1 GRS Measurement By A. Cacciani Frascati, March 21th 2006.

Slides:



Advertisements
Similar presentations
TWO STEP EQUATIONS 1. SOLVE FOR X 2. DO THE ADDITION STEP FIRST
Advertisements

LABBEVERATORIO DI SALINARDO Prospetto in scala 1:10.
Cirrone G. A. P. , Cuttone G. , Raffaele L. , Sabini M. G
Slide 1 Insert your own content. Slide 2 Insert your own content.
Satellite meeting - Designating habitable planets for follow-up study: what are the relative parameter spaces of RV and astrometry? (P2 Panel) Scientific.
The H-alpha radial velocities of an arch filament system in solar emerging flux region Shino Kawahara Rakutou High School KYOTO.
FIGURE 6.1 The electromagnetic radiation spectrum covers everything from very low frequency (VLF) radio to X-rays and beyond. Curtis Johnson Process.
2. The WAM Model: Solves energy balance equation, including Snonlin
0 - 0.
Light and the Electromagnetic Spectrum
Radio Astronomy By looking at the radio part of the EM spectrum, we can get a different perspective on the nature of the universe. the atmospheric window.
Stefan Hild for the GEO600 team October 2007 LSC-Virgo meeting Hannover Homodyne readout of an interferometer with Signal Recycling.
G.Barbiellini -- 1 AGILE 1yr G. Barbiellini on behalf of the AGILE team.
FROM MICRO TO MACROCOSMOS
NEWS: Nuclear Emulsion Wimp Search
5.9 + = 10 a)3.6 b)4.1 c)5.3 Question 1: Good Answer!! Well Done!! = 10 Question 1:
Fiber Optic Gyroscopes Instrumentation: Sensors and Signals.
10. ConcepTest 5.8a Earth and Moon I
Analyze the information brought by the polarization diversity (HH-VV-HV for ASAR, full-polarimetric for airborne radar) for wind and wave studies Validate.
Chapter 9. PN-junction diodes: Applications
March , Birmingham GR tests and micro-arcsecond light bending parameters by global and differential Gaia mesurements Maria Teresa Crosta Astronomical.
During the past few decades, scientists have discovered smaller sub- atomic particles that create the electrons, protons, and neutrons of an atom. As they.
1 LOA-ENSTA. 2 3 For PW class laser, a contrast better than is required I ASE has to be < W/cm² The ASE intensity is enough to generate.
Factoring ax2+bx +c ax2+bx +c
P 7 20 Questions Traffic Light Quiz. Rules Everyone should reveal their answer at the same time Count down: 3, 2, 1, show!
What is Slope Assignment. List the four types of slope and sketch each type. 1.
UNIT 2 Two Dimensional Motion
Sezione di Napoli Univ. “Federico II” Experimental study of beam hardening artefacts in photon counting breast computed tomography M.G. Bisogni a, A. Del.
Week 1.
Fisica Generale - Alan Giambattista, Betty McCarty Richardson Copyright © 2008 – The McGraw-Hill Companies s.r.l. 1 Chapter 26: Relativity The Postulates.
PH 508: Spacecraft systems
MAROON-X: An instrument for identifying another Earth
Chem. 133 – 2/19 Lecture. Announcements Lab Work –Turn in Electronics Lab –Starting Set 2 HW1.2 Due Today Quiz 2 Today Today’s Lecture –Noise –Electrochemistry.
Evolving X-ray Polarimetry towards high energy and solar science Sergio Fabiani Università degli Studi di Roma “Tor Vergata” INAF / IAPS I A P S Istituto.
Stellar Deaths II Neutron Stars and Black Holes 17.
8 Black Holes and General Relativity Stuff that warps your mind.
Sergey Kucheryavski Raman spectroscopy Acquisition, preprocessing and analysis of spectra.
Escape Velocity Must travel about 8 km/s or 18,000 mi/hr Trouble is that at this speed the atmosphere heats up objects and burns them up Image from.
14 Black Holes and General Relativity Stuff that warps your mind.
The MOF at South Pole Italian-American Research Collaboration Amundsen-Scott Station December 2002 – January 2003.
How The GPS System Works. How the GPS System Works 24 satellites + spares 6 orbital planes 55° inclination Each satellite orbits twice every 24 hours.
FREE ENERGY & Antigravity By William S. Alek INTALEK, INC. June 25, 2005.
Nuclear Physics E = mc 2. Outline Theory of Special Relativity Postulates E = mc 2 The Atom What makes up the atom? What holds the atom together? Quantum.
Live Cell Fluorescence Imaging Presented by: Nicholas Beavers – Media Cybernetics, Inc. Welcome to Sponsored by Starting Soon…
Pioneer Anomaly Test – Jonathan Fitt 1 Design Assessment of Lunar, Planetary and Satellite Ranging Applied to Fundamental Physics Jonathan Fitt Friday,
B. Gentry/GSFCGTWS 2/26/01 Doppler Wind Lidar Measurement Principles Bruce Gentry NASA / Goddard Space Flight Center based on a presentation made to the.
Relatively Einstein 2005 has been chosen as the World Year of Physics to celebrate the 100th anniversary of Einstein’s Miraculous Year. In this presentation,
Development of CCDs for the SXI We have developed 2 different types of CCDs for the SXI in parallel.. *Advantage =>They are successfully employed for current.
09/10/2005NSTAR Graal collaboration1 The Graal collaboration results and prospects Presented by Carlo Schaerf Università di Roma “Tor Vergata” and.
Status of AIRFLY fluorescence yield measurements Paolo Privitera Università di Roma Tor Vergata, INFN Prague, May 19, 2006.
T’ = Dilated Time t = Stationary time V = velocity C = Speed of light.
LAW OF UNIVERSAL GRAVITATION F G gravitational force (in two directions) G universal gravitation constant 6.67x Nm 2 kg -2 r distance between the.
09/10/2005NSTAR Graal collaboration1 The Graal collaboration results and prospects Presented by Carlo Schaerf Università di Roma “Tor Vergata” and.
Use of the Moon as a calibration reference for NPP VIIRS Frederick S. Patt, Robert E. Eplee, Robert A. Barnes, Gerhard Meister(*) and James J. Butler NASA.
Chem. 133 – 2/16 Lecture. Announcements Lab today –Will cover last 4 set 2 labs + start on set 2 labs –Lab Report on electronics labs – due 2/23 (I planned.
Chem. 133 – 2/18 Lecture. Announcements Homework Set 1.2 (bold problems) – due today Quiz 2 Today Electronics Lab Reports – due Tuesday Seminar this Friday.
So what about mass? 1. What happens to time from the frame of reference of a stationary observer on Earth as objects approach c? 2. What notation is given.
Soichiro Isoyama Collaborators : Norichika Sago, Ryuichi Fujita, and Takahiro Tanaka The gravitational wave from an EMRI binary Influence of the beyond.
Black Hole. Special Relativity Einstein’s special theory of relativity has two parts. –All objects moving at constant velocity have the same laws of physics.
Electronics Lecture 5 By Dr. Mona Elneklawi.
Belle-II VXD radiation monitoring and beam abort with sCVD diamond sensors Lorenzo Vitale, Belle-II SVD collaboration INFN and Univ. Trieste, ITALY Requirements.
The Search for Gravitational Waves with Advanced LIGO
Onboard Instruments of ASTROSAT
Really Basic Optics Instrument Sample Sample Prep Instrument Out put
GENERAL RELATIVITY General relativity describes the effect of gravitational fields on space and time.
Chem. 133 – 2/16 Lecture.
Exam 3 average: 65%. You will have all of class time on Thursday to do the group review. The response “Exams” will be on Learning Suite by Wed noon. They.
Radiation in the Atmosphere
GENERAL RELATIVITY General relativity describes the effect of gravitational fields on space and time.
Precision cosmology, status and perspectives
Presentation transcript:

1 GRS Measurement By A. Cacciani Frascati, March 21th 2006

2 Introduction GRS … one of the three classical tests of General Relativity … so far it has been tested only to the first order in m/r, THAT IS, no test for the Einstein field eqn

3 Theoretical background for gravity In general where with α, β, γ constants. Einstein puts them all = 1.

4 GRS depends only on gtt. A large mass is needed to increase the expected signal Also, it should be at rest or perfectly known relative velocity: The Sun is the only choise. To the first order, for the Sun: Δν/ν is 633 m/s Doppler equivalent, that is the speed of light. The second order adds another term smaller, that is, a signal of about 1 mm/s Doppler equivalent. Theoretical background for gravity

5 Competing instruments Masers, radio,.. They have enough stability ( claimed ) But they need to be launched in orbits around the Sun

6 Competing instruments Our instrument: the MOF It is already proven to the level of It does not need to be launched around the Sun, We are looking at the SOLAR SPECTRUM Previous measurements (not MOF) of the Solar GRS did not go better than few % (LoPresto et al )

7 MISURA DEL GRS SOLARE by: Alessandro Cacciani Runa Briguglio University of Rome LA SAPIENZA, Italy Fabrizio Massa INFN sez. Di Roma Paolo Rapex External collaborator James LoPresto Edinboro University of Pennsylvania, USA

8 A sensitive test of Fundamental Physics, especially General Relativity Previous results: Pound & al. 1960: Effetto Mossbauer Vessot & al. 1980: Maser Lo Presto 1991: GRS Snider 1971: GRS

9 How to improve? Instrumental progress such as MOF Technology Two narrow bands trasmission filter: FWHM= 50 mA, tuned on a Solar Line Intrinsic stability High efficiency (30%) Photon-shot noise limited Image detector

10 In order to reach this sensitivity, a comparison between the solar MOF signals from two satellites, one near the Earth and the other close to the Sun, will cancel all the unwanted effects, but the GRS alone. The second order signal is in the range of a mm/s (Doppler equivalent), well within the capability of our MOF. Real test of General Relativity requires time dilation effect at a second order times the first order effect. On the sun we expect a second order effect of x 636 m/s 1mm/s

11 Typical Doppler image with MOF

12 Doppler signal on the solar equator

13 Preliminary Results

14 Human ResourceActivity A.Cacciani (70%) 1 ) General Supervisor 2) External contacts 3) Cell fabrication a) Lab set up b) Fabrication c) Test 4) Observations F. Massa (70%) 5) Data Acquisition Software Developm. a) Design b) Test 6) Observations R. Briguglio (70%) 7 ) Instrument set up, test and maintenance 8) Observations P. Rapex (50%) 9 ) Data reduction Software a) Analysis b) Test and implementations c) Final results production 10) Electronic design support a) Cell heaters b) CCD synchronization