the Inaugural Lecture of the 2024 Jacques Solvay International Chair in Physics by Professor Samaya Nissanke (UvA & Nikhef, The Netherlands). > > The lecture will be held on Tuesday 1 October at 4:00 p.m (ULB, Campus Plaine, Building NO, 5th Floor, Salle Solvay). > > Title: New Perspectives onto the Universe in the Era of Multi-Messenger Astrophysics > > Abstract: Since the revolutionary discovery of gravitational wave (GW) emission from a binary black hole merger in 2015, the remarkable GW detectors LIGO, Virgo and KAGRA have detected at least ninety compact object mergers. These events are transforming modern astronomy. In particular, the first binary neutron star merger, dubbed GW170817, was observed in both gravitational and electromagnetic radiation, thus opening up a new era in multi-messenger astrophysics. The multi-messenger characterisation of such an event has enabled major advances into diverse fields of modern physics from gravity, high-energy astrophysics, nuclear physics, to cosmology. In this talk, I will present a review of gravitational wave observations to date, as well as my work in strong-field gravity astrophysics and how combining observations, theory and experiment have been key in making progress in this field. I will present the challenges and the opportunities that have emerged in multi-messenger astrophysics, and what the future holds in this new era. > > Everybody is cordially invited! > > Best wishes, > Marc Henneaux >

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Fwd: ULB PhysTH Seminar by Raffaele-Tito D’agnolo - 14/06/2024 at 11 am
by Alberto Mariotti 12 Jun '24

12 Jun '24

An interesting talk about high frequency GW, Friday at 11:00 at ULB, I could go…. Alberto > Begin forwarded message: > > From: VERMA Sonali <sonali.verma(a)ulb.be> > Subject: ULB PhysTH Seminar by Raffaele-Tito D’agnolo - 14/06/2024 at 11 am > Date: 10 June 2024 at 14:01:02 CEST > To: GRP_ULB_PhysTh <GRP_phys_th(a)ulb.be>, GRP_ULB_Sem_Add <GRP_physth_sem(a)ulb.be> > Resent-From: <alberto.mariotti(a)vub.be> > > Dear All, > > It is my great pleasure to announce that Raffaele-Tito D’agnolo (IPhT, Paris) will give a seminar on Friday, the 14th of June, at 11am in room 2.N7.110 (building NO, campus Plaine). He will talk about > > Heuristics for Primordial Gravitational Wave Detection > > Abstract: Stochastic backgrounds of gravitational waves can potentially open a window on extremely high energies, giving us information on phase transitions at the GUT scale and many other BSM phenomena. In this talk I will discuss simple heuristic arguments that allow to establish the smallest detectable energy density in a primordial gravitational wave background. I will focus mainly on what is achievable with realistic detectors, and comment on the potential of advanced quantum sensing techniques. In the foreseeable future, it is not feasible to go beyond the BBN bound for frequencies above 100 kHz. > > Best regards, > > Sonali (for the seminar organizers) > > > You're receiving this message because you're a member of the GRP_ULB_Sem_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_sem@ulb.be/groupsubscription.a…> | Leave group <https://outlook.office365.com/owa/GRP_physth_sem@ulb.be/groupsubscription.a…> | Learn more about Microsoft 365 Groups <https://aka.ms/o365g> > >

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seminar of Arianna Renzini June 11th at 14:00
by Alberto Mariotti 10 Jun '24

10 Jun '24

Dear all, This email is to announce the seminar of Arianna Renzini (Milano Bicocca University) , on 11th June (Tuesday) at 14:00, in the Large Seminar room at the IIHE (G.1.03 Sacton Room). Title: Reaching beneath the surface: Gravitational-wave Background search methods, targets, and implications: Abstract: "Gravitational-wave backgrounds (GWBs) encompass a multitude of signals across the wide gravitational-wave (GW) frequency spectrum, and represent key targets in the panorama of gravitational-wave data analysis. Typically, GWBs are considered to be the collection of GW signals that lie just beneath the threshold of detection. In this talk, I will broadly introduce GWBs and various ongoing or near-future detection efforts, focusing on ground-based interferometers such as LIGO and Virgo. I will specifically focus on the astrophysical GWB from binary black holes and neutron stars, as it is expected to be the main background source in the LIGO-Virgo-KAGRA (LVK) frequency range. I will describe the flagship LVK GWB searches and outline their key implications beyond GWs: The GWB power spectrum includes information on binary formation history and mass distribution, while its angular power spectrum is a tracer of large-scale structure, and many other potential sky distributions. I will present two new and improved GWB searches I am involved in, which are expected to outperform current approaches and which we plan to apply to O4 data. Finally, I will close with an overview of the future of GWBs with promising new detectors such as LISA and 3G interferometers." Here the indico page of the event: https://indico.iihe.ac.be/event/1884/ Feel free to share this announcement with anyone who might be interested in your groups. Hope to see you all there. Best, Alberto #---------------------------------------------------------------------# Alberto Mariotti Vrije Universiteit Brussel (VUB) 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 #---------------------------------------------------------------------#

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Fwd: [allusers-iihe] Next two HEP@VUB colloquia: 13/06 and 20/06
by Alberto Mariotti 10 Jun '24

