Sunday, December 28, 2008


Hey everyone!
I'm posting from my phone, so it's not going to be very elaborate. I just want to mention a few things.
1. I'm really mad that so many of my cedar books are outdated! Since I'm in NUSH, I don't need them. But this means wasted time and money getting them. Well, I just hope that my sister enjoys herself there.
2. I'm back from Hong Kong! I had something to do on all six days! Reached there at twelve noon, dumped our stuff at Hollywood Hotel, and left for Disneyland. Only came back at ten something after the fireworks. Day two, check out and spend the rest of the day at Disneyland. Check in at Harbour Plaza Metropolis Hotel and fall asleep. Day three, half day tour and then shopping! No, Hong Kong stuff is not cheaper than Singapore! Day four, cable car ride to Lantau Island. Day five, Ocean park! Trust me, it's much, much better than Disneyland. It's so much more fun. I went on the Abyss. wow. and all the roller coasters. Finally, day six, space museum and then it's back to Singapore! Like I said, something to do everyday.
3. Oh man class allocation is out on eportfolio! Thank goodness, i'm in 306 with Gloria! whoo! I'm really looking forward to meeting my classmates and getting to know them better.
4. I'm really afraid that my cousins and I are not prepared for the performance on the 31st. argh!
5. I really love my new textbooks! But why does the bio seem the same?
6. Yes, I am still thinking about physics problems.

Yeap, I think that's all for now.
Merry Christmas and Happy New Year!



JAYASHRI(:




Sunday, December 14, 2008


I just want to talk about a few things.
1. W960!
2. A possible answer to the black hole question.


1. W960!

It's been 3 weeks since I got the phone, and therefore have had enough time to get used to it.
It's basically a business phone with a touch screen, no D-pad, a little laggy, but great overall.
Here's a picture:


Well, it has WLAN, which is a definite PLUS+. The touchscreen also allows me to get to places without much navigation. The walkman player is PRETTY(:


Well, basically I love it. My sister got W760 [chris' phone, yup!]. It's really nice too. It doesn't have WLAN, yea, but it does have a motion sensor! It's a very user-friendly phone. Mine really take some getting used to, but once you do, it does whatever you want. It's just that you can't drop it, unlike my G502, which will probably be the hardiest and best [overall] phone I will ever use in my life. It has all that you need on a phone on an everyday basis. You can drop it with no worries. It's just that mine had a software problem that couldn't be fixed, and the SE people couldn't do anything and wouldn't replace the set. Well, I was promised a new phone so I got W960.
If I had a choice, I would choose Nokia 6120 over W960, but it wasn't available. Well, now it's my job to pester my dad to get that!



2. A possible answer to the black hole question.

I had a 2 hour long conversation with Sharne about this the other day. I definitely learnt something.

Here is an illustration to show how density and mass make a difference in warping space. I do not know how the density is represented in equations [I did not study Einstein's equations], but here it is in image. This is what Einstein said.
If you have two drums, one being pierced by a needle and one being pressed with a ball, both with a force of 10N, you can see that the needle will make a bigger warp than the ball. So a more dense sphere will warp space more than a less dense ball.



Today, Gloria sent me a message telling me that she found something in the physics textbook [I have no idea how I missed this!].




There big sphere is the Sun, with its current size. It exhibits gravity X on object Y at distance Z from its CENTRE. But if the Sun shrunk to the size of the smaller sphere, the gravity between object Y at distance Z from the sphere's centre is still X! But when the object comes within the area that the large Sun once occupied, the warp on space is much more significant and this is the tremendous gravity of the black hole. The escape velocity increases as you get nearer and nearer to the sphere, until finally, it exceeds light speed. That's the event horizon of the black hole, beyond which NOTHING can escape. That's the dark part of the black hole, which is essentially, black.

Newton's F = Gmm/r^2 was an approximate equation, suitable for relatively low-gravity situations. But when it comes to strong gravitational fields, such as a black hole, relativity equations do much better. So although Newton's equation does not include density, perhaps that's why I got so confused. Einstein's equations are too confusing for me to analyse at this point.

