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Models for physics of the very small and very large / Thomas J. Buckholtz
Models for physics of the very small and very large / Thomas J. Buckholtz
Autore Buckholtz, Thomas J.
Pubbl/distr/stampa [Amsterdam], : Atlantis, 2016
Descrizione fisica XII, 382 p. : ill. ; 24 cm
Soggetto topico 00A79 (77-XX) - Physics [MSC 2020]
Soggetto non controllato Beyond the standard model
Cosmology
Dark Matter
Elementary Particles
Mathematical physics
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Titolo uniforme
Record Nr. UNICAMPANIA-VAN0114992
Buckholtz, Thomas J.  
[Amsterdam], : Atlantis, 2016
Materiale a stampa
Lo trovi qui: Univ. Vanvitelli
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Paths to dark energy [[electronic resource] ] : theory and observation / / Gene Byrd ... [et al.]
Paths to dark energy [[electronic resource] ] : theory and observation / / Gene Byrd ... [et al.]
Autore Byrd Gene
Pubbl/distr/stampa Berlin ; ; Boston, : De Gruyter, c2012
Descrizione fisica 1 online resource (416 p.)
Disciplina 523.01
Altri autori (Persone) ByrdGene G
Collana De Gruyter Studies in Mathematical Physics
Soggetto topico Dark energy (Astronomy)
Dark matter (Astronomy)
Cosmology
Soggetto non controllato Cosmology
Dark Energy
Dark Matter
Mathematical Models
ISBN 9786613940391
1-283-62794-9
Classificazione US 2200
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Nota di contenuto Front matter -- Preface -- Contents -- Chapter 1. The start of the paths -- Chapter 2. General Relativity: apparent acceleration of gravity -- Chapter 3. Tests of General Relativity -- Chapter 4. Curved space in cosmology -- Chapter 5. Finite versus infinite universe in space and time -- Chapter 6. Cosmology and the ''first appearance'' of dark energy -- Chapter 7. Einstein's equations, critical density and dark energy -- Chapter 8. Model Universes -- Chapter 9. Dark energy discovered -- Chapter 10. Relics: cosmic microwave background (CMB) photons and neutrinos -- Chapter 11. Baryonic matter -- Chapter 12. Discovering dark matter -- Chapter 13. Dark matter and baryonic structures -- Chapter 14. Dark energy and gravitating matter from structure in the universe -- Chapter 15. The local path to dark energy -- Chapter 16. Cosmological inflation -- Chapter 17. Cosmic internal symmetry -- Bibliography -- Index
Record Nr. UNINA-9910786471203321
Byrd Gene  
Berlin ; ; Boston, : De Gruyter, c2012
Materiale a stampa
Lo trovi qui: Univ. Federico II
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Paths to dark energy [[electronic resource] ] : theory and observation / / Gene Byrd ... [et al.]
Paths to dark energy [[electronic resource] ] : theory and observation / / Gene Byrd ... [et al.]
Autore Byrd Gene
Edizione [1st ed.]
Pubbl/distr/stampa Berlin ; ; Boston, : De Gruyter, c2012
Descrizione fisica 1 online resource (416 p.)
Disciplina 523.01
Altri autori (Persone) ByrdGene G
Collana De Gruyter Studies in Mathematical Physics
Soggetto topico Dark energy (Astronomy)
Dark matter (Astronomy)
Cosmology
Soggetto non controllato Cosmology
Dark Energy
Dark Matter
Mathematical Models
ISBN 9786613940391
1-283-62794-9
Classificazione US 2200
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Nota di contenuto Front matter -- Preface -- Contents -- Chapter 1. The start of the paths -- Chapter 2. General Relativity: apparent acceleration of gravity -- Chapter 3. Tests of General Relativity -- Chapter 4. Curved space in cosmology -- Chapter 5. Finite versus infinite universe in space and time -- Chapter 6. Cosmology and the ''first appearance'' of dark energy -- Chapter 7. Einstein's equations, critical density and dark energy -- Chapter 8. Model Universes -- Chapter 9. Dark energy discovered -- Chapter 10. Relics: cosmic microwave background (CMB) photons and neutrinos -- Chapter 11. Baryonic matter -- Chapter 12. Discovering dark matter -- Chapter 13. Dark matter and baryonic structures -- Chapter 14. Dark energy and gravitating matter from structure in the universe -- Chapter 15. The local path to dark energy -- Chapter 16. Cosmological inflation -- Chapter 17. Cosmic internal symmetry -- Bibliography -- Index
Record Nr. UNINA-9910826320303321
Byrd Gene  
Berlin ; ; Boston, : De Gruyter, c2012
Materiale a stampa
Lo trovi qui: Univ. Federico II
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Science With The Cherenkov Telescope Array
Science With The Cherenkov Telescope Array
Autore The Cta Consortium
Pubbl/distr/stampa Singapore : , : World Scientific Publishing Company, , 2018
Descrizione fisica 1 electronic resource (364 p.)
