Searching for Axion-Like Particles with X-Ray Polarimeters
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European Astroparticle Physics Strategy 2017-2026 Astroparticle Physics European Consortium
European Astroparticle Physics Strategy 2017-2026 Astroparticle Physics European Consortium August 2017 European Astroparticle Physics Strategy 2017-2026 www.appec.org Executive Summary Astroparticle physics is the fascinating field of research long-standing mysteries such as the true nature of Dark at the intersection of astronomy, particle physics and Matter and Dark Energy, the intricacies of neutrinos cosmology. It simultaneously addresses challenging and the occurrence (or non-occurrence) of proton questions relating to the micro-cosmos (the world decay. of elementary particles and their fundamental interactions) and the macro-cosmos (the world of The field of astroparticle physics has quickly celestial objects and their evolution) and, as a result, established itself as an extremely successful endeavour. is well-placed to advance our understanding of the Since 2001 four Nobel Prizes (2002, 2006, 2011 and Universe beyond the Standard Model of particle physics 2015) have been awarded to astroparticle physics and and the Big Bang Model of cosmology. the recent – revolutionary – first direct detections of gravitational waves is literally opening an entirely new One of its paths is targeted at a better understanding and exhilarating window onto our Universe. We look of cataclysmic events such as: supernovas – the titanic forward to an equally exciting and productive future. explosions marking the final evolutionary stage of massive stars; mergers of multi-solar-mass black-hole Many of the next generation of astroparticle physics or neutron-star binaries; and, most compelling of all, research infrastructures require substantial capital the violent birth and subsequent evolution of our infant investment and, for Europe to remain competitive Universe. -
The Puzzling Nature of Dwarf-Sized Gas Poor Disk Galaxies
Dissertation submitted to the Department of Physics Combined Faculties of the Astronomy Division Natural Sciences and Mathematics University of Oulu Ruperto-Carola-University Oulu, Finland Heidelberg, Germany for the degree of Doctor of Natural Sciences Put forward by Joachim Janz born in: Heidelberg, Germany Public defense: January 25, 2013 in Oulu, Finland THE PUZZLING NATURE OF DWARF-SIZED GAS POOR DISK GALAXIES Preliminary examiners: Pekka Heinämäki Helmut Jerjen Opponent: Laura Ferrarese Joachim Janz: The puzzling nature of dwarf-sized gas poor disk galaxies, c 2012 advisors: Dr. Eija Laurikainen Dr. Thorsten Lisker Prof. Heikki Salo Oulu, 2012 ABSTRACT Early-type dwarf galaxies were originally described as elliptical feature-less galax- ies. However, later disk signatures were revealed in some of them. In fact, it is still disputed whether they follow photometric scaling relations similar to giant elliptical galaxies or whether they are rather formed in transformations of late- type galaxies induced by the galaxy cluster environment. The early-type dwarf galaxies are the most abundant galaxy type in clusters, and their low-mass make them susceptible to processes that let galaxies evolve. Therefore, they are well- suited as probes of galaxy evolution. In this thesis we explore possible relationships and evolutionary links of early- type dwarfs to other galaxy types. We observed a sample of 121 galaxies and obtained deep near-infrared images. For analyzing the morphology of these galaxies, we apply two-dimensional multicomponent fitting to the data. This is done for the first time for a large sample of early-type dwarfs. A large fraction of the galaxies is shown to have complex multicomponent structures. -
Icecube Searches for Neutrinos from Dark Matter Annihilations in the Sun and Cosmic Accelerators
