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SUMMARY:The hiccupping Universe
DTSTART;VALUE=DATE-TIME:20190913T121500Z
DTEND;VALUE=DATE-TIME:20190913T123000Z
DTSTAMP;VALUE=DATE-TIME:20260926T112418Z
UID:indico-contribution-2-11@cern.ch
DESCRIPTION:Speakers: Dr. TERESI\, Daniele (Università di Pisa)\nWe consi
 der a scalar field with a bottom-less linear potential\, finding that cosm
 ologies unavoidably end up with a crunch\, even in scenarios compatible wi
 th the observed positive cosmological constant. Assuming that rebounces av
 oid singularities\, this generates a new kind of multiverse: the universe 
 undergoes cycles with different cosmological constants\, all with finite l
 ifetime regardless of the sign. This novel "temporal" multiverse avoids so
 me of the usual ambiguities present in the standard "spatial" one. Moreove
 r\, if a "hiccupping" mechanism changes the vacuum energy by a small amoun
 t at each cycle\, this dynamics  selects a small vacuum energy and becomes
  the most likely source of universes with anthropically small cosmological
  constant. Its probability distribution could avoid the gap of 2 orders of
  magnitude that seems left by standard anthropic selection.\n\nhttp://indi
 co.fuw.edu.pl/contributionDisplay.py?contribId=11&sessionId=2&confId=59
LOCATION:University of Warsaw 1.40
URL:http://indico.fuw.edu.pl/contributionDisplay.py?contribId=11&sessionId
 =2&confId=59
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BEGIN:VEVENT
SUMMARY:Global fits in the coloured scalar model
DTSTART;VALUE=DATE-TIME:20190913T120000Z
DTEND;VALUE=DATE-TIME:20190913T121500Z
DTSTAMP;VALUE=DATE-TIME:20260926T112418Z
UID:indico-contribution-2-20@cern.ch
DESCRIPTION:Speakers: MIRALLES\, Victor (IFIC-UV)\nIn this work we study t
 he phenomenological constraints to the parameter space of scalars carring 
 color quantum numbers. Specifically we constrain the Manohar-Wise model ba
 sed on the addition of a SU(2) double and SU(3) octet to the minimal Higgs
  model. The fits are performed using the open source HEPfit package. We in
 clude both theoretical constraints\, such as unitarity and pertubativity\,
  and experimental constraints\, like the ones coming from flavour and elec
 troweak observables. For the first time we combine all these results and w
 e are able to constrain the parameters of the potential\, the Yukawa coupl
 ings and the masses of the scalars.\n\nhttp://indico.fuw.edu.pl/contributi
 onDisplay.py?contribId=20&sessionId=2&confId=59
LOCATION:University of Warsaw 1.40
URL:http://indico.fuw.edu.pl/contributionDisplay.py?contribId=20&sessionId
 =2&confId=59
END:VEVENT
BEGIN:VEVENT
SUMMARY:Curved spacetime effective field theory (cEFT) -- formalism and so
 me applications
DTSTART;VALUE=DATE-TIME:20190913T131500Z
DTEND;VALUE=DATE-TIME:20190913T133000Z
DTSTAMP;VALUE=DATE-TIME:20260926T112418Z
UID:indico-contribution-2-23@cern.ch
DESCRIPTION:Speakers: Dr. NAKONIECZNY\, Lukasz (Institute of Theoretical P
 hysics\, Faculty of Physics\, University of Warsaw)\nThe effective field t
 heory (EFT) turns out to be an instrument of an immense value in all aspec
 ts of modern particle physics being theory\, phenomenology or experiment. 