Disciplina 522/.6862
Altri autori (Persone) OngRene A
The Cta Consortium
Soggetto topico Gamma ray astronomy
Astronomy
Soggetto non controllato Gamma Rays
Astrophysics
Cherenkov Telescope Array (CTA)
Cherenkov Telescopes
Astroparticle Physics
Multiwavelength
Multimessenger
Astronomy
Dark Matter
ISBN 981-327-010-1
981-327-009-8
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Nota di contenuto Intro -- Contents -- Executive Summary -- Authors -- Acknowledgements -- Chapters and Corresponding Authors -- Chapter 1. Introduction to CTA Science -- 1.1 Key Characteristics and Capabilities -- 1.1.1 Surveying Capabilities -- 1.1.2 Short Timescale Capabilities -- 1.1.3 Capabilities Beyond Gamma Rays -- 1.2 Overview of CTA Science Themes -- 1.2.1 Understanding the Origin and Role of Relativistic Cosmic Particles -- 1.2.1.1 Cosmic accelerators -- 1.2.1.2 Propagation and influence of accelerated particles -- 1.2.2 Probing Extreme Environments -- 1.2.2.1 Black holes and jets -- 1.2.2.2 Neutron stars and relativistic outflows -- 1.2.2.3 Cosmic voids -- 1.2.3 Exploring Frontiers in Physics -- 1.2.3.1 Dark matter -- 1.2.3.2 Quantum gravity and axion-like particle search -- 1.3 Community Input to the Science Case -- Chapter 2. Synergies -- 2.1 Radio to (Sub)Millimetre -- 2.2 Infrared/Optical through Ultraviolet and Transient Factories -- 2.3 X-ray -- 2.4 Sub-VHE Gamma-ray Energies -- 2.5 Complementary VHE Gamma-ray Instruments -- 2.6 VHE and UHE Neutrinos -- 2.7 Gravitational Waves -- Chapter 3. Core Programme Overview -- Chapter 4. Dark Matter Programme -- 4.1 Science Targeted -- 4.1.1 Existence of Dark Matter -- 4.1.2 Distribution of Dark Matter -- 4.1.3 The Nature of Dark Matter -- 4.1.4 Search Methods for Dark Matter -- 4.1.5 Annihilation of Dark Matter Particles -- 4.1.6 Parameters Expected for WIMP Dark Matter -- 4.1.7 Rate of Gamma Rays in Detector -- 4.2 Strategy -- 4.2.1 Milky Way -- 4.2.1.1 Description -- 4.2.1.2 Evolution of knowledge -- 4.2.1.3 Observational strategy -- 4.2.1.4 Performance -- 4.2.2 Dwarf Spheroidal Galaxies and Dark Clumps -- 4.2.2.1 Description -- 4.2.2.2 Evolution of knowledge -- 4.2.2.3 Observational strategy -- 4.2.2.4 Performance -- 4.2.3 Large Magellanic Cloud -- 4.2.3.1 Description -- 4.2.3.2 Evolution of knowledge.