UNIVERSITE´ DE GENEVE` FACULTE´ DES SCIENCES Section de physique Professeur Teresa Montaruli D´epartement de physique nucl´eaireet corpusculaire IceCube searches for neutrinos from dark matter annihilations in the Sun and cosmic accelerators. THESE` pr´esent´ee`ala Facult´edes sciences de l'Universit´ede Gen`eve pour obtenir le grade de Docteur `essciences, mention physique par M. Rameez de Kozhikode, Kerala (India) Th`eseN◦ 4923 GENEVE` 2016 i Declaration of Authorship I, Mohamed Rameez, declare that this thesis titled, 'IceCube searches for neutrinos from dark matter annihilations in the Sun and cosmic accelerators.' and the work presented in it are my own. I confirm that: This work was done wholly or mainly while in candidature for a research degree at this University. Where any part of this thesis has previously been submitted for a degree or any other qualifica- tion at this University or any other institution, this has been clearly stated. Where I have consulted the published work of others, this is always clearly attributed. Where I have quoted from the work of others, the source is always given. With the exception of such quotations, this thesis is entirely my own work. I have acknowledged all main sources of help. Where the thesis is based on work done by myself jointly with others, I have made clear exactly what was done by others and what I have contributed myself. Signed: Date: 27 April 2016 ii UNIVERSITE´ DE GENEVE` Abstract Section de Physique D´epartement de physique nucl´eaireet corpusculaire Doctor of Philosophy IceCube searches for neutrinos from dark matter annihilations in the Sun and cosmic accelerators. -
Why Gravity Cannot Be Quantized Canonically, and What We Can We Do About It
WHY GRAVITY CANNOT BE QUANTIZED CANONICALLY, AND WHAT WE CAN WE DO ABOUT IT Philip D. Mannheim Department of Physics University of Connecticut Presentation at Miami 2013, Fort Lauderdale December 2013 1 GHOST PROBLEMS, UNITARITY OF FOURTH-ORDER THEORIES AND PT QUANTUM MECHANICS 1. P. D. Mannheim and A. Davidson, Fourth order theories without ghosts, January 2000 (arXiv:0001115 [hep-th]). 2. P. D. Mannheim and A. Davidson, Dirac quantization of the Pais-Uhlenbeck fourth order oscillator, Phys. Rev. A 71, 042110 (2005). (0408104 [hep-th]). 3. P. D. Mannheim, Solution to the ghost problem in fourth order derivative theories, Found. Phys. 37, 532 (2007). (arXiv:0608154 [hep-th]). 4. C. M. Bender and P. D. Mannheim, No-ghost theorem for the fourth-order derivative Pais-Uhlenbeck oscillator model, Phys. Rev. Lett. 100, 110402 (2008). (arXiv:0706.0207 [hep-th]). 5. C. M. Bender and P. D. Mannheim, Giving up the ghost, Jour. Phys. A 41, 304018 (2008). (arXiv:0807.2607 [hep-th]) 6. C. M. Bender and P. D. Mannheim, Exactly solvable PT-symmetric Hamiltonian having no Hermitian counterpart, Phys. Rev. D 78, 025022 (2008). (arXiv:0804.4190 [hep-th]) 7. C. M. Bender and P. D. Mannheim, PT symmetry and necessary and sufficient conditions for the reality of energy eigenvalues, Phys. Lett. A 374, 1616 (2010). (arXiv:0902.1365 [hep-th]) 8. P. D. Mannheim, PT symmetry as a necessary and sufficient condition for unitary time evolution, Phil. Trans. Roy. Soc. A. 371, 20120060 (2013). (arXiv:0912.2635 [hep-th]) 9. C. M. Bender and P. D. Mannheim, PT symmetry in relativistic quantum mechanics, Phys. -
ALESSANDRA CORSI Curriculum Vitae Et Studiorum
ALESSANDRA CORSI Curriculum Vitae et Studiorum Contact information • Post: Texas Tech University, Physics Department, Box 41051, Lubbock, TX 79409-1051 • e-mail: [email protected] • Phone: +1-806-834-6931 (Office) Education • 2007: Astronomy Ph.D, University of Rome Sapienza. Thesis title: \Gamma-ray Burst afterglows: fireball physics and clues to the progenitor" - Advisors: Prof. Enrico Massaro and Dr. Luigi Piro. • 2003: Laurea in Physics cum laude, University of Rome Sapienza. Academic positions • 2014 (August) - present: Assistant Professor of Physics, Texas Tech University. • 2012 - 2014 (July): Assistant Professor of Physics, The George Washington University. • 2010 - 2012: Post-doc, California Institute of Technology (Advisors: Prof. Alan J. Weinstein and Prof. Shrinivas R. Kulkarni). • 2008 - 2010: Post-doc, University of Rome Sapienza & Pennsylvania State University (Advisors: Prof. Fulvio Ricci and Prof. Peter Meszaros). • 2007 - 2008: Post-doc, National Institute for Astrophysics (INAF/IASF-Rome) and Rome Univer- sity Sapienza (Advisors: Dr. Luigi Piro and Prof. Fulvio Ricci). Professional Memberships • American Astronomical Society, member since 2013. • American Physical Society, member since 2012. • LIGO Scientific Collaboration, member since 2010. • Palomar Transient Factory Collaboration, member since 2010. • Virgo Collaboration, 2007-2010. Honors, Awards & Scholarships • AAS Bruno Rossi Prize for high-energy astrophysics (as part of the LSC; 2017). • UK Royal Astronomical Society Group Achievement Award in Astronomy (as part of the LSC; 2017). • Honorary Adjunct Assistant Professor, TTU Department of Mathematics and Statistics (2016). • Gruber Cosmology Prize (as part of the LSC; 2016). • Special Breakthrough Prize in Fundamental Physics (as part of the LSC; 2016). • Fellow of the Research Corporation for Science Advancement (Scialog) (TDA, 2015-2016). -
