Some consequences of a Universal Tension arising from Dark Energy for structures from Atomic Nuclei to Galaxy Clusters
|
|
- Shanon Harrell
- 6 years ago
- Views:
Transcription
1 unning Head: Universal Tension fro DE Article Type: Original esearch Soe consequences of a Universal Tension arising fro Dark Energy for structures fro Atoic Nuclei to Galaxy Clusters C Sivara Indian Institute of Astrophysics, Banore, 560 0, India Telephone: ; Fax: e-ail: sivara@iiap.res.in Kenath Arun Christ Junior College, Banore, , India Telephone: ; Fax: e-ail: kenath.arun@cjc.christcollege.edu Kiren O V Christ Junior College, Banore, , India Telephone: ; Fax: e-ail: kiren.ov@cjc.christcollege.edu Abstract: In recent work, a new cosological paradig iplied a ass-radius relation, suggesting a universal tension related to the background dark energy (cosological constant), leading to an energy per unit area that holds for structures fro atoic nuclei to clusters of axies. Here we explore soe of the consequences that arise fro such a universal tension.
2 . Introduction In recent papers (Sivara, 99a; 99b; 008; Sivara & Arun, 0a; 0) a new kind of cosological paradig was invoked wherein the requireent that for a hierarchy of large scale structures, like axies, axy clusters, super-clusters, etc. their gravitational (binding) self energy density ust at least equal or exceed the background repulsive dark energy density (a cosological constant as current observations strongly suggests) iplies a ass-radius relation of the type: c... () G G c c c (i.e. gives rise to a universal tension, T ) 8 8G G This is the background curvature x superstring tension (Sivara, 99a; 005). Or this can also be inferred as the local ass x local curvature. (Superstring tension is cosological dark energy) c ~, is the G This paradig focuses on the universe s fundaental structures and syetries and ephasises a new universal paraeter underlying systes fro the sallest (atoic nuclei) to the largest (clusters of axies), encopassing nearly 80 orders of agnitude in ass and nearly 0 orders of agnitude in size. (Oldershaw, 987; Sivara, 99; 00; 005). Nuclear Tension c The energy per unit area (surface tension) given by above equations, i.e. T c, has G the sae nuerical value as that in nuclear physics, (Sivara, 005; 008) like the surface tension in the nuclear liquid drop odel of nucleus and nuclear atter. ~ 0 ergs / c. This has consequences for the In the nucleus this nuclear surface tension balances the Coulob repulsion: Z e T... ()
3 Where 0 A, 0 ~.50 c For T ~ 0 ergs / c, this sets a liit of: Z A 0 which agrees with the usual Bohr-Wheeler criterion. (Bohr & Wheeler, 99) Considering also the rotation (spin) of the nucleus we have:... () Z e T... () 5 Where the ters on the left are repulsive in nature and that on the right is attractive. This gives the radius of the size of the nucleus as (where P A, P is the proton ass): Z e 5 T A P... (5) The angular frequency dependence on nuclear size is given in figure (): Figure : Dependence of Angular Frequency with Nuclear size
4 For the liiting case as T 5 : P A... (6) This sets a liit on the frequency as: 0T... (7) A P For A = we have: 0 s... (8) And the corresponding tie period of: ~ 0 s... (9) This corresponds to the nuclear tie scale. Figure () gives the variation of angular frequency with the nuber of nucleons. Figure : Variation of angular frequency with A
5 This liit on the frequency will also put a constraint on the rotational energy levels of nucleus: n... (0) 5 7 n 0A... () For A = 0, we have n 00 These states correspond to the yrast states, which are the lowest excited level at high angular oentu ~ 70 as suggested in the following reference (Grover, 967). Later observations indicate high angular oentu ~ 00. Figure () gives the alost linear dependence of the order (n) with the ass nuber. Figure : Variation of n with ass nuber. Gravitationally bound structure, Angular oentu and Dark Energy In the case of large, gravitationally bound structures such as axies, axy clusters, etc. the requireent is that gravitational self energy density should be coparable to the background cosic vacuu energy density for the object to be an autonoous structure. That is: G c... () 8 8G 5
6 This would also give the sae result as equation (), i.e.: Where is the cosological constant with an observed value of 0 G c 56 c. This equation holds for a whole range of large scale structures, including the Hubble volue. (Sivara, 008 and references there in) The relation is suggestive of a surface tension which has the sae universal value for all the large scale cosic structures fro globular clusters, large olecular clouds, all the way to the Hubble universe (Sivara, 99a; 008). A kind of universal surface tension, suggesting the holographic picture! (Sivara & Arun, 0) (It also holds for the electron!) The universality of this surface tension again constrains the size of a neutron star. For a neutron star coposed on N neutrons: G NS NST N... () NS For a solar ass neutron star, detected neutron star. (Crawford, et a 006) Considering also the rotation of the neutron stars we have: G NS T N NS NS NS NS 57 N 50, which atches the observations for the heaviest... () This sets a liit on the rotational frequency and the corresponding tie period of the neutron star as: 0 s, 0. 5s... (5) This is consistent with the observations of the illisecond pulsar having the fastest rotational period detected so far, which is ~.s. (Hessels, et a 006) In the case of axies, this surface tension balancing the rotational energy can possibly explain the flat rotation curve of the axies. That is, for axies, their rotation balances this surface tension. This gives: T... (6) 6