4.2.3.3 Observational strategy -- 4.2.3.4 Performance -- 4.2.4 Clusters of Galaxies -- 4.2.5 Summary of Targets -- 4.3 Data Products -- Chapter 5. KSP: Galactic Centre -- 5.1 Science Targeted -- 5.1.1 Scientific Objectives -- 5.1.1.1 Revealing the nature of the central gamma-ray source -- 5.1.1.2 Diffuse VHE emission: Particle acceleration in the vicinity of the Galactic Centre -- 5.1.1.3 Exploring large-scale outflows -- 5.1.1.4 Supernova remnants, pulsar-wind nebulae, and molecular clouds -- 5.1.2 Context/Advance beyond State of the Art -- 5.1.2.1 Central engine -- 5.1.2.2 Advances in the study of diffuse emission -- 5.2 Strategy -- 5.2.1 Timeline and Sub-array Choice -- 5.2.2 Relation to other KSPs -- 5.2.3 Analysis Strategy -- 5.3 Data Products -- 5.4 Expected Performance/Return -- 5.4.1 Determination of the Nature of the Central Source -- 5.4.2 A Detailed View of the Diffuse VHE Emission -- 5.4.3 Resolving New, Previously Undetectable Sources -- 5.4.4 Search for Variability in the VHE Source Near Sgr A* -- 5.4.5 Studying the Interaction of the Central Source with Neighbouring Clouds -- 5.4.6 Science Impact -- Chapter 6. KSP: Galactic Plane Survey -- 6.1 Science Targeted -- 6.1.1 Scientific Objectives -- 6.1.2 Context/Advance beyond State of the Art -- 6.1.3 Multi-wavelength/Multi-messenger Context -- 6.1.3.1 Synergy with HAWC -- 6.1.3.2 Synergies with other instruments -- 6.2 Strategy -- 6.2.1 Observation Requirements -- 6.2.2 Targets, Observation Strategy, and Follow-ups -- 6.2.3 Relation/Importance to other KSPs -- 6.3 Data Products -- 6.4 Expected Performance/Return -- 6.4.1 Performance of the CTA GPS -- 6.4.2 Source Confusion -- 6.4.3 Summary -- Chapter 7. KSP: Large Magellanic Cloud Survey -- 7.1 Science Targeted -- 7.1.1 Scientific Objectives -- 7.1.2 Context/Advance beyond State of the Art -- 7.2 Strategy -- 7.3 Data Products.
7.4 Expected Performance/Return -- Chapter 8. KSP: Extragalactic Survey -- 8.1 Science Targeted -- 8.1.1 Scientific Objectives -- 8.1.2 Context/advance beyond state of the art -- 8.2 Strategy -- 8.2.1 Possibility of Several Pointings for a given Field of View -- 8.2.2 Shallow survey versus deep survey -- 8.2.3 Targets -- 8.3 Data Products -- 8.4 Expected Performance/Return -- 8.4.1 Method -- 8.4.2 Serendipitous Discoveries during the Construction Phase -- 8.4.3 Results after the Completion of the Survey -- 8.4.4 Participation of LSTs -- 8.4.5 Prospects for Divergent Pointing -- Chapter 9. KSP: Transients -- 9.1 Science Targeted -- 9.1.1 Scientific Objectives -- 9.1.2 Context/Advance beyond State of the Art -- 9.2 Strategy -- 9.3 Data Products -- 9.4 Expected Performance/Return -- Chapter 10. KSP: Cosmic Ray PeVatrons -- 10.1 Science Targeted -- 10.1.1 Scientific Objectives -- 10.1.2 Context/Advance beyond State of the Art -- 10.1.2.1 Hadronic mechanisms and the connection with cosmic-ray origin -- 10.2 Strategy -- 10.2.1 Targets -- 10.3 Data Products -- 10.4 Expected Performance/Return -- Chapter 11. KSP: Star Forming Systems -- 11.1 Science Targeted -- 11.1.1 Scientific Objectives -- 11.1.2 Context/Advance beyond State of the Art -- 11.1.2.1 Star-forming regions -- 11.1.2.2 Star-forming galaxies -- 11.1.2.3 Starburst galaxies -- 11.1.2.4 ULIRGs -- 11.2 Strategy -- 11.3 Data Products -- 11.4 Expected Performance/Return -- 11.4.1 Star-forming Regions -- 11.4.2 Star-forming Galaxies -- 11.4.3 Starburst Galaxies -- 11.4.4 ULIRGs -- Chapter 12. KSP: Active Galactic Nuclei -- 12.1 Science Targeted -- 12.1.1 Relativistic Jets from Supermassive Black Holes -- 12.1.1.1 What are the relevant particle acceleration and emission processes in VHE blazars? How are different blazar types related?.