Working Document for the Creation of a Doctorate in Archaeoastronomy and Astrophysics in the UNSAAC of Cusco
Working Document for the creation of a Doctorate in Archaeoastronomy and Astrophysics in the UNSAAC of Cusco Working Document for the creation of a Doctorate in Archaeoastronomy and Astrophysics in the UNSAAC of Cusco Introduction The First International Congress on Astrophysics and Archeology of the UNSAAC was held on the Auditorium of the Faculty of Science on July 4, 5 and 6, 2019 with the presence of local professors, foreign guests, students and university authorities with the programming in annex . The objective of this event was to discuss and shape a proposal for the creation of a Postgraduate degree in Archaeoastronomy and Astrophysics at the Doctorate level, giving a strong boost to human resources research and training activities at UNSAAC. The initiative of the meeting had the contribution of several teachers of the institution, from the first contacts made by the meeting coordinator (CZV) with Professor Milton Rojas Gamarra, in Ollantaytambo, in 2018, during the IWARA2018 meeting (8th International Workshop on Astronomy and Relativistic Astrophysics), until the later stages that culminated with the writing of this proposal. Among the various professors involved in the different stages of the meeting, we highlight the relevant participation of professors Marco Antonio Zamalloa Jara, Milton Rojas Gamarra, Miriam H. Romero Peña, Pastor Raúl Chura Serrano, Sayri Tupac García Roca and Victor Ayma. We also cite the extremely important contribution of the UNSAAC authorities. The full nominate is: Dr. Gilbert Alagon Huallpa (Vice Chancellor for Research), Dr. Alejandro Ttito Ttica (Dean of the Faculty of Science), Dr. Edilberto Atau Enriquez (Director of the Professional School of Physics), Dr. -
Searches for Leptophilic Dark Matter with Astrophysical Experiments
. Searches for leptophilic dark matter with astrophysical experiments . Von der Fakult¨atf¨urMathematik, Informatik und Naturwissenschaften der RWTH Aachen University zur Erlangung des akademischen Grades einer Doktorin der Naturwissenschaften genehmigte Dissertation vorgelegt von M. Sc. Leila Ali Cavasonza aus Finale Ligure, Savona, Italien Berichter: Universit¨atsprofessorDr. rer. nat. Michael Kr¨amer Universit¨atsprofessorDr. rer. nat. Stefan Schael Tag der m¨undlichen Pr¨ufung: 13.05.16 Diese Dissertation ist auf den Internetseiten der Universit¨atsbibliothekonline verf¨ugbar RWTH Aachen University Leila Ali Cavasonza Institut f¨urTheoretische Teilchenphysik und Kosmologie Searches for leptophilic dark matter with astrophysical experiments PhD Thesis February 2016 Supervisors: Prof. Dr. Michael Kr¨amer Prof. Dr. Stefan Schael Zusammenfassung Suche nach leptophilischer dunkler Materie mit astrophysikalischen Experimenten Die Natur der dunklen Materie (DM) zu verstehen ist eines der wichtigsten Ziele der Teilchen- und Astroteilchenphysik. Große experimentelle Anstrengungen werden un- ternommen, um die dunkle Materie nachzuweisen, in der Annahme, dass sie neben der Gravitationswechselwirkung eine weitere Wechselwirkung mit gew¨ohnlicher Materie hat. Die dunkle Materie in unserer Galaxie k¨onnte gew¨ohnliche Teilchen durch An- nihilationsprozesse erzeugen und der kosmischen Strahlung einen zus¨atzlichen Beitrag hinzuf¨ugen.Deswegen sind pr¨aziseMessungen der Fl¨ussekosmischer Strahlung ¨außerst wichtig. Das AMS-02 Experiment misst die -
Analysis of Repulsive Central Universal Force Field on Solar and Galactic