 In this talk I will show how to extend the systematic top down approach to
  construction of the EFT proposed by Hitoshi Murayama (LBL\, Berkeley) and
  separately by John Ellis (King’s Coll. London) groups to the curved spa
 cetime. To this end\, I will take advantage of the heat kernel method so f
 ar extensively used in obtaining the one-loop effective action in curved s
 pacetime. After an introduction of the formalism I will discuss its applic
 ation to the problem of an influence of gravity on the stability of the Hi
 ggs effective potential. The talk is based on JHEP01(2019)034.\n\nhttp://i
 ndico.fuw.edu.pl/contributionDisplay.py?contribId=23&sessionId=2&confId=59
LOCATION:University of Warsaw 1.40
URL:http://indico.fuw.edu.pl/contributionDisplay.py?contribId=23&sessionId
 =2&confId=59
END:VEVENT
BEGIN:VEVENT
SUMMARY:The effective potential method in 5D warped models
DTSTART;VALUE=DATE-TIME:20190913T123000Z
DTEND;VALUE=DATE-TIME:20190913T124500Z
DTSTAMP;VALUE=DATE-TIME:20260926T112418Z
UID:indico-contribution-2-57@cern.ch
DESCRIPTION:Speakers: Dr. MARTINEZ LIZANA\, Javier (University of Warsaw)\
 nWarped extra dimensions have been widely used in the last twenty years to
  address the hierarchy problem and construct phenomenologically viable BSM
  models. These models require some mechanism to stabilize the size of the 
 extra dimension\, which usually produces a light radion.\nA common tool  u
 sed to study the stabilization mechanism is the effective potential of the
  radion and several approximations to it. This object takes a crucial role
  in finite temperature calculations\, relevant to study possible phase tra
 nsitions that these models predict in the early universe.\nIn this talk I 
 will discuss different approximations used to compute the effective potent
 ial. I will analyze their exact meaning\, what trustable information we ca
 n extract from them\, and under what circumstances they are a good approxi
 mation to the exact solution.\n\nhttp://indico.fuw.edu.pl/contributionDisp
 lay.py?contribId=57&sessionId=2&confId=59
LOCATION:University of Warsaw 1.40
URL:http://indico.fuw.edu.pl/contributionDisplay.py?contribId=57&sessionId
 =2&confId=59
END:VEVENT
BEGIN:VEVENT
SUMMARY:Multi-peaked Gravitational footprints of neutrino mass and lepton 
 symmetry violation
DTSTART;VALUE=DATE-TIME:20190913T124500Z
DTEND;VALUE=DATE-TIME:20190913T130000Z
DTSTAMP;VALUE=DATE-TIME:20260926T112418Z
UID:indico-contribution-2-51@cern.ch
DESCRIPTION:Speakers: Dr. MORAIS\, Antonio (Aveiro University)\nWe investi
 gate the production of primordial Gravitation Waves (GWs) arising from Fir
 st Order Phase Transitions (FOPT) associated to neutrino mass generation i
 n the context of type-I seesaw models. We examine both high scale and low 
 scale variants\, with either explicit or spontaneously broken lepton numbe
 r symmetry. In the latter case\, a pseudo-Goldstone boson\, dubbed Majoron
 \, may provide a candidate for warm or cold cosmological dark matter. We h
 ave found that schemes without Majoron lead to either no FOPT or to very w
 eak FOPT\, precluding the detectability of GWs in present or near future e
 xperiments. However\, in the presence of Majorons\, one can have strong FO
 PT and non-trivial GW spectra which can fall well within the frequency and
  amplitude sensitivity range of upcoming experiments. Furthermore\, we sho
 w that in certain cases\, the resulting GW spectra entail as characteristi
 c features double or multiple peaks at the reach of future experiments. Ou
 r analysis shows that GWs can provide a new and complementary portal to te
 st the neutrino mass sector.\n\nhttp://indico.fuw.edu.pl/contributionDispl
 ay.py?contribId=51&sessionId=2&confId=59
LOCATION:University of Warsaw 1.40
URL:http://indico.fuw.edu.pl/contributionDisplay.py?contribId=51&sessionId
 =2&confId=59
END:VEVENT
BEGIN:VEVENT
SUMMARY:Stopping the dynamical relaxation by a particle production
DTSTART;VALUE=DATE-TIME:20190913T130000Z
DTEND;VALUE=DATE-TIME:20190913T131500Z
DTSTAMP;VALUE=DATE-TIME:20260926T112418Z
UID:indico-contribution-2-62@cern.ch
DESCRIPTION:Speakers: Mr. MARKIEWICZ\, Adam (University of Warsaw)\nDynami
 c relaxation provides an interesting framework which intends to solve the 
 hierarchy problem by postulating\, that the observed value of the electrow
 eak scale was determined dynamically in the early Universe. Values of the 
 electroweak scale were scanned during an evolution of axion-like field (a 
 relaxion)\, with a stopping mechanism responsible for fixing the scale at 
 a small value. \n\nThe original relaxation proposal depended on an ongoing
  inflation\, putting significant constraints on the inflationary sector. S
 ince then alternative variants of relaxation were proposed\, which allow t
 o decouple it from inflation completely. In these scenarios relaxation is 
 stopped though a burst of particle production which happens when the relax
 ion enters a non-adiabatic region. \n\nQualitative and analytical approach
  can tell us a lot about the viability of such relaxation models. It is ho
 wever still interesting to track the relaxation process in detail\, which 
 can only be done numerically. In this talk we will present our work toward
 s such analysis done with a goal of investigating a subtle interplay betwe
 en the relaxion\, the electroweak scale\, and the produced particles.\n\nh
 ttp://indico.fuw.edu.pl/contributionDisplay.py?contribId=62&sessionId=2&co
 nfId=59
LOCATION:University of Warsaw 1.40
URL:http://indico.fuw.edu.pl/contributionDisplay.py?contribId=62&sessionId
 =2&confId=59
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