12.1.1.2 What causes the observed variability in AGN from time scales of a few years down to a few minutes? -- 12.1.1.3 From where does the VHE emission of radio galaxies originate? -- 12.1.1.4 Do other classes of AGN emit VHE gamma rays? -- 12.1.2 Blazars as Probes of the Universe -- 12.1.2.1 What is the spectrum of the EBL at redshift z ∼ 0 and how does it evolve at higher redshifts? -- 12.1.2.2 What is the strength of the IGMF? -- 12.1.3 UHECRs and Fundamental Physics -- 12.1.3.1 AGN as potential sources of UHECRs -- 12.1.3.2 Can we find signatures for the existence of axion-like particles? -- 12.1.3.3 Can we rule out Lorentz Invariance Violation? -- 12.1.4 Advance beyond State of the Art -- 12.2 Strategy -- 12.2.1 Target Selection -- 12.2.1.1 Long-term monitoring -- 12.2.1.2 AGN flare programme -- 12.2.1.3 High-quality spectra -- 12.2.1.4 Time distribution model for the AGN KSP -- 12.2.2 Multi-wavelength and Multi-messenger Coverage -- 12.3 Data Products -- 12.4 Expected Performance/Return -- 12.4.1 Guaranteed Science Return -- 12.4.2 Discovery Potential -- Chapter 13. KSP: Clusters of Galaxies -- 13.1 Science Targeted -- 13.1.1 Scientific Objectives -- 13.1.2 Context/Advance beyond State of the Art -- 13.2 Strategy -- 13.2.1 Targets -- 13.3 Data Products -- 13.4 Expected Performance/Return -- Chapter 14. Capabilities beyond Gamma Rays -- 14.1 Cosmic-Ray Nuclei -- 14.2 Cosmic-Ray Electrons -- 14.3 Optical Measurements with CTA -- Chapter 15. Appendix: Simulating CTA -- References -- Glossary.
Record Nr. UNINA-9910346694803321
The Cta Consortium  
Singapore : , : World Scientific Publishing Company, , 2018
Materiale a stampa
Lo trovi qui: Univ. Federico II
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Shedding Light to the Dark Sides of the Universe: Cosmology from Strong Interactions
Shedding Light to the Dark Sides of the Universe: Cosmology from Strong Interactions
Pubbl/distr/stampa Basel, : MDPI - Multidisciplinary Digital Publishing Institute, 2022
Descrizione fisica 1 electronic resource (234 pages)
Soggetto topico Research
Physics
Soggetto non controllato dynamics of phase transitions
spinodal instability
heavy-ion collisions
neutron stars
dark energy
non-Abelian gauge theory
condensate
QCD
DGLAP equations
physics beyond the standard model
tensorgluons
extended DGLAP equations
tensorgluon splitting functions
neutron star
equation of state
many-body methods of nuclear matter
neutron-skin thickness
GW170817
Weyl gravity
renormalization group
inflation
light scalar fields
axial anomaly
SU(2) Yang-Mills thermodynamics
de-percolation of axionic lumps
cosmological and galactic dark-matter densities
cosmology
particle physics
particle symmetry
stable particles
dark matter
cosmic rays
QCD in the early universe
phase transitions
hydrodynamical evolution
equation of state of super-dense matter
classical Yang-Mills fields
Dark Energy
Dark Matter
gluon condensate
effective Yang-Mills action
cosmic inflation
ISBN 3-0365-5870-5
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Altri titoli varianti Shedding Light to the Dark Sides of the Universe
Record Nr. UNINA-9910639989103321
Basel, : MDPI - Multidisciplinary Digital Publishing Institute, 2022
Materiale a stampa
Lo trovi qui: Univ. Federico II
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The Amazing Unity of the Universe : and Its Origin in the Big Bang / Edward van den Heuvel
The Amazing Unity of the Universe : and Its Origin in the Big Bang / Edward van den Heuvel
Autore Heuvel, Edward : van den
Edizione [2. ed]
Pubbl/distr/stampa Cham, : Springer, 2016
