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.
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[Amsterdam], : Atlantis, 2016 | ||
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Lo trovi qui: Univ. Vanvitelli | ||
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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
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Berlin ; ; Boston, : De Gruyter, c2012 | ||
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Lo trovi qui: Univ. Federico II | ||
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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
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Berlin ; ; Boston, : De Gruyter, c2012 | ||
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Lo trovi qui: Univ. Federico II | ||
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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
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Singapore : , : World Scientific Publishing Company, , 2018 | ||
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Lo trovi qui: Univ. Federico II | ||
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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 | ||
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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 |
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
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Cham, : Springer, 2016 | ||
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Lo trovi qui: Univ. Vanvitelli | ||
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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
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Frontiers Media SA, 2020 | ||
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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 |
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 | ||
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Lo trovi qui: Univ. Vanvitelli | ||
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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 | ||
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Lo trovi qui: Univ. Vanvitelli | ||
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