Open Phys. 2019; 17:364–372 Research Article Kamal Barghout* Analysis of repulsive central universal force field on solar and galactic dynamics https://doi.org/10.1515/phys-2019-0041 otic matter-energy to the matter side of Einstein field equa- Received Jun 30, 2018; accepted Apr 02, 2019 tions, dubbed “dark matter” and “dark energy”; see [5] and references therein. Abstract: Recent astrophysical observations hint toward The existence of dark matter is mostly inferred from the need for an extended theory of gravity to explain puz- gravitational effects on visible matter and is thought toac- zles presented by the standard cosmological model such count for approximately 85% of the matter in the universe as the need for dark matter and dark energy to understand while dark energy is inferred from the accelerated expan- the dynamics of the cosmos. This paper investigates the ef- sion of the universe and along with dark matter constitutes fect of a repulsive central universal force field on the be- about 95% of the total mass-energy content in the universe. havior of celestial objects. Negative tidal effect on the solar The origin of dark matter is a mystery and a wide range and galactic orbits, like that experienced by Pioneer space- of theories speculate its type, its particle’s mass, its self- crafts, was derived from the central force and was shown to interaction and its interaction with normal matter. Also, manifest itself as dark matter and dark energy. Vertical os- experiments to directly detect dark matter particles in the cillation of the sun about the galactic plane was modeled lab have failed to produce positive results which presents a as simple harmonic motion driven by the repulsive force. -
1 Paolo BERNARDINI - Elenco Completo Delle Pubblicazioni (September 2, 2021)
1 Paolo BERNARDINI - elenco completo delle pubblicazioni (September 2, 2021) PUBBLICAZIONI SU RIVISTA [1] P. Bernardini \La statistica di Einstein e la seconda quantizzazione: quale continuit`a?", Physis 23 (1981) 337 [2] P. Bernardini "Pascual Jordan, interprete coerente dell'ipotesi quantistica", Testi e Contesti 5 (1981) 85 [3] I. Boscolo, J. Gallardo, P. Bernardini \Free Electron Laser Features in Small-Signal Regime with a Gaussian Mode", Nuclear Instruments and Methods A 237 (1985) 69 [4] P. Bernardini, F. Grianti, F. Vetrano \Un sistema idraulico come filtro passa-basso", Studi Urbinati C 27 (1985) 61 [5] I. Boscolo, P. Bernardini, A. Pando, A. Passaseo \A High Power CH3OH Laser System with Long-Term Stability", International Journal of Infrared and Millimeter Waves 7 (1986) 1677 [6] I. Boscolo, P. Bernardini, A. Passaseo \A Powerful and Stable CO2 Laser for CH3OH FIR Laser Optical Pumping", Infrared Physics 26 (1986) 287 [7] P. Bernardini, F. Grianti, F. Vetrano \A Mechanical Ventilator with Programable Flow Waveforms", Rassegna di Bioingegneria 11 (1986) 99 [8] P. Bernardini, F. Vetrano \Esperienza didattica su un sistema idraulico: analisi del sistema e analogie con un circuito elettrico", Giornale di Fisica 28 (1987) 33 [9] P. Bernardini, R. Mantovani, F. Vetrano \Determinazione dell'ordine di grandezza del coefficiente di viscosit`adell'aria", Studi Urbinati C 29 (1987) 97 [10] P. Bernardini, R. Mantovani, F. Vetrano \Dieci Strumenti dell'Antico Laboratorio di Fisica dell'Universit`aUrbinate", Studi Urbinati C 29 (1987) 115 [11] F. Baldetti, P. Bernardini, F. Grianti, F. Vetrano \Analisi dei vincoli imposti ad una particolare discretizzazione della curva di flusso nella ventilazione automatica programmabile", Automazione e Strumentazione 35/12 (1987) 153 [12] I. -
Dark Matter Searches Targeting Dwarf Spheroidal Galaxies with the Fermi Large Area Telescope
Doctoral Thesis in Physics Dark Matter searches targeting Dwarf Spheroidal Galaxies with the Fermi Large Area Telescope Maja Garde Lindholm Oskar Klein Centre for Cosmoparticle Physics and Cosmology, Particle Astrophysics and String Theory Department of Physics Stockholm University SE-106 91 Stockholm Stockholm, Sweden 2015 Cover image: Top left: Optical image of the Carina dwarf galaxy. Credit: ESO/G. Bono & CTIO. Top center: Optical image of the Fornax dwarf galaxy. Credit: ESO/Digitized Sky Survey 2. Top right: Optical image of the Sculptor dwarf galaxy. Credit:ESO/Digitized Sky Survey 2. Bottom images are corresponding count maps from the Fermi Large Area Tele- scope. Figures 1.1a, 1.2, 1.3, and 