Analysis of Repulsive Central Universal Force Field on Solar and Galactic
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Genesis Cosmology* Genesis Cosmology Is the Cosmology Model in Agreement with the Interpretive Description of the First Three Da
Genesis Cosmology* Genesis Cosmology is the cosmology model in agreement with the interpretive description of the first three days in Genesis. Genesis Cosmology is derived from the unified theory that unifies various phenomena in our universe. In Genesis, the first day involves the emergence of the separation of light and darkness from the formless, empty, and dark pre-universe, corresponding to the emergence of the current asymmetrical dual universe of the light universe with light and the dark universe without light from the simple and dark pre-universe in Genesis Cosmology. The light universe is the current observable universe, while the dark universe coexisting with the light universe is first separated from the light universe and later connected with the light universe as dark energy. In Genesis, the second day involves the separation of waters from above and below the expanse, corresponding to the separation of dark matter and baryonic matter from above and below the interface between dark matter and baryonic matter for the formation of galaxies in Genesis Cosmology. In Genesis, the third day involves the separation of sea and land where organisms appeared, corresponding to the separation of interstellar medium and star with planet where organisms were developed in Genesis Cosmology. The unified theory for Genesis Cosmology unifies various phenomena in our observable universe and other universes. In terms of cosmology, our universe starts with the 11-dimensional membrane universe followed by the 10-dimensional string universe and then by the 10-dimensional particle universe, and ends with the asymmetrical dual universe with variable dimensional particle and 4-dimensional particles. -
Chapter 8 Relationship Between Rotational Speed and Magnetic
Chapter 8 Relationship Between Rotational Speed and Magnetic Fields 8.1 Introduction It is well-known that sunspots and other solar magnetic features rotate faster than the surface plasma (Howard & Harvey, 1970). The sidereal rotation speeds of weak magnetic features and plages (Howard, Gilman, & Gilman, 1984; Komm, Howard, & Harvey, 1993), individual sunspots (Howard, Gilman, & Gilman, 1984; Sivaraman, Gupta, & Howard, 1993) and sunspot groups (Howard, 1992) have been studied for many years by different research groups by use of different observatory data (see reviews of Howard 1996 and Beck 2000). Such studies are deemed as diagnostics of subsurface conditions based on the assumption that the faster rotation of magnetic features was caused by the faster-rotating plasma in the interior where the magnetic features were anchored (Gilman & Foukal, 1979). By matching the sunspot surface speed with the solar interior rotational speed robustly derived by helioseismology (e.g., Thompson et al., 1996; Kosovichev et al., 1997; Howe et al., 2000a), several studies estimated the depth of sunspot roots for sunspots of different sizes and life spans (e.g., Hiremath, 2002; Sivaraman et al., 2003). Such studies are valuable for understanding the solar dynamo and origin of solar active regions. However, D’Silva & Howard (1994) proposed a different explanation, namely that effects of buoyancy 111 112 CHAPTER 8. ROTATIONAL SPEED AND MAGNETIC FIELDS and drag coupled with the Coriolis force during the emergence of active regions might lead to the faster rotational speed. Although many studies were done to infer the rotational speed of various solar magnetic features, the relationship between the rotational speed of the magnetic fea- tures and their magnetic strength has not yet been studied. -
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. -
Dark Matter and the Early Universe: a Review Arxiv:2104.11488V1 [Hep-Ph
Dark matter and the early Universe: a review A. Arbey and F. Mahmoudi Univ Lyon, Univ Claude Bernard Lyon 1, CNRS/IN2P3, Institut de Physique des 2 Infinis de Lyon, UMR 5822, 69622 Villeurbanne, France Theoretical Physics Department, CERN, CH-1211 Geneva 23, Switzerland Institut Universitaire de France, 103 boulevard Saint-Michel, 75005 Paris, France Abstract Dark matter represents currently an outstanding problem in both cosmology and particle physics. In this review we discuss the possible explanations for dark matter and the experimental observables which can eventually lead to the discovery of dark matter and its nature, and demonstrate the close interplay between the cosmological properties of the early Universe and the observables used to constrain dark matter models in the context of new physics beyond the Standard Model. arXiv:2104.11488v1 [hep-ph] 23 Apr 2021 1 Contents 1 Introduction 3 2 Standard Cosmological Model 3 2.1 Friedmann-Lema^ıtre-Robertson-Walker model . 4 2.2 A quick story of the Universe . 5 2.3 Big-Bang nucleosynthesis . 8 3 Dark matter(s) 9 3.1 Observational evidences . 9 3.1.1 Galaxies . 9 3.1.2 Galaxy clusters . 10 3.1.3 Large and cosmological scales . 12 3.2 Generic types of dark matter . 14 4 Beyond the standard cosmological model 16 4.1 Dark energy . 17 4.2 Inflation and reheating . 19 4.3 Other models . 20 4.4 Phase transitions . 21 5 Dark matter in particle physics 21 5.1 Dark matter and new physics . 22 5.1.1 Thermal relics . 22 5.1.2 Non-thermal relics . -