7 Where the rotation frequency and the corresponding tie periods are given as: T 0 s, 0 s... (7) Since is a constant even for a axy, the relation given by equation (6) leads to: constant... (8) Therefore, the velocity, which is given by: v T... (9) will also be a constant as expected fro the axy rotation curves! This suggests a velocity independent of radial distance (flat rotation curve) without invoking dark atter. It is interesting to note that this dependence of rotational frequency going as inverse of the size hold true even right down to the atoic nucleus, as indicated by figure. Figure : Variation of rotational frequency with size 7
8 In an earlier work (Sivara & Arun, 0b) a priordial cosic rotation was suggested which can give rise to the observed rotation angular oenta of axies, axy clusters, stellar planetary systes, etc., the origin of which is otherwise not clearly understood. The angular oentu of the axy given by have (again since is a constant): J, is conserved. Therefore we J v is a constant... (0) This also leads to constant and therefore a velocity independent of radial distance.. Dynaics of evolving structures The requireent that the gravitational self energy density ust at least equal or exceed the background repulsive dark energy density iplied a ass-radius relation as given by equation (), for a hierarchy of large scale structures, like axies, axy clusters, super-clusters, etc. This ass-radius relation holds good for nebulae too. Any perturbation to it will lead to its collapse and eventual foration of the star (and possibly planetary syste). For a typical star of ass, the order of star 0 g, the condition that iplies that the initial size of the nebula be of Neb 6 ~ 0 c. It is also of interest to note that the sae value for the tension (arising as we have seen, fro the cosic dark energy ( ter)) which we have used for axies, axy clusters, atoic nuclei, etc. also sees to be relevant for the diensions of planets and stars. For exaple, for a typical planetary ass of gravitational self energy, i.e. 8 ~ 0 g, balancing surface energy and G T... () we get the radius, which is given by: 8
9 G T... () For 8 ~ 0 g, we get 5000k (the earth radius). The above equation also gives a Jupiter radius of ~ 0 5 k for the corresponding ass. For a typical stellar ass of ~ 0 g, the above equation iplies ~ 0 c. So the range of stellar and planetary sizes is also given by the sae value of T! This suggests a deep underlying connection between the background dark energy (-ter, which gives the background curvature) and all the structures ebedded in this background. For the large structures we had balance of gravitational energy densities with the background dark energy density. For the planetary and stellar objects, the balance was with surface energies and gravitational self energies. 5. Densities of various structures As noted above, we had a universa ratio, i.e. a ubiquitous surface tension of c G 0 ergs / c know that nuclear density is, underlying all entities fro nuclei to axy superclusters! But we ~ 0 understand this diversity in densities? 5 g / cc, superclusters have a density of ~ 0 g / cc. How to It is just that the average density is ~, so that if we have the universal T, i.e. c G g / T ~ c! (As T, the densities of the various structures considered would scale as, so is just T ) As T is a universal constant the density siply scales as tension, this is the Laplace pressure for a droplet).. (In connection with surface 9
10 Thus for a nucleus ~ feri, we have ~ 0 0 g / cc. For a axy ~ 0 c, we have 5 5 ~ 0 g / cc. For a super-cluster ~ 0 c, ~ 0 g / cc. And for the Hubble volue, ~ 9 ~ ~ 0 g / cc, just what is observed! H So we have another universal result: constant Holding fro nuclei to the universe!... () Figure 5: Variation of density with size 6. Nuclear Vibrational and otational Energy levels In connection with the energy levels of the nucleus, including both vibrational and rotational levels, we can invoke the liquid drop odel of nuclei. In the drop odel there is equilibriu between surface tension and Coulob repulsion. Sall perturbations of the drop surface of radius by r gives changes in surface energy (surface given by Fr,, constant), which can be expanded in spherical haronics (like in fluid echanics of incopressible liquid spheres). 0
11 Thus: C l Y... (), l Y l L Yl, l,... (5) The surface energy is perturbed as: T * ES l l C C... (6) While the electrostatic (repulsive) Coulob energy is perturbed as: Z e l * EC C C... (7) l Finally we can write the Hailtonian including also the kinetic energy: 5 C l, C l *... (8) The lowest ode being l we have the energy levels of a five-diensional haronic oscillator as: E n 5 l... (9) This for l gives the ground state energy level as: E Z e T 0... (0) An For a nuclei of Z 0, A 0, the above equation gives a ground state energy of: E 0 5 ergs 0eV 0 The higher levels will be in ultiples of 0eV.... () For l 0, stability is given by: Z e T, A 0 The higher vibrational excited states are given by n,,..., etc.... ()
12 We can include the rotational energy levels (like in atoic spectroscopy). Thus rotational levels are n rot. The liiting values of rot for various A have been given above. Energy levels of rotation are: E rot ll I... () Where the oent of inertia of the nuclei is: The rotational energy is then given as: I 5 E rot 0. ev... () And the total energy is: E total E E... (5) vib rot For various n, etc. Siilar relations as those above hold also for (nuclei of) priordial axies, provided we replace the Coulob energy ter with the gravitational energy. This would also have a negative sign as it is binding energy. In other words the replaceent is perturbed as: Ze by G would give the result. That is, the surface energy T * ES l l C C... (6) And the gravitational energy is perturbed as: (Lab, 95) 6 G l * EG C C... (7) l The tension (T) ter would be the sae. Scaling relations are as before and equation (0) will not apply to axies! The frequency of oscillation due to the perturbation for the axies is given as: 8 T G... (8)