4.2 used with permission. ISBN 978-91-7649-224-6 (pp. i{xxii, 1{120) pp. i{xxii, 1{120 c Maja Garde Lindholm, 2015 Printed by Publit, Stockholm, Sweden, 2015. Typeset in pdfLATEX Abstract In this thesis I present our recent work on gamma-ray searches for dark matter with the Fermi Large Area Telescope (Fermi-LAT). We have tar- geted dwarf spheroidal galaxies since they are very dark matter dominated systems, and we have developed a novel joint likelihood method to com- bine the observations of a set of targets. In the first iteration of the joint likelihood analysis, 10 dwarf spheroidal galaxies are targeted and 2 years of Fermi-LAT data is analyzed. The re- sulting upper limits on the dark matter annihilation cross-section range 26 3 1 from about 10− cm s− for dark matter masses of 5 GeV to about 5 10 23 cm3 s 1 for dark matter masses of 1 TeV, depending on the × − − annihilation channel. -
Título Do Projeto
Search for new physics in light of interparticle potentials and a very heavy dark matter candidate Felipe Almeida Gomes Ferreira Supervisor: Prof. Carsten Hensel Rio de Janeiro, July 2019 List of Publications This thesis is based on the following scientific articles: • Manuel Drees and Felipe A. Gomes Ferreira, A very heavy sneutrino as vi- able thermal dark matter candidate in U(1)0 extensions of the MSSM, JHEP04(2019)167 [arXiv:1711.00038]. • F. A. Gomes Ferreira, P. C. Malta, L. P. R. Ospedal and J. A. Helayël-Neto, Topologically Massive Spin-1 Particles and Spin-Dependent Potentials, Eur.Phys.J. C75 (2015) no.5, 238 [arXiv:1411.3991]. ii Abstract It is generally well known that the Standard Model of particle physics is not the ul- timate theory of fundamental interactions as it has inumerous unsolved problems, so it must be extended. Deciphering the nature of dark matter remains one of the great chal- lenges of contemporary physics. Supersymmetry is probably the most attractive extension of the SM as it can simultaneously provide a natural solution to the hierarchy problem and unify the gauge couplings at the GUT scale in such a way that doesn’t affect its low-energy phenomenology. Furthermore, the lightest supersymmetric particle is one of the most popular candidates for the dark matter particle. In the first part of this thesis we study the interparticle potentials generated bythe interactions between spin-1/2 sources that are mediated by spin-1 particles in the limit of low momentum transfer. We investigate different representations of spin-1 particle to see how it modifies the profiles of the interparticle potentials and we also include inour analysis all types of couplings between fermionic currents and the mediator boson. -
Astroparticle Astroparticle Physics
AstroparticleAstroparticleAstroparticle PhysicsPhysicsPhysics Summerstudent Lecture 2010 Axel Lindner DESY e-mail: [email protected] A. Lindner Summer Student Lecture 2010 Astroparticle Physics AstroparticleAstroparticleAstroparticle Physics:Physics:Physics: HistoryHistoryHistory High energy physics started with discoveries and analysis of particles generated by the cosmic radiation in the atmosphere. • 1932: Positron • 1937: Muons • 1947: Pions, Λ, K • 1952: Ξ-, Σ+ • 1971: Charm (?) • 1998: Neutrino oscillation SK 2005 A. Lindner Summer Student Lecture 2010 Astroparticle Physics AstroparticleAstroparticleAstroparticle Physics:Physics:Physics: CosmicCosmicCosmic LaboratoryLaboratoryLaboratory Really high energies are only provided by the cosmos: • particles beyond 1020eV (107·LHC beam energy) • Access to physics at the Planck scale via indirect observations of the very early universe Really long baselines are only provided by the cosmos: • Oscillation of υ from the sun: 150·109 m • υ from SN 1987A (LMC): 150.000 light-years A. Lindner Summer Student Lecture 2010 Astroparticle Physics AstroparticleAstroparticleAstroparticle Physics:Physics:Physics: PhenomenaPhenomenaPhenomena There are many natural phenomena waiting for explanation: • Cosmic Radiation • Dark Matter • Cosmic Microwave Background Radiation The cosmic connection: • The development (and origin?) of the cosmos can only be addressed with HEP knowledge A. Lindner Summer Student Lecture 2010 Astroparticle Physics A. Lindner Summer Student Lecture 2010 Astroparticle Physics