So basically, it's just that density does play a part when you are within the area that the big star once occupied before its collapse into a black hole, that's when you feel its immense strength. But beyond that, it feels like it would have if it had never collapsed. Still, it's not possible not get crushed when you're so close to the star! Even if you were standing just outside the area that was once occupied by the star, it's still extremely strong because it's as though you're standing 1cm away from the star!



Well, I hope I gave you something to think about.
Merry Christmas and Happy New Year!



JAYASHRI(:




Thursday, December 4, 2008


Hello. Just a thing before I continue:


[Why do people say 'netball practice makes me black'? I mean, come on.

1. It doesn't make you black. It makes you darker. There's definitely a difference.

2. Doesn't this statement sound a bit derogatory?
- I actually typed quite a bit about this, but I've deleted it. -

You might say I'm reading too much into this statement, but I do not think you should say this at all, no matter what your intentions.]



Okay, I've gotten that out of my system, so now I can continue. I just want to ask a few questions. If you know the answer, let me know.



1. Is the probability of finding an electron in the nucleus 0 or 100%? Well, look at this graph:


[src: http://www.intute.ac.uk/sciences/reference/plambeck/chem1/p01233.htm]


You see that in an s orbital, the electron density decreases all the way from the nucleus [1s has no nodes]. But then look at the second graph. When you take into account the spherical volume at the nucleus [0], combining the volume with electron density, you get a different graph. This is radial probability, where there is a clear peak at 53pm [incidentally the most probable radii in Bohr theory! Bohr orbits were at these most probable radii, so n=1 was at 53pm]. Okay.

So then we are constantly using radial probability, I assume, since we've learned the prob at the nucleus is 0. But then how can the prob in an orbital be 95-99%? That really doesn't make sense. The probability in an s orbital is 95-99%, but judging from this radial prob graph, that really doesn't seem likely at all.

I really think I'm getting this all wrong! Correct me if you can.



2. Black holes! I posted a question on Yahoo!Answers regarding this.

Gravity, gravitons, the sun & black holes: density-based or mass-based?

Hey'all. A 14 year-old asking a question about gravity here, so I'm sorry if it sounds dumb.

Is gravity based on the mass of an object, or the density of an object?
The equations of gravity don't seem to say anything about density,
F = Gm1m2/r^2, unless I've got it wrong.

But then again, let's look at the sun. Currently, it has mass x, but it's not a black hole. But if it was crushed to a sphere of radius 3km [if I've got it right], it would be a black hole. And there's something about Schwarzschild radii. What's that?

Here's my question. Firstly, does this make this black-hole sun's gravity stronger than the sun we have now? I've checked this up on google, and some sources say yes, the black hole would be stronger [at the same distance y from the surface of both], while some say that no, at the same distance, the gravity is still the same. But I doubt the latter, because then how would only it be strong enough to bend light like that, in comparison to our normal sun?

Assuming that yes, the black hole is stronger, then does gravity depend on the mass, or the density of an object? I mean, using the example I have given above, it doesn't make sense that gravity is entirely mass-independent. But if that is true, then how does density fit into the Gm1m2/r^2... equation?

Also, another question.
How do gravitons fit into the picture of relativity described by General Relativity? Curves in spacetime vs force particles? ?!!


I'm really sorry if I've got this all wrong. This is NOT what I'm learning in school. I'm just a physics lover who likes to read about these things on my spare time, so it's quite likely I'm not getting the big picture, and most of my thoughts and assumptions are wrong. Unlike many people who ask questions on Y!A, I HAVE done my research, but cannot find comprehensive answers. So please help me out! Thank you. (:


Best Answer - Chosen by Asker

"Is gravity based on the mass of an object, or the density of an object?"

in a sense both. you wrote the right equation for the Force due to gravity.
M1 is the mass of the object "creating" the gravity (earth), and m2 is the object "seeing" the gravity (you).

the density comes in in the sense that the minimum value of r for the earth+you case is the radius of the earth, and M1 is the density of the earth time (4/pi)r^3 (the volume of the earth).

but in the most common & general case, it's *masses* that count, not densities.

the Schwarzschild radius is a characteristic parameter of every object w/ mass. It is the radius for a given mass where, if that mass could be compressed to fit within that radius, no known force or degeneracy pressure could stop it from continuing to collapse into a black hole.