Rotating Objects Tend to Keep Rotating While Non- Rotating Objects Tend to Remain Non-Rotating
12 Rotational Motion Rotating objects tend to keep rotating while non- rotating objects tend to remain non-rotating. 12 Rotational Motion In the absence of an external force, the momentum of an object remains unchanged— conservation of momentum. In this chapter we extend the law of momentum conservation to rotation. 12 Rotational Motion 12.1 Rotational Inertia The greater the rotational inertia, the more difficult it is to change the rotational speed of an object. 1 12 Rotational Motion 12.1 Rotational Inertia Newton’s first law, the law of inertia, applies to rotating objects. • An object rotating about an internal axis tends to keep rotating about that axis. • Rotating objects tend to keep rotating, while non- rotating objects tend to remain non-rotating. • The resistance of an object to changes in its rotational motion is called rotational inertia (sometimes moment of inertia). 12 Rotational Motion 12.1 Rotational Inertia Just as it takes a force to change the linear state of motion of an object, a torque is required to change the rotational state of motion of an object. In the absence of a net torque, a rotating object keeps rotating, while a non-rotating object stays non-rotating. 12 Rotational Motion 12.1 Rotational Inertia Rotational Inertia and Mass Like inertia in the linear sense, rotational inertia depends on mass, but unlike inertia, rotational inertia depends on the distribution of the mass. The greater the distance between an object’s mass concentration and the axis of rotation, the greater the rotational inertia. 2 12 Rotational Motion 12.1 Rotational Inertia Rotational inertia depends on the distance of mass from the axis of rotation. -
Review Talks
REVIEW TALKS ALDO MORSELLI II UNIVERSITA DI ROMA "TOR VERGATA” - ITALY ARIEL SÁNCHEZ MPE - GERMANY CARLA BONIFAZI UFRJ - BRAZIL CHRISTOPHER J. CONSELICE UNIVERSITY OF NOTTINGHAM - UNITED KINGDOM JODI COOLEY SOUTHERN METHODIST UNIV. - USA KEN GANGA APC - FRANCE “THE PLANCK MISSION” The planck satellite, created to measure the anisotropies in the temperature and polarization of the cosmic microwave background, was launched in may of 2009 and has performed well. Some early, non-cmb results have been published already. The first set of cmb temperature data and papers will be released at the beginning of 2013. The full data set, including polarization, is scheduled to be made public in early 2014. Galactic and other astronomical results will continue to be released during this period. I will review the non-cmb results which have been released to date and give previews of what we hope to be able to do with the cosmological data releases. MATTHIAS STEINMETZ AIP - GERMANY NICOLAO FORNENGO UNIVERSITY OF TORINI - ITALY PAOLO SALUCCI SISSA – ITALY “DARK MATTER IN GALAXIES: LEADS TO ITS NATURE” In the past years a wealth of observations has revealed the structural properties of the Dark and Luminous mass distribution in galaxies. These have pointed out to an intriguing scenario. In spirals, the investigation of individual and coadded objects has shown that their rotation curves follow, from their centers out to their virial radii, a Universal profile (URC) that arises from a tuned combination of a stellar disk and of a dark halo. The importance of the latter component decreases with galaxy mass. Individual objects have clearly revealed that the dark halos encompassing the luminous discs have a constant density core. -
Newtonian Wormholes
Newtonian wormholes José P. S. Lemos∗ and Paulo Luz† Centro Multidisciplinar de Astrofísica - CENTRA, Departamento de Física, Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Av. Rovisco Pais 1, 1049-001 Lisboa, Portugal Abstract A wormhole solution in Newtonian gravitation, enhanced through an equation relating the Ricci scalar to the mass density, is presented. The wormhole inhabits a spherically symmetric curved space, with one throat and two asymptotically flat regions. Particle dynamics in this geometry is studied, and the three distinct dynamical radii, namely, the geodesic, circumferential, and curvature radii, appear naturally in the study of circular motion. Generic motion is also analysed. A limiting case, although inconclusive, suggests the possibility of having a Newtonian black hole in a region of finite (nonzero) size. arXiv:1409.3231v1 [gr-qc] 10 Sep 2014 ∗ [email protected] † [email protected] 1 I. INTRODUCTION When many alternative theories to general relativity are being suggested, and the grav- itational field is being theoretically and experimentally put to test, it is interesting to try an alternative to Newton’s gravitation through an unexpected but simple modification of it. The idea is to have Newtonian gravitation, not in flat space, as we are used to, but in curved space. This intriguing possibility has been suggested by Abramowicz [1]. It was noted that Newtonian gravitation in curved space, and the corresponding Newtonian dy- namics in a circle, distinguishes three radii, namely, the geodesic radius (which gives the distance from the center to its perimeter), the circumferential radius (which is given by the perimeter divided by 2π), and the curvature radius (which is Frenet’s radius of curvature of a curve, in this case a circle). -
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. -