13 For a typical axy of 0 g, 0 g / cc, the frequency is 0 s. These oscillations will eit gravitational waves, where the quadrupole gravitational power is given by: (Sivara & Arun, 0) G 6 P GW... (9) 5 c And for a typical axy of 0 g, 0 c, this gives: P GW ~ 0 5 ergs / s... (0) GEGW The corresponding strain produce on a detector, which is given as h ~ 0 c r within the liits of proposed space based gravitational wave observatories like LISA. 0, which is 6. Conclusion In this paper, we have extended our earlier work (which gave rise to a ass-radius relation) with a universal value of a surface tension ~ 0 ergs / c arising fro the requireent that the binding energy density of gravitationally bound objects be at least equal or exceed the background repulsive dark energy density. This universal tension arising fro dark energy doinating three-fourths of the universe, leads to various consequences for a hierarchy of objects, fro atoic nuclei to axy clusters. This can for instance set a liit on the rotational energy levels of a nucleus; set the diensions of planets and stars; to even explain the flat rotation curve of axies without invoking dark atter and liit the size of axy clusters. In short, we have a new paradig encopassing features of structures ranging over eighty orders in ass and forty orders in length scale. eference: Bohr, N & Wheeler, J. H. 99, Phys. ev., 56, 6 Crawford, F. et a 006, Astrophysical J., 65, 99 Grover, J.. 967, Phys. ev., 57, 8 Hessels, J. et a 006, Science,, 90
14 Lab, H., 95, Hydrodynaics (6 th Edition), Dover: New York Oldershaw,. L. 987, Astrophys. J.,, Sivara, C. 99, Astrophys. Spc. Sci., 07, 7 Sivara, C. 99a, Astrophys. Space Sci., 5, 85 Sivara, C. 99b, Astrophys. Space Sci., 9, 5 Sivara, C. 00, Astrophys. Space Sci., 7, Sivara, C., 005, in st century astrophysics, eds S. K. Saha & V. K. astogi, Anita Publications, New Delhi, p.6 Sivara, C. 008, preprint, arxiv:080.8v Sivara, C & Arun, K. 0, The Open Astron. J., (Suppl -), 7 Sivara, C & Arun, K. 0a, preprint, arxiv:05.6v Sivara, C & Arun, K. 0b, The Open Astron. J., 5, 7 Sivara, C & Arun, K. 0, Astrophys. Space Sci., DOI 0.007/s
Open Access Some Consequences of a Universal Tension Arising from Dark Energy for Structures from Atomic Nuclei to Galaxy Clusters
Send Orders for Reprints to reprints@benthamscience.net 90 The Open Astronomy Journal, 0, 6, 90-97 Open Access Some Consequences of a Universal Tension Arising from Dark Energy for Structures from Atomic
More informationNuclear Physics (10 th lecture)
~Theta Nuclear Physics ( th lecture) Content Nuclear Collective Model: Rainwater approx. (reinder) Consequences of nuclear deforation o Rotational states High spin states and back bending o Vibrational
More informationNewton's Laws. Lecture 2 Key Concepts. Newtonian mechanics and relation to Kepler's laws The Virial Theorem Tidal forces Collision physics
Lecture 2 Key Concepts Newtonian echanics and relation to Kepler's laws The Virial Theore Tidal forces Collision physics Newton's Laws 1) An object at rest will reain at rest and an object in otion will
More informationField Mass Generation and Control. Chapter 6. The famous two slit experiment proved that a particle can exist as a wave and yet
111 Field Mass Generation and Control Chapter 6 The faous two slit experient proved that a particle can exist as a wave and yet still exhibit particle characteristics when the wavefunction is altered by
More informationU V. r In Uniform Field the Potential Difference is V Ed
SPHI/W nit 7.8 Electric Potential Page of 5 Notes Physics Tool box Electric Potential Energy the electric potential energy stored in a syste k of two charges and is E r k Coulobs Constant is N C 9 9. E
More information2 Q 10. Likewise, in case of multiple particles, the corresponding density in 2 must be averaged over all
Lecture 6 Introduction to kinetic theory of plasa waves Introduction to kinetic theory So far we have been odeling plasa dynaics using fluid equations. The assuption has been that the pressure can be either
More informationLecture #8-3 Oscillations, Simple Harmonic Motion
Lecture #8-3 Oscillations Siple Haronic Motion So far we have considered two basic types of otion: translation and rotation. But these are not the only two types of otion we can observe in every day life.
More informationDispersion. February 12, 2014
Dispersion February 1, 014 In aterials, the dielectric constant and pereability are actually frequency dependent. This does not affect our results for single frequency odes, but when we have a superposition
More informationDimensions and Units
Civil Engineering Hydraulics Mechanics of Fluids and Modeling Diensions and Units You already know how iportant using the correct diensions can be in the analysis of a proble in fluid echanics If you don
More informationTheoretical Astrophysics and Cosmology Master Degree in Astronomy and Erasmus-Mundus A.A. 2016/17 Alberto Franceschini Cosmology Course
Theoretical Astrophysics and Cosology Master Degree in Astronoy and Erasus-Mundus A.A. 16/17 Alberto Franceschini Cosology Course Hoogeneous Friedan Universe.1 PROGRAMME FOR THE COSMOLOGY COURSE. The Hoogeneous
More informationScattering and bound states
Chapter Scattering and bound states In this chapter we give a review of quantu-echanical scattering theory. We focus on the relation between the scattering aplitude of a potential and its bound states
More informationPotential Energy 4/7/11. Lecture 22: Chapter 11 Gravity Lecture 2. Gravitational potential energy. Total energy. Apollo 14, at lift-off
Lecture 22: Chapter 11 Gravity Lecture 2 2 Potential Energy r Gravitational potential energy Escape velocity of a point ass for ass distributions Discrete Rod Spherical shell Sphere Gravitational potential
More informationPractice Final Exam PY 205 Monday 2004 May 3
Practice Final Exa PY 05 Monday 004 May 3 Nae There are THREE forula pages. Read all probles carefully before attepting to solve the. Your work ust be legible, and the organization ust be clear. Correct
More informationQ5 We know that a mass at the end of a spring when displaced will perform simple m harmonic oscillations with a period given by T = 2!