Descrizione fisica x, 315 p. : ill. ; 24 cm
Soggetto topico 00A79 (77-XX) - Physics [MSC 2020]
85-XX - Astronomy and Astrophysics [MSC 2020]
85A40 - Cosmology [MSC 2020]
Soggetto non controllato Anthropic Principle
Big Bang
Cosmic Evolution
Cosmic Microwave Background Radiation
Cosmological Constant
Dark Energy
Dark Matter
Evolution of the Universe
Inflation of the Universe
Life in the Universe
Origin of the Universe
Structure Formation
Unity of the Universe
Vaccuum Energy
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Titolo uniforme
Record Nr. UNICAMPANIA-VAN0175625
Heuvel, Edward : van den  
Cham, : Springer, 2016
Materiale a stampa
Lo trovi qui: Univ. Vanvitelli
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The Physics Associated with Neutrino Masses
The Physics Associated with Neutrino Masses
Autore Aristizabal Sierra Diego
Pubbl/distr/stampa Frontiers Media SA, 2020
Descrizione fisica 1 electronic resource (293 p.)
Soggetto topico Science: general issues
Physics
Soggetto non controllato Neutrinos
Flavor
Colliders
Beyond the Standard Model
Dark Matter
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Record Nr. UNINA-9910557601503321
Aristizabal Sierra Diego  
Frontiers Media SA, 2020
Materiale a stampa
Lo trovi qui: Univ. Federico II
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The Renaissance of General Relativity in Context / Alexander S. Blum, Roberto Lalli, Jürgen Renn editors
The Renaissance of General Relativity in Context / Alexander S. Blum, Roberto Lalli, Jürgen Renn editors
Pubbl/distr/stampa Cham, : Birkhäuser, 2020
Descrizione fisica x, 406 p. : ill. ; 24 cm
Soggetto topico 01-XX - History and biography [MSC 2020]
01A60 - History of mathematics in the 20th century [MSC 2020]
83C05 - Einstein's equations (general structure, canonical formalism, Cauchy problems) [MSC 2020]
83-XX - Relativity and gravitational theory [MSC 2020]
85A40 - Cosmology [MSC 2020]
00B15 - Collections of articles of miscellaneous specific interest [MSC 2020]
83C56 - Dark matter and dark energy [MSC 2020]
Soggetto non controllato Dark Matter
GEO600 detector
General Relativity
Gravitation theory history
Gravitation theory in physics
Gravitation theory vs general relativity
Gravitational Waves
Gravitational physics
John Wheeler physics
Massive graviton
Max Planck Society history
Quantum gravity theory
Relativistic Astrophysics
Virgo gravitational waves
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Titolo uniforme
Record Nr. UNICAMPANIA-VAN0233692
Cham, : Birkhäuser, 2020
Materiale a stampa
Lo trovi qui: Univ. Vanvitelli
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Workshop on Frontiers in High Energy Physics 2019 : FHEP 2019 / Anjan Giri, Rukmani Mohanta editors
Workshop on Frontiers in High Energy Physics 2019 : FHEP 2019 / Anjan Giri, Rukmani Mohanta editors
Pubbl/distr/stampa Singapore, : Springer, 2020
Descrizione fisica xxviii, 471 p. : ill. ; 24 cm
Soggetto topico 00Bxx - Conference proceedings and collections of articles [MSC 2020]
85A40 - Cosmology [MSC 2020]
81V35 - Nuclear physics [MSC 2020]
81Txx - Quantum field theory; related classical field theories [MSC 2020]
Soggetto non controllato Dark Energy
Dark Matter
Flavor physics
Gravitational Waves
Hadron Collider
Non-Accelerator Probes
Particle cosmology
Particle physics
Formato Materiale a stampa
Livello bibliografico Monografia
Lingua di pubblicazione eng
Titolo uniforme
Record Nr. UNICAMPANIA-VAN0233980
Singapore, : Springer, 2020
Materiale a stampa
Lo trovi qui: Univ. Vanvitelli
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