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CERN Document Server 8 εγγραφές βρέθηκαν  Η έρευνα πήρε 0.61 δευτερόλεπτα. 
1.
Report of the Topical Group on Physics Beyond the Standard Model at Energy Frontier for Snowmass 2021 / Bose, Tulika (Wisconsin U., Madison) ; Boveia, Antonio (Ohio State U., CCAPP) ; Doglioni, Caterina (Manchester U.) ; Griso, Simone Pagan (LBNL, Berkeley ; Sao Paulo, IFT) ; Hirschauer, James (Fermilab) ; Lipeles, Elliot (Pennsylvania U.) ; Liu, Zhen (Minnesota U.) ; Shah, Nausheen R. (Wayne State U.) ; Wang, Lian-Tao (Chicago U., EFI ; Chicago U., KICP) ; Agashe, Kaustubh (Maryland U.) et al.
This is the Snowmass2021 Energy Frontier (EF) Beyond the Standard Model (BSM) report. [...]
arXiv:2209.13128 ; FERMILAB-FN-1204-AD-QIS-SCD. - 108.
Fermilab Library Server - eConf - Fulltext - Fulltext
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2.
The International Linear Collider: Report to Snowmass 2021 / ILC International Development Team Collaboration
The International Linear Collider (ILC) is on the table now as a new global energy-frontier accelerator laboratory taking data in the 2030s. [...]
arXiv:2203.07622 ; DESY-22-045 ; IFT-UAM/CSIC-22-028 ; KEK Preprint 2021-61 ; IFT--UAM/CSIC--22-028 ; KEK Preprint 2021-61, PNNL-SA-160884 ; SLAC-PUB-17662 ; FERMILAB-FN-1171-PPD-QIS-SCD-TD ; PNNL-SA-160884. - 356.
Fermilab Library Server - eConf - FUlltext - Fulltext
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3.
Impact of a XENONnT signal on LHC dijet searches / Baum, Sebastian (Stockholm U., OKC ; Nordita ; Royal Inst. Tech., Stockholm) ; Catena, Riccardo (Chalmers U. Tech.) ; Krauss, Martin B. (Chalmers U. Tech. ; Rome III U.)
It is well-known that dark matter (DM) direct detection experiments and the LHC are complementary, since they probe physical processes occurring at different energy scales. And yet, there are aspects of this complementarity which are still not fully understood, or exploited. [...]
arXiv:1812.01594.- 2019-07-03 - 23 p. - Published in : JHEP 1907 (2019) 015 Article from SCOAP3: scoap3-fulltext - PDF; scoap - PDF; Fulltext: PDF;
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4.
Measuring Changes in the Atmospheric Neutrino Rate Over Gigayear Timescales / Jordan, Johnathon R. (Michigan U.) ; Baum, Sebastian (Stanford U. ; Stockholm U., OKC) ; Stengel, Patrick (Stockholm U., OKC) ; Ferrari, Alfredo (CERN) ; Morone, Maria Cristina (Rome U., Tor Vergata ; INFN, Rome) ; Sala, Paola (INFN, Milan) ; Spitz, Joshua (Michigan U.)
Measuring the cosmic ray flux over timescales comparable to the age of the solar system, $\sim 4.5\,$Gyr, could provide a new window on the history of the Earth, the solar system, and even our galaxy. We present a technique to indirectly measure the rate of cosmic rays as a function of time using the imprints of atmospheric neutrinos in paleo-detectors, natural minerals which record damage tracks from nuclear recoils. [...]
arXiv:2004.08394.- 2020-11-30 - 6 p. - Published in : Phys. Rev. Lett. 125 (2020) 231802 Article from SCOAP3: PDF; Fulltext: PDF;
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5.
First Results on the Search for Chameleons with the KWISP Detector at CAST / Arguedas Cuendis, S. (CERN) ; Baier, J. (Freiburg U.) ; Barth, K. (CERN) ; Baum, S. (Royal Inst. Tech., Stockholm ; Stockholm U., OKC ; Nordita) ; Bayirli, A. (Istanbul U.) ; Belov, A. (Moscow, INR) ; Bräuninger, H. (Garching, Max Planck Inst., MPE) ; Cantatore, G. (INFN, Trieste ; Trieste U.) ; Carmona, J.M. (Zaragoza U.) ; Castel, J.F. (Zaragoza U.) et al.
We report on a first measurement with a sensitive opto-mechanical force sensor designed for the direct detection of coupling of real chameleons to matter. These dark energy candidates could be produced in the Sun and stream unimpeded to Earth. [...]
arXiv:1906.01084.- 2019-12 - 21 p. - Published in : Phys. Dark Univ. 26 (2019) 100367 Fulltext: 1-s2.0-S2212686419301517-main - PDF; 1906.01084 - PDF; Fulltext from Publisher: PDF;
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6.
Detecting solar chameleons through radiation pressure / Baum, S. (Uppsala U. ; CERN) ; Cantatore, G. (Trieste U. ; INFN, Trieste) ; Hoffmann, D.H.H. (Darmstadt, Tech. Hochsch.) ; Karuza, M. (INFN, Trieste ; Rijeka U.) ; Semertzidis, Y.K. (KISTI, Daejeon ; KAIST, Taejon) ; Upadhye, A. (Wisconsin U., Madison) ; Zioutas, K. (CERN ; Patras U.)
Light scalar fields can drive the accelerated expansion of the universe. Hence, they are obvious dark energy candidates. [...]
arXiv:1409.3852.- 2014-10-24 - 6 p. - Published in : Phys. Lett. B 739 (2014) 167-173 Article from SCOAP3: PDF; Elsevier Open Access article : PDF; Fulltext: S0370269314007886 - XML; arXiv:1409.3852 - PDF;
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7.
Detecting solar chameleons through radiation pressure / Baum, Sebastian (Uppsala Universitet, CERN)
Light scalar fields can drive accelerated expansion of the universe. [...]
CERN-STUDENTS-Note-2014-133. - 2014
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8.
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Looking for chameleons / BAUM, Sebastian (speaker)
2014 - 1412. Summer Student Lecture Programme General; Student Session External links: Talk details; Event details In : Student Session
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Δείτε ακόμη: παρόμοια ονόματα συγγραφέων
7 BAUM, Sebastian
16 Baum, S
89 Baum, S A
7 Baum, Sebastian
1 Baum, Seth
2 Baum, Seth D
3 Baum, Stefi
27 Baum, Stefi A
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