Chapter 4.1 Q1 n oscillation is any otion in which the displaceent of a particle fro a fixed point keeps changing direction and there is a periodicity in the otion i.e. the otion repeats in soe way. In
More informationNUMERICAL MODELLING OF THE TYRE/ROAD CONTACT
NUMERICAL MODELLING OF THE TYRE/ROAD CONTACT PACS REFERENCE: 43.5.LJ Krister Larsson Departent of Applied Acoustics Chalers University of Technology SE-412 96 Sweden Tel: +46 ()31 772 22 Fax: +46 ()31
More informationThe anisotropy of the cosmic background radiation due to mass clustering in a closed universe
Astron. Astrophys. 9, 79 7 (997) ASTRONOMY AND ASTROPHYSICS The anisotropy of the cosic background radiation due to ass clustering in a closed universe Daing Chen, Guoxuan Song, and Yougen Shen, Shanghai
More informationEigenvalues of the Angular Momentum Operators
Eigenvalues of the Angular Moentu Operators Toda, we are talking about the eigenvalues of the angular oentu operators. J is used to denote angular oentu in general, L is used specificall to denote orbital
More informationwhich is the moment of inertia mm -- the center of mass is given by: m11 r m2r 2
Chapter 6: The Rigid Rotator * Energy Levels of the Rigid Rotator - this is the odel for icrowave/rotational spectroscopy - a rotating diatoic is odeled as a rigid rotator -- we have two atos with asses
More information13 Harmonic oscillator revisited: Dirac s approach and introduction to Second Quantization
3 Haronic oscillator revisited: Dirac s approach and introduction to Second Quantization. Dirac cae up with a ore elegant way to solve the haronic oscillator proble. We will now study this approach. The
More information1 (40) Gravitational Systems Two heavy spherical (radius 0.05R) objects are located at fixed positions along
(40) Gravitational Systes Two heavy spherical (radius 0.05) objects are located at fixed positions along 2M 2M 0 an axis in space. The first ass is centered at r = 0 and has a ass of 2M. The second ass
More informationMoment of Inertia. Terminology. Definitions Moment of inertia of a body with mass, m, about the x axis: Transfer Theorem - 1. ( )dm. = y 2 + z 2.
Terinology Moent of Inertia ME 202 Moent of inertia (MOI) = second ass oent Instead of ultiplying ass by distance to the first power (which gives the first ass oent), we ultiply it by distance to the second
More informationTHE ROCKET EXPERIMENT 1. «Homogenous» gravitational field
THE OCKET EXPEIENT. «Hoogenous» gravitational field Let s assue, fig., that we have a body of ass Μ and radius. fig. As it is known, the gravitational field of ass Μ (both in ters of geoetry and dynaics)
More informationGeneralized r-modes of the Maclaurin spheroids
PHYSICAL REVIEW D, VOLUME 59, 044009 Generalized r-odes of the Maclaurin spheroids Lee Lindblo Theoretical Astrophysics 130-33, California Institute of Technology, Pasadena, California 9115 Jaes R. Ipser
More information8.1 Force Laws Hooke s Law
8.1 Force Laws There are forces that don't change appreciably fro one instant to another, which we refer to as constant in tie, and forces that don't change appreciably fro one point to another, which
More informationQuestion number 1 to 8 carries 2 marks each, 9 to 16 carries 4 marks each and 17 to 18 carries 6 marks each.
IIT-JEE5-PH-1 FIITJEE Solutions to IITJEE 5 Mains Paper Tie: hours Physics Note: Question nuber 1 to 8 carries arks each, 9 to 16 carries 4 arks each and 17 to 18 carries 6 arks each. Q1. whistling train
More informationThe Charged Liquid Drop Model Binding Energy and Fission
The Charged Liquid Drop Model Binding Energy and Fission 103 This is a simple model for the binding energy of a nucleus This model is also important to understand fission and how energy is obtained from
More informationCrystallization of Supercooled Liquid Elements Induced by Superclusters Containing Magic Atom Numbers Abstract: Keywords: 1.
Crystallization of Supercooled Liquid Eleents Induced by Superclusters Containing Magic Ato Nubers Robert F. Tournier, CRETA /CNRS, Université Joseph Fourier, B.P. 166, 804 Grenoble cedex 09, France. E-ail:
More informationPhysics 314 (Survey of Astronomy) Exam 1
Physics 314 (Survey of Astronomy) Exam 1 Please show all significant steps clearly in all problems. Please give clear and legible responses to qualitative questions. See the last page for values of constants.