Dark Matter As a Metric Perturbation
Preprints (www.preprints.org) | NOT PEER-REVIEWED | Posted: 16 November 2016 doi:10.20944/preprints201611.0080.v1 Article Dark Matter as a Metric Perturbation W. M. Stuckey 1*, Timothy McDevitt 2, A. K. Sten 1 and Michael Silberstein 3,4 1 Department of Physics, Elizabethtown College, Elizabethtown, PA 17022, USA 2 Department of Mathematics, Elizabethtown College, Elizabethtown, PA 17022, USA 3 Department of Philosophy, Elizabethtown College, Elizabethtown, PA 17022, USA 4 Department of Philosophy, University of Maryland, College Park, MD 20742, USA * Correspondence: [email protected]; Tel.: +1-717-361-1436 Abstract: Since general relativity (GR) has already established that matter can simultaneously have two different values of mass depending on its context, we argue that the missing mass attributed to non-baryonic dark matter (DM) actually obtains because there are two different values of mass for the baryonic matter involved. The globally obtained “dynamical mass” of baryonic matter can be understood as a small perturbation to a background spacetime metric even though it’s much larger than the locally obtained “proper mass.” Having successfully fit the SCP Union2.1 SN Ia data without accelerating expansion or a cosmological constant, we employ the same ansatz to compute dynamical mass from proper mass and explain galactic rotation curves (THINGS data), the mass profiles of X-ray clusters (ROSAT and ASCA data) and the angular power spectrum of the cosmic microwave background (Planck 2015 data) without DM. We compare our fits to modified Newtonian dynamics (MOND), metric skew-tensor gravity (MSTG) and scalar-tensor-vector gravity (STVG) for each data set, respectively, since these modified gravity programs are known to generate good fits to these data. -
Collapsed Dark Matter Structures
Collapsed Dark Matter Structures Matthew R. Buckley and Anthony DiFranzo Department of Physics and Astronomy, Rutgers University, Piscataway, NJ 08854, USA (Dated: February 14, 2018) The distributions of dark matter and baryons in the Universe are known to be very different: the dark matter resides in extended halos, while a significant fraction of the baryons have radiated away much of their initial energy and fallen deep into the potential wells. This difference in morphology leads to the widely held conclusion that dark matter cannot cool and collapse on any scale. We revisit this assumption, and show that a simple model where dark matter is charged under a \dark electromagnetism" can allow dark matter to form gravitationally collapsed objects with characteris- tic mass scales much smaller than that of a Milky Way-type galaxy. Though the majority of the dark matter in spiral galaxies would remain in the halo, such a model opens the possibility that galaxies and their associated dark matter play host to a significant number of collapsed substructures. The observational signatures of such structures are not well explored, but potentially interesting. Though dark matter outmasses the baryons five-to-one Outside it, the characteristic cooling time is longer than [1], we typically assume the baryonic components are far the infall time. As a result, little of the kinetic and po- more complex than their dark matter equivalents. While tential energy in the halo is lost. Thus, it is completely some of this is certainly due to baryonic chauvinism, it possible for compact objects to form at the scale of, say 6 is clear from rotation curves and lensing measurements 10 M and below, while above this scale, no significant 9 that, at the mass scales of dwarf galaxies (∼10 M ) and deviation from CDM would be seen, despite 100% of the above, dark matter resides in approximately spherical dark matter having the same set of non-gravitational in- \halos" whose shapes are consistent with primordial over- teractions. -
Exploring Robotics Joel Kammet Supplemental Notes on Gear Ratios
CORC 3303 – Exploring Robotics Joel Kammet Supplemental notes on gear ratios, torque and speed Vocabulary SI (Système International d'Unités) – the metric system force torque axis moment arm acceleration gear ratio newton – Si unit of force meter – SI unit of distance newton-meter – SI unit of torque Torque Torque is a measure of the tendency of a force to rotate an object about some axis. A torque is meaningful only in relation to a particular axis, so we speak of the torque about the motor shaft, the torque about the axle, and so on. In order to produce torque, the force must act at some distance from the axis or pivot point. For example, a force applied at the end of a wrench handle to turn a nut around a screw located in the jaw at the other end of the wrench produces a torque about the screw. Similarly, a force applied at the circumference of a gear attached to an axle produces a torque about the axle. The perpendicular distance d from the line of force to the axis is called the moment arm. In the following diagram, the circle represents a gear of radius d. The dot in the center represents the axle (A). A force F is applied at the edge of the gear, tangentially. F d A Diagram 1 In this example, the radius of the gear is the moment arm. The force is acting along a tangent to the gear, so it is perpendicular to the radius. The amount of torque at A about the gear axle is defined as = F×d 1 We use the Greek letter Tau ( ) to represent torque.