Presentation is loading. Please wait.

Presentation is loading. Please wait.

Beyond standard model.. 1. Gravity 2. Dark matter 3. Dark energy 4. Matter-Antimatter asymmetry problem. 5. Magnetic Monopole.

Published byRaymond Houston Modified over 8 years ago

Similar presentations

Presentation on theme: "Beyond standard model.. 1. Gravity 2. Dark matter 3. Dark energy 4. Matter-Antimatter asymmetry problem. 5. Magnetic Monopole."— Presentation transcript:

1 Beyond standard model.

2

3 1. Gravity 2. Dark matter 3. Dark energy 4. Matter-Antimatter asymmetry problem. 5. Magnetic Monopole.

4

5  DM interacts only gravitational effect.  Also, DM be able to interact weak force.  DM doesn’t interact that EM, Strong force with matter.  We can’t see DM via light.

6

7 Dark matter halo Halo Galaxy

8

9

10  DM is very mystery objects.  But DM is interesting subjects.  We have many problems to solve out.  We don’t know anything about that, yet...

11 But!!!!! We will find a answer. always we did… Thank you.

Download ppt "Beyond standard model.. 1. Gravity 2. Dark matter 3. Dark energy 4. Matter-Antimatter asymmetry problem. 5. Magnetic Monopole."

Similar presentations

What is dark matter?. 96% of the universe is missing In fact, all of the stuff we can detect in the universe: –All of the matter –All of the energy –Only.

What is dark matter?. 96% of the universe is missing In fact, all of the stuff we can detect in the universe: –All of the matter –All of the energy –Only.
Week 10 Dark Matter Reading: Dark Matter: 16.1, 16.5d (4 pages)

Week 10 Dark Matter Reading: Dark Matter: 16.1, 16.5d (4 pages)
Dark Matter Mike Brotherton Professor of Astronomy, University of Wyoming Author of Star Dragon and Spider Star.

Dark Matter Mike Brotherton Professor of Astronomy, University of Wyoming Author of Star Dragon and Spider Star.
GRAVITY Chapter 3 Section 2.

GRAVITY Chapter 3 Section 2.
Now I am become Death, the destroyer of worlds. Robert Oppenheimer after the first test of the atomic bomb.

"Now I am become Death, the destroyer of worlds." Robert Oppenheimer after the first test of the atomic bomb.
Major Epochs in the Early Universe t3x10 5 years: Universe matter dominated Why? Let R be the scale length.

Major Epochs in the Early Universe t3x10 5 years: Universe matter dominated Why? Let R be the scale length.
Dark Matter, Dark Energy, and the Fate of the Universe.

Dark Matter, Dark Energy, and the Fate of the Universe.
Q44.1 The strong nuclear force has a short range compared to the electromagnetic force. Why is this? 1. the particles that mediate the strong force are.

Q44.1 The strong nuclear force has a short range compared to the electromagnetic force. Why is this? 1. the particles that mediate the strong force are.
The Four Forces of Nature A Brief Introduction. The forces of nature are responsible for providing the energy we used everyday! Recall…Energy comes from.

The Four Forces of Nature A Brief Introduction. The forces of nature are responsible for providing the energy we used everyday! Recall…Energy comes from.
The Uncertain Nature of Gravity An Illustration of Science as a Process of Investigating Nature.

The Uncertain Nature of Gravity An Illustration of Science as a Process of Investigating Nature.
Chapter 23: Our Galaxy Our location in the galaxy Structure of the galaxy Dark matter Spiral arm formation Our own supermassive black hole.

Chapter 23: Our Galaxy Our location in the galaxy Structure of the galaxy Dark matter Spiral arm formation Our own supermassive black hole.
Physics: Concepts and Connections, 4 th ed., Art Hobson Chapter 11 – General Relativity.

Physics: Concepts and Connections, 4 th ed., Art Hobson Chapter 11 – General Relativity.
Class 23 : The mass of galaxies and the need for dark matter How do you measure the mass of a galaxy? What is “dark matter” and why do we need it?

Class 23 : The mass of galaxies and the need for dark matter How do you measure the mass of a galaxy? What is “dark matter” and why do we need it?
ASTR100 (Spring 2008) Introduction to Astronomy The Case for Dark Matter Prof. D.C. Richardson Sections 0101-0106.

ASTR100 (Spring 2008) Introduction to Astronomy The Case for Dark Matter Prof. D.C. Richardson Sections
Copyright © 2010 Pearson Education, Inc. Dark Matter and Dark Energy.

Copyright © 2010 Pearson Education, Inc. Dark Matter and Dark Energy.
Dark Matter Masses of Galaxies Gravity and Light Black Holes What is Dark Matter?

Dark Matter Masses of Galaxies Gravity and Light Black Holes What is Dark Matter?
Forces Force – any push or pull acting on an object

Forces Force – any push or pull acting on an object
A generic test for Modified Gravity Models* Emre Onur Kahya University of Florida * astro-ph/0705.0153.

A generic test for Modified Gravity Models* Emre Onur Kahya University of Florida * astro-ph/
Particle Physics J4 Leptons and the standard model.

Particle Physics J4 Leptons and the standard model.
Components of the Milky Way The light from galaxies is centrally concentrated. But is the mass also centrally concentrated? Does Mass follow Light in Galaxies?

Components of the Milky Way The light from galaxies is centrally concentrated. But is the mass also centrally concentrated? Does Mass follow Light in Galaxies?

Similar presentations

Ads by Google