More informationFeshbach Resonances in Ultracold Gases
Feshbach Resonances in Ultracold Gases Sara L. Capbell MIT Departent of Physics Dated: May 5, 9) First described by Heran Feshbach in a 958 paper, Feshbach resonances describe resonant scattering between
More informationMASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department Earth, Atmospheric, and Planetary Sciences Department. Quiz 2
MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Departent Earth, Atospheric, and Planetary Sciences Departent Astronoy 8.8J 1.40J April 19, 006 Quiz Nae Solutions (please print) Last First 1. Work any 7
More information(a) Why cannot the Carnot cycle be applied in the real world? Because it would have to run infinitely slowly, which is not useful.
PHSX 446 FINAL EXAM Spring 25 First, soe basic knowledge questions You need not show work here; just give the answer More than one answer ight apply Don t waste tie transcribing answers; just write on
More informationA NEW ELECTROSTATIC FIELD GEOMETRY. Jerry E. Bayles
INTRODUCTION A NEW ELECTROSTATIC FIELD GEOMETRY by Jerry E Bayles The purpose of this paper is to present the electrostatic field in geoetrical ters siilar to that of the electrogravitational equation
More informationProblem T1. Main sequence stars (11 points)
Proble T1. Main sequence stars 11 points Part. Lifetie of Sun points i..7 pts Since the Sun behaves as a perfectly black body it s total radiation power can be expressed fro the Stefan- Boltzann law as
More informationAstro 7B Midterm 1 Practice Worksheet
Astro 7B Midter 1 Practice Worksheet For all the questions below, ake sure you can derive all the relevant questions that s not on the forula sheet by heart (i.e. without referring to your lecture notes).
More informationarxiv: v2 [hep-ph] 9 Jan 2014
Fluctuation induced equality of ulti-particle eccentricities for four or ore particles Ada Bzdak a, Piotr Bozek b,c, Larry McLerran d,a,e arxiv:1311.7325v2 [hep-ph] 9 Jan 2014 a RIKEN BNL Research Center,
More informationA simple model for Jeans instability in the presence of a constant magnetic field arxiv:astro-ph/ v1 12 Feb 2004
A siple odel for Jeans instability in the presence of a constant agnetic field arxiv:astro-ph/0402321v1 12 Feb 2004 A. Sandoval-Villalbazo a, L.S. García-Colín b, c and A. Arrieta-Ostos a a Departaento
More informationThe accelerated expansion of the universe is explained by quantum field theory.
The accelerated expansion of the universe is explained by quantu field theory. Abstract. Forulas describing interactions, in fact, use the liiting speed of inforation transfer, and not the speed of light.
More informationIn the session you will be divided into groups and perform four separate experiments:
Mechanics Lab (Civil Engineers) Nae (please print): Tutor (please print): Lab group: Date of lab: Experients In the session you will be divided into groups and perfor four separate experients: (1) air-track
More informationHee = ~ dxdy\jj+ (x) 'IJ+ (y) u (x- y) \jj (y) \jj (x), V, = ~ dx 'IJ+ (x) \jj (x) V (x), Hii = Z 2 ~ dx dy cp+ (x) cp+ (y) u (x- y) cp (y) cp (x),
SOVIET PHYSICS JETP VOLUME 14, NUMBER 4 APRIL, 1962 SHIFT OF ATOMIC ENERGY LEVELS IN A PLASMA L. E. PARGAMANIK Khar'kov State University Subitted to JETP editor February 16, 1961; resubitted June 19, 1961
More informationPrimordial Black Holes as Heat Sources for Living Systems with Longest Possible Lifetimes
Primordial Black Holes as Heat Sources for Living Systems with Longest Possible Lifetimes C Sivaram Indian Institute of Astrophysics, Bangalore, 560 0, India elephone: +91-80-55 067; Fax: +91-80-55 0 e-mail:
More informationQuantum Ground States as Equilibrium Particle Vacuum Interaction States
Quantu Ground States as Euilibriu article Vacuu Interaction States Harold E uthoff Abstract A rearkable feature of atoic ground states is that they are observed to be radiationless in nature despite (fro
More informationThe calculation method of interaction between metal atoms under influence of the radiation
IOP Conference Series: Materials Science and Engineering PAPER OPEN ACCESS The calculation ethod of interaction between etal atos under influence of the radiation To cite this article: S N Yanin 015 IOP
More informationA new Lagrangian of the simple harmonic oscillator 1 revisited
A new Lagrangian of the siple haronic oscillator 1 revisited Faisal Ain Yassein Abdelohssin Sudan Institute for Natural Sciences, P.O.BOX 3045, Khartou, Sudan Abstract A better and syetric new Lagrangian
More information7. Renormalization and universality in pionless EFT
Renoralization and universality in pionless EFT (last revised: October 6, 04) 7 7. Renoralization and universality in pionless EFT Recall the scales of nuclear forces fro Section 5: Pionless EFT is applicable
More informationThe Hydrogen Atom. Nucleus charge +Ze mass m 1 coordinates x 1, y 1, z 1. Electron charge e mass m 2 coordinates x 2, y 2, z 2
The Hydrogen Ato The only ato that can be solved exactly. The results becoe the basis for understanding all other atos and olecules. Orbital Angular Moentu Spherical Haronics Nucleus charge +Ze ass coordinates
More informationma x = -bv x + F rod.
