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VERSION:2.0
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BEGIN:VEVENT
SUMMARY:Particle Physics Seminars II
DTSTART:20230201T160000Z
DTEND:20230201T190000Z
DTSTAMP:20260623T225633Z
UID:7082cd16-b720-4512-921c-df8c9dc646a5
SEQUENCE:5
CREATED:20221223T115939Z
DESCRIPTION:Speaker: Ruben ConceiçãoTitle: Exploring the extreme energy 
 UniverseAbstract: Ultra-high-energy cosmic rays (UHECRs) and very high-ene
 rgy gamma rays are the highest-energy known particles and radiation\, resp
 ectively. Their study allows us to probe some of the most extreme phenomen
 a in our Universe and to investigate its fundamental physics properties. T
 he Pierre Auger Observatory\, with its upgrade\, AugerPrime\, and the futu
 re Southern Wide-field Gamma-ray Observatory\, are two of the most ambitio
 us astroparticle physics facilities in the world. In this talk\, I will br
 iefly discuss the technological challenges and physics opportunities conne
 cted with the study of these physics objects\, which defy our understandin
 g about acceleration mechanisms and particle interactions.Speaker: Catarin
 a CosmeTitle: Glimpses of a physicist journey to the dark side of the Univ
 erseAbstract: In this talk\, I will introduce myself\, give an overview of
  my academic path\, and briefly discuss the main lines of investigation th
 at I have pursued so far. I will pay special attention to the dynamics and
  phenomenology of non-thermal Dark Matter candidates\, in both standard an
 d non-standard cosmologies. Finally\, I will give a taste of future projec
 ts I want to follow.Speaker: Luiz Vale SilvaTitle: Opportunities in a high
 -statistics era for flavor physics: novel predictions of the Standard Mode
 l and New Physics probesAbstract: Flavor physics plays a central role in p
 article physics: for instance\, it led to the discovery of Charge-Parity (
 CP) violation. I discuss briefly the current and future status of the extr
 action of the CKM matrix elements in the Standard Model (SM). I also comme
 nt on the role charm physics can play in testing the Kobayashi-Maskawa mec
 hanism\, responsible for generating CP violation in the quark sector of th
 e SM. Finally\, I discuss bounds on different categories of generic New Ph
 ysics contributions.Speaker: Cristóvão VilelaTitle: Neutrino experiments
  at the intensity and energy frontiersAbstract: Neutrinos are some of the 
 least well understood particles in the Standard Model (SM) and play a cent
 ral role in major open questions in Physics: How did matter come to domina
 te over antimatter in the history of the Universe? Are there symmetries un
 derlying the flavour structure of the SM? Why are neutrino masses so small
 ? In this talk I will briefly describe two neutrino experiments which will
  help elucidate these puzzles: DUNE\, which is set to discover or rule out
  matter-antimatter asymmetry in neutrino oscillations\; and SND@LHC\, whic
 h will measure for the first time interactions of neutrinos of all three f
 lavours produced at CERN&#x27\;s Large Hadron Collider.
LAST-MODIFIED:20230130T200013Z
LOCATION:VA4\, Piso -1\, Pavilhão de Engenharia Civil
URL:http://df.vps.tecnico.ulisboa.pt/pt/eventos/particle-physics-seminars-
 ii/
X-ALT-DESC;FMTTYPE=text/html:<p data-block-key="ebaf2"><b>Speaker:</b> Rub
 en Conceição</p><p data-block-key="bj415"><b>Title:</b> Exploring the ex
 treme energy Universe</p><p data-block-key="64lks"><b>Abstract:</b> Ultra-
 high-energy cosmic rays (UHECRs) and very high-energy gamma rays are the h
 ighest-energy known particles and radiation\, respectively. Their study al
 lows us to probe some of the most extreme phenomena in our Universe and to
  investigate its fundamental physics properties. The Pierre Auger Observat
 ory\, with its upgrade\, AugerPrime\, and the future Southern Wide-field G
 amma-ray Observatory\, are two of the most ambitious astroparticle physics
  facilities in the world. In this talk\, I will briefly discuss the techno
 logical challenges and physics opportunities connected with the study of t
 hese physics objects\, which defy our understanding about acceleration mec
 hanisms and particle interactions.</p><p data-block-key="6d9ss"></p><p dat
 a-block-key="31mbr"><b>Speaker:</b> Catarina Cosme</p><p data-block-key="d
 ciik"><b>Title:</b> Glimpses of a physicist journey to the dark side of th
 e Universe</p><p data-block-key="au0cb"><b>Abstract:</b> In this talk\, I 
 will introduce myself\, give an overview of my academic path\, and briefly
  discuss the main lines of investigation that I have pursued so far. I wil
 l pay special attention to the dynamics and phenomenology of non-thermal D
 ark Matter candidates\, in both standard and non-standard cosmologies. Fin
 ally\, I will give a taste of future projects I want to follow.</p><p data
 -block-key="154qi"></p><p data-block-key="e186s"><b>Speaker:</b> Luiz Vale
  Silva</p><p data-block-key="160cv"><b>Title:</b> Opportunities in a high-
 statistics era for flavor physics: novel predictions of the Standard Model
  and New Physics probes</p><p data-block-key="to46"><b>Abstract:</b> Flavo
 r physics plays a central role in particle physics: for instance\, it led 
 to the discovery of Charge-Parity (CP) violation. I discuss briefly the cu
 rrent and future status of the extraction of the CKM matrix elements in th
 e Standard Model (SM). I also comment on the role charm physics can play i
 n testing the Kobayashi-Maskawa mechanism\, responsible for generating CP 
 violation in the quark sector of the SM. Finally\, I discuss bounds on dif
 ferent categories of generic New Physics contributions.</p><p data-block-k
 ey="e7vj6"></p><p data-block-key="2jt1o"><b>Speaker:</b> Cristóvão Vilel
 a</p><p data-block-key="97prd"><b>Title:</b> Neutrino experiments at the i
 ntensity and energy frontiers</p><p data-block-key="910b7"><b>Abstract:</b
 > Neutrinos are some of the least well understood particles in the Standar
 d Model (SM) and play a central role in major open questions in Physics: H
 ow did matter come to dominate over antimatter in the history of the Unive
 rse? Are there symmetries underlying the flavour structure of the SM? Why 
 are neutrino masses so small? In this talk I will briefly describe two neu
 trino experiments which will help elucidate these puzzles: DUNE\, which is
  set to discover or rule out matter-antimatter asymmetry in neutrino oscil
 lations\; and SND@LHC\, which will measure for the first time interactions
  of neutrinos of all three flavours produced at CERN&#x27\;s Large Hadron 
 Collider.</p>
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