10 Jun '24

Hi All, just a reminder about this HEP@VUB events. While the one of this week might be though because of the visit of Denise, the one of following week should be more easy to attend. Sandwiches are provided. Cheers, Alberto > Begin forwarded message: > > From: Denise Muller via allusers-iihe <allusers-iihe(a)listserv.vub.be> > Subject: [allusers-iihe] Re: Next two HEP@VUB colloquia: 13/06 and 20/06 > Date: 6 June 2024 at 13:58:15 CEST > To: hep(a)listserv.vub.ac.be, All users <allusers-iihe(a)listserv.vub.be> > Reply-To: Denise Muller <denise.muller(a)vub.be> > > Dear colleagues, > > this is a kind reminder of the next two HEP@VUB colloquia, the first one taking place on June 13th and the second one taking place on June 20th: > > Thu, 13th June, 12h: Dr. Matteo Bonanomi (Hamburg University), "Going beyond the Standard Model with the CMS detector", https://indico.iihe.ac.be/event/2006/ > Thu, 20th June, 12h: Kathrine Mørch Groth (Niles Bohr Institute), "Galactic and extragalactic neutrino source populations", https://indico.iihe.ac.be/event/2024/ > For Matteo's talk, please register by Monday noon. > > For Kathrine's talk, please register by the end of next week. > > > Kind regards, > Denise & Yarno on behalf of the organizing team > > > On 30.05.24 11:40, Denise Muller wrote: >> Dear colleagues, >> >> We are happy to announce our next two HEP@VUB colloquia. The first talk will be on June 13th, the second one on June 20th: >> >> Thu, 13th June, 12h: Dr. Matteo Bonanomi (Hamburg University), "Going beyond the Standard Model with the CMS detector", https://indico.iihe.ac.be/event/2006/ >> Thu, 20th June, 12h: Kathrine Mørch Groth (Niles Bohr Institute), "Galactic and extragalactic neutrino source populations", https://indico.iihe.ac.be/event/2024/ >> >> As usual, sandwiches and cake will be served during the colloquia. Please register on the indico pages indicated above. >> >> Kind regards, >> Denise & Yarno on behalf of the organizing team > > _______________________________________________ > allusers-iihe mailing list -- allusers-iihe(a)listserv.vub.be > To unsubscribe send an email to allusers-iihe-leave(a)listserv.vub.be

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Fwd: JC 06/06/2024
by Alberto Mariotti 04 Jun '24

04 Jun '24

Hi All, don’t miss Aaron JC at ULB on Thursday ! Cheers, Alberto > Begin forwarded message: > > From: KOROCHKIN Alexander <alexander.korochkin(a)ulb.be> > Subject: JC 06/06/2024 > Date: 4 June 2024 at 12:26:22 CEST > To: GRP_ULB_PhysTh <GRP_phys_th(a)ulb.be>, GRP_ULB_JC_Add <GRP_physth_jc(a)ulb.be> > Resent-From: <alberto.mariotti(a)vub.be> > > Dear all, > > I would like to announce that our next JC will take place this Thursday 06/06 at 12:30 in the room 2.N7.110. > > Aaron Rase (VUB, PhD student) kindly volunteered to talk about "Collapsing Domain Wall Networks: Impact on Pulsar Timing Arrays and Primordial Black Holes" based on <https://arxiv.org/abs/2404.16094>arXiv:2401.14331 <https://arxiv.org/abs/2401.14331> (and arXiv:1807.01707 <https://arxiv.org/abs/1807.01707>) > > > > Best, > Alexander > > > 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>

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BPS Scientific Meeting 2024 May 29th at VUB
by Alberto Mariotti 21 May '24

21 May '24

Dear All, here the last reminder to register for the Belgian Physical Society Meeting of 29th May at VUB. The preliminary program, including the parallel sessions, can be found on the website of the conference https://www.belgianphysicalsociety.be/event/conference-2024/page/101 The registration close tomorrow 22 May (midnight) ! Please forward this last announcement to possible interested members in your group. Best, Alberto #---------------------------------------------------------------------# Alberto Mariotti Vrije Universiteit Brussel (VUB) 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 #---------------------------------------------------------------------#

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Fwd: ULB PhysTH Seminar by Andrea Caputo - 24/05/2024 at 11 am
by Alberto Mariotti 21 May '24

21 May '24

FYI, Seminar at ULB on Friday at 11:00. #---------------------------------------------------------------------# Alberto Mariotti Vrije Universiteit Brussel (VUB) 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: FACCHINETTI Gaëtan <gaetan.facchinetti(a)ulb.be> > Subject: ULB PhysTH Seminar by Andrea Caputo - 24/05/2024 at 11 am > Date: 21 May 2024 at 10:11:12 CEST > To: GRP_ULB_PhysTh <GRP_phys_th(a)ulb.be>, GRP_ULB_Sem_Add <GRP_physth_sem(a)ulb.be> > Resent-From: <alberto.mariotti(a)vub.be> > > Dear All, > > We are happy to announce that Andrea Caputo (CERN) will give us a seminar this Friday, the 24th of May, at 11am in room 2.N7.110 (building NO, campus Plaine). His presentation will be about > > Axion hunting using (proto)-neutron stars > In this talk I will describe some new ideas to discover (or constrain) new hypothetical particles, such as axions and axion-like particles. In the first part of the talk, in particular, I will show how we can use luminosity curves and spectra of low-energy supernovae to detect exotic energy injection due to particles produced in the newborn proto neutron star. Then, in the second part of the talk, I will advance the clock in the life of the neutron star and study the impact on new particles on the cooling of old neutron stars and the dynamics of the magnetosphere. > > Best regards, > > Gaétan (for the seminar organizers) > > > You're receiving this message because you're a member of the GRP_ULB_Sem_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_sem@ulb.be/groupsubscription.a…> | Leave group <https://outlook.office365.com/owa/GRP_physth_sem@ulb.be/groupsubscription.a…> | Learn more about Microsoft 365 Groups <https://aka.ms/o365g> > >

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Enhancing Nursing Education: My Tutor Club - Your Virtual Learning Community
by ea5562498＠gmail.com 16 May '24

16 May '24

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by ea5562498＠gmail.com 16 May '24

16 May '24

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