Notes on Dynaical Systes Dynaics is the study of change. The priary ingredients of a dynaical syste are its state and its rule of change (also soeties called the dynaic). Dynaical systes can be continuous
More informationPY /005 Practice Test 1, 2004 Feb. 10
PY 205-004/005 Practice Test 1, 2004 Feb. 10 Print nae Lab section I have neither given nor received unauthorized aid on this test. Sign ature: When you turn in the test (including forula page) you ust
More informationReview: Relativistic mechanics. Announcements. Relativistic kinetic energy. Kinetic energy. E tot = γmc 2 = K + mc 2. K = γmc 2 - mc 2 = (γ-1)mc 2
Announceents Reading for Monday: Chapters 3.7-3.12 Review session for the idter: in class on Wed. HW 4 due Wed. Exa 1 in 6 days. It covers Chapters 1 & 2. Roo: G1B30 (next to this classroo). Review: Relativistic
More informationSpinning Disk and Chladni Plates
Spinning Disk and Chladni Plates Subitted By MD MARUFUR RAHMAN Msc Sustainable Energy Systes Beng(Hons) Mechanical Engineering Bsc Coputer Science and Engineering Table of Contents Spinning Disk... 3 1.0
More informationP235 Midterm Examination Prof. Cline
P235 Mier Exaination Prof. Cline THIS IS A CLOSED BOOK EXAMINATION. Do all parts of all four questions. Show all steps to get full credit. 7:00-10.00p, 30 October 2009 1:(20pts) Consider a rocket fired
More informationPhysics 221B: Solution to HW # 6. 1) Born-Oppenheimer for Coupled Harmonic Oscillators
Physics B: Solution to HW # 6 ) Born-Oppenheier for Coupled Haronic Oscillators This proble is eant to convince you of the validity of the Born-Oppenheier BO) Approxiation through a toy odel of coupled
More informationPhys463.nb. Many electrons in 1D at T = 0. For a large system (L ), ΕF =? (6.7) The solutions of this equation are plane waves (6.
â â x Ψn Hx Ε Ψn Hx 35 (6.7) he solutions of this equation are plane waves Ψn Hx A exphä n x (6.8) he eigen-energy Εn is n (6.9) Εn For a D syste with length and periodic boundary conditions, Ψn Hx Ψn
More informationThe Characteristic Planet
The Characteristic Planet Brano Zivla, bzivla@gail.co Abstract: I have calculated a relation significant for planets fro a logical starting point that a whole and its parts are ianently depandant on each
More informationPhysics 139B Solutions to Homework Set 3 Fall 2009
Physics 139B Solutions to Hoework Set 3 Fall 009 1. Consider a particle of ass attached to a rigid assless rod of fixed length R whose other end is fixed at the origin. The rod is free to rotate about
More informationSmall Neutrino Masses: Another Anthropic principle aspect? C Sivaram. Indian Institute of Astrophysics, Bangalore , India
Small Neutrino Masses: Another Anthropic principle aspect? C Sivaram Indian Institute of Astrophysics, Bangalore - 560 034, India Telephone: +91-80-553 067; Fax: +91-80-553 4043 e-mail: sivaram@iiap.res.in
More informationChapter 1: Basics of Vibrations for Simple Mechanical Systems
Chapter 1: Basics of Vibrations for Siple Mechanical Systes Introduction: The fundaentals of Sound and Vibrations are part of the broader field of echanics, with strong connections to classical echanics,
More informationPhysics 120 Final Examination
Physics 120 Final Exaination 12 August, 1998 Nae Tie: 3 hours Signature Calculator and one forula sheet allowed Student nuber Show coplete solutions to questions 3 to 8. This exaination has 8 questions.
More informationSimple Harmonic Motion
Siple Haronic Motion Physics Enhanceent Prograe for Gifted Students The Hong Kong Acadey for Gifted Education and Departent of Physics, HKBU Departent of Physics Siple haronic otion In echanical physics,
More informationA toy model of quantum electrodynamics in (1 + 1) dimensions
IOP PUBLISHING Eur. J. Phys. 29 (2008) 815 830 EUROPEAN JOURNAL OF PHYSICS doi:10.1088/0143-0807/29/4/014 A toy odel of quantu electrodynaics in (1 + 1) diensions ADBoozer Departent of Physics, California
More informationPHYS 102 Previous Exam Problems
PHYS 102 Previous Exa Probles CHAPTER 16 Waves Transverse waves on a string Power Interference of waves Standing waves Resonance on a string 1. The displaceent of a string carrying a traveling sinusoidal
More informationDepartment of Physics Preliminary Exam January 3 6, 2006
Departent of Physics Preliinary Exa January 3 6, 2006 Day 1: Classical Mechanics Tuesday, January 3, 2006 9:00 a.. 12:00 p.. Instructions: 1. Write the answer to each question on a separate sheet of paper.
More informationKinetic Theory of Gases: Elementary Ideas
Kinetic Theory of Gases: Eleentary Ideas 17th February 2010 1 Kinetic Theory: A Discussion Based on a Siplified iew of the Motion of Gases 1.1 Pressure: Consul Engel and Reid Ch. 33.1) for a discussion
More informationGeneral Physics General Physics General Physics General Physics. Language of Physics
1 Physics is a science rooted equally firly in theory and experients Physicists observe Nature series of experients easure physical quantities discover how the things easured are connected discover a physical
More informationClassical systems in equilibrium
35 Classical systes in equilibriu Ideal gas Distinguishable particles Here we assue that every particle can be labeled by an index i... and distinguished fro any other particle by its label if not by any
More informationFour-vector, Dirac spinor representation and Lorentz Transformations
Available online at www.pelagiaresearchlibrary.co Advances in Applied Science Research, 2012, 3 (2):749-756 Four-vector, Dirac spinor representation and Lorentz Transforations S. B. Khasare 1, J. N. Rateke
More informationDr G. I. Ogilvie Lent Term 2005 INTRODUCTION
Accretion Discs Mathematical Tripos, Part III Dr G. I. Ogilvie Lent Term 2005 INTRODUCTION 0.1. Accretion If a particle of mass m falls from infinity and comes to rest on the surface of a star of mass
More informationAccuracy of the Scaling Law for Experimental Natural Frequencies of Rectangular Thin Plates
The 9th Conference of Mechanical Engineering Network of Thailand 9- October 005, Phuket, Thailand Accuracy of the caling Law for Experiental Natural Frequencies of Rectangular Thin Plates Anawat Na songkhla
More informationNB1140: Physics 1A - Classical mechanics and Thermodynamics Problem set 2 - Forces and energy Week 2: November 2016
NB1140: Physics 1A - Classical echanics and Therodynaics Proble set 2 - Forces and energy Week 2: 21-25 Noveber 2016 Proble 1. Why force is transitted uniforly through a assless string, a assless spring,
More informationOptical Properties of Plasmas of High-Z Elements
Forschungszentru Karlsruhe Techni und Uwelt Wissenschaftlishe Berichte FZK Optical Properties of Plasas of High-Z Eleents V.Tolach 1, G.Miloshevsy 1, H.Würz Project Kernfusion 1 Heat and Mass Transfer
More informationAn Overview of the Mechanics of Oscillating Mechanisms
Aerican Journal of echanical Engineering, 3, Vol., No. 3, 58-65 Available online at http://pubs.sciepub.co/aje//3/ Science Education Publishing DOI:.69/aje--3- An Overview of the echanics of Oscillating
More informationSupporting Information
Supporting Inforation Nash et al. 10.1073/pnas.1507413112 Equation of Motion If a gyroscope is spinning with a large constant angular frequency, ω, around its principal axis, ^l, then its dynaics are deterined
More informationKinetic Theory of Gases: Elementary Ideas
Kinetic Theory of Gases: Eleentary Ideas 9th February 011 1 Kinetic Theory: A Discussion Based on a Siplified iew of the Motion of Gases 1.1 Pressure: Consul Engel and Reid Ch. 33.1) for a discussion of
More informationA Different Derivation of the Calogero Conjecture
1 Abstract: A Different Derivation of the Calogero Conjecture Ioannis Iraklis Haranas Physics and Astronoy Departent York University 314 A Petrie Science Building Toronto Ontario CANADA E ail: ioannis@yorku.ca
More informationLecture contents. Magnetic properties Diamagnetism Band paramagnetism Atomic paramagnetism. NNSE508 / NENG452 Lecture #14
1 Lecture contents agnetic properties Diaagnetis and paraagnetis Atoic paraagnetis NNSE58 / NENG45 Lecture #14 agnetic units H /r V s 1 Wb T 1 T Wb T 1H A A Fro Treolet de Lacheisserie, 5 NNSE58 / NENG45
More informationAstronomy Stars, Galaxies and Cosmology Exam 3. Please PRINT full name
Astronomy 132 - Stars, Galaxies and Cosmology Exam 3 Please PRINT full name Also, please sign the honor code: I have neither given nor have I received help on this exam The following exam is intended to
More informationLecture 12: Waves in periodic structures
Lecture : Waves in periodic structures Phonons: quantised lattice vibrations of a crystalline solid is: To approach the general topic of waves in periodic structures fro a specific standpoint: Lattice
More informationName: Partner(s): Date: Angular Momentum
Nae: Partner(s): Date: Angular Moentu 1. Purpose: In this lab, you will use the principle of conservation of angular oentu to easure the oent of inertia of various objects. Additionally, you develop a
More informationJournal of Modern Physics, 2011, 2, doi: /jmp Published Online November 2011 (http://www.scirp.
Journal of Modern Physics, 11,, 1331-1347 doi:1.436/jp.11.11165 Published Online Noveber 11 (http://www.scirp.org/journal/jp) Transforation of the Angular Power Spectru of the Cosic Microwave Background
More information1 Statistics of volumes, swept by spheroidal particles, in a turbulent flow.
1 Statistics of volues, swept by spheroidal particles, in a turbulent flow. B. Grits*, M. Pinsky, and A. Khain Institute of Earth Science, The Hebrew University of Jerusale 1. INTRODUCTION Collisions between
More informationPh 20.3 Numerical Solution of Ordinary Differential Equations
Ph 20.3 Nuerical Solution of Ordinary Differential Equations Due: Week 5 -v20170314- This Assignent So far, your assignents have tried to failiarize you with the hardware and software in the Physics Coputing
More informationwhich proves the motion is simple harmonic. Now A = a 2 + b 2 = =
Worked out Exaples. The potential energy function for the force between two atos in a diatoic olecules can be expressed as follows: a U(x) = b x / x6 where a and b are positive constants and x is the distance
More informationi ij j ( ) sin cos x y z x x x interchangeably.)
Tensor Operators Michael Fowler,2/3/12 Introduction: Cartesian Vectors and Tensors Physics is full of vectors: x, L, S and so on Classically, a (three-diensional) vector is defined by its properties under
More informationPART 4. Theoretical Competition
PART 4 Theoretical Copetition Exa coission page 98 Probles in English page 99 Solutions in English page 106 Probles in three other languages and back-translations of these page 117 Exaples of student papers
More informationEnergy and Momentum: The Ballistic Pendulum
Physics Departent Handout -10 Energy and Moentu: The Ballistic Pendulu The ballistic pendulu, first described in the id-eighteenth century, applies principles of echanics to the proble of easuring the
More informationPH 221-1D Spring Oscillations. Lectures Chapter 15 (Halliday/Resnick/Walker, Fundamentals of Physics 9 th edition)
PH 1-1D Spring 013 Oscillations Lectures 35-37 Chapter 15 (Halliday/Resnick/Walker, Fundaentals of Physics 9 th edition) 1 Chapter 15 Oscillations In this chapter we will cover the following topics: Displaceent,
More informationPhysics 525, Condensed Matter Homework 5 Due Tuesday, 7 th November 2006
Physics 55, Condensed Matter Hoework 5 Due Tuesday, 7 th Noveber 6 Jacob Lewis Bourjaily Proble : Phonon Spectru of a Diatoic One-Diensional Crystal Consider a one-diensional, diatoic crystal coposed of
More informationDefinition of Work, The basics
Physics 07 Lecture 16 Lecture 16 Chapter 11 (Work) v Eploy conservative and non-conservative forces v Relate force to potential energy v Use the concept of power (i.e., energy per tie) Chapter 1 v Define
More informationm A 1 m mgd k m v ( C) AP Physics Multiple Choice Practice Oscillations
P Physics Multiple Choice Practice Oscillations. ass, attached to a horizontal assless spring with spring constant, is set into siple haronic otion. Its axiu displaceent fro its equilibriu position is.
More informationOscillations: Review (Chapter 12)
Oscillations: Review (Chapter 1) Oscillations: otions that are periodic in tie (i.e. repetitive) o Swinging object (pendulu) o Vibrating object (spring, guitar string, etc.) o Part of ediu (i.e. string,
More informationRationality Problems of the Principles of Equivalence and General Relativity
Rationality Probles of the Principles of Equivalence and General Relativity Mei Xiaochun (Departent of Physics, Fuzhou University, E-ail: xc1@163.co Tel:86-591-8761414) (N.7-B, South Building, Zhongfu
More information16.512, Rocket Propulsion Prof. Manuel Martinez-Sanchez Lecture 30: Dynamics of Turbopump Systems: The Shuttle Engine
6.5, Rocket Propulsion Prof. Manuel Martinez-Sanchez Lecture 30: Dynaics of Turbopup Systes: The Shuttle Engine Dynaics of the Space Shuttle Main Engine Oxidizer Pressurization Subsystes Selected Sub-Model
More informationMotion Analysis of Euler s Disk
Motion Analysis of Euler s Disk Katsuhiko Yaada Osaka University) Euler s Disk is a nae of a scientific toy and its otion is the sae as a spinning coin. In this study, a siple atheatical odel is proposed
More informationLecture 4: Nuclear Energy Generation
Lecture 4: Nuclear Energy Generation Literature: Prialnik chapter 4.1 & 4.2!" 1 a) Some properties of atomic nuclei Let: Z = atomic number = # of protons in nucleus A = atomic mass number = # of nucleons
More information2009 Academic Challenge
009 Acadeic Challenge PHYSICS TEST - REGIONAL This Test Consists of 5 Questions Physics Test Production Tea Len Stor, Eastern Illinois University Author/Tea Leader Doug Brandt, Eastern Illinois University
More informationLecture 8 Symmetries, conserved quantities, and the labeling of states Angular Momentum
Lecture 8 Syetries, conserved quantities, and the labeling of states Angular Moentu Today s Progra: 1. Syetries and conserved quantities labeling of states. hrenfest Theore the greatest theore of all ties
More informationThe Night Sky. The Universe. The Celestial Sphere. Stars. Chapter 14
The Night Sky The Universe Chapter 14 Homework: All the multiple choice questions in Applying the Concepts and Group A questions in Parallel Exercises. Celestial observation dates to ancient civilizations
More informationSOLUTIONS. PROBLEM 1. The Hamiltonian of the particle in the gravitational field can be written as, x 0, + U(x), U(x) =
SOLUTIONS PROBLEM 1. The Hailtonian of the particle in the gravitational field can be written as { Ĥ = ˆp2, x 0, + U(x), U(x) = (1) 2 gx, x > 0. The siplest estiate coes fro the uncertainty relation. If
More informationACCUMULATION OF FLUID FLOW ENERGY BY VIBRATIONS EXCITATION IN SYSTEM WITH TWO DEGREE OF FREEDOM
ENGINEERING FOR RURAL DEVELOPMENT Jelgava, 9.-.5.8. ACCUMULATION OF FLUID FLOW ENERGY BY VIBRATION EXCITATION IN YTEM WITH TWO DEGREE OF FREEDOM Maris Eiduks, Janis Viba, Lauris tals Riga Technical University,
More informationAll you need to know about QM for this course
Introduction to Eleentary Particle Physics. Note 04 Page 1 of 9 All you need to know about QM for this course Ψ(q) State of particles is described by a coplex contiguous wave function Ψ(q) of soe coordinates
More information1 Introduction. 2 The hadronic many body problem
Models Lecture 18 1 Introduction In the next series of lectures we discuss various models, in particluar models that are used to describe strong interaction problems. We introduce this by discussing the
More information