An object smaller than its Schwarzschild radius is called a black hole. The surface at the Schwarzschild radius acts as an event horizon in a non-rotating body.

"does this make this black-hole sun's gravity stronger than the sun we have now?"

at the "surface" of the new sun, yes.
if r was the same distance from the center of the sun as it was before, then no.
this is effectively a result of the equivalent of Gauss's law for gravity.

"How do gravitons fit into the picture of relativity described by General Relativity?"

all forces can be described equivalently either via the interaction of body 2 with the "field" defined by body 1, or via the exchange of the "carrier" of the force between the two bodies.

for example, the electrical acceleration of particle 2 can be calculated as the force on particle 2 due to the electric field defined by particle 1 *or* viewed as the exchange of the carrier of the electromagnetic field, the photon.

same with gravity. interactions can be viewed as particles interacting with fields, or particles interacting with particles by exchanging force carriers. this is equivalence is "quantum field theory".

the carrier of the gravitational force is the "graviton". it has yet to be experimentally measured like the other force carriers. the other force carriers are the pion or gluon for the strong force, the W and Z bosons for the weak force, and as i mentioned, the photon for the electromagnetic force.

cheers


Okay, so basically the surface gravity is stronger, but the gravity at a distance is the same. But if that is the case, how does light get pulled in to a black hole? Light isn't touching the surface when it gets pulled in, right? So how does it work?



3. Which brings me to my third question. What is escape velocity? When they say earth's escape velocity is 11.2km/s [that's fast!], is it an initial thrust such that the intial velocity [of course after the initial acceleration] 11.2, and then it's sufficiently slowed down by earth's gravity but even after that, 11.2 is the minimum to make it away from earth? Is it that, or is it that the speed must constantly be 11.2km/s? I think I've gotten a wrong idea about escape velocity.



So help me out here! Thanks. I know you're probably wondering why I'm thinking about all this in the holidays, but I'm sure you know me. A healthy dose of physics keeps me happy ;)


I really wish I had the year 3 syllabus. I don't want to just waste my holidays without studying or preparing myself. :/



So, happy holidays! Enjoy them!



JAYASHRI(:




Wednesday, December 3, 2008


Hi! I know it's been a long time since I last posted.

Well, I was kinda thinking about year 3 and how I probably will NOT be able to get a 4.5. My aim is just to keep it at 4.00, an average of B+, and I think even that will be hard.
And right now, I'm pretty sure I won't get into the principal's list. I mean, the top 5%! That's only 8 people! Yes, I did score 4.5s, but QUITE A FEW PEOPLE SCORED 4.5. At first I was disappointed, but now I've learnt to appreciate that I even got >4.5.
I will NOT say 'Thank you God!' because I'm starting to doubt the existence of god, and therefore I will not thank something I believe does not exist.

Anyway, get a load of this. I found it pretty funny. I hacked my mum's email account.
From Jean-Marc:

Dear Parents of Jayashri,
Allow me to introduce myself. I am Jean-Marc, the French Language Teacher at NUS High School. I am writing to you this little note because I don't know as yet if I'll be able to meet you on Parent-Teacher-Meetings day, i.e. next Monday 24 November '08. This is due to the fact that I have to go for surgery.
I would have liked to talk to you to praise your daughter Jayashri. I am a very demanding teacher, yet, she has performed very far beyond my expectations. She finished with a distinction (A+) and is the top student in class. I am really more than pleased with her progress. Jayashri is very talented, very hard-working, serious about her learning and eager to learn yet funny and easy-going. Jayashri is also quite outspoken and is not afraid of making mistakes. She always ask very pertinent questions. Jayashri is also very attentive. She has a great and positive attitude. I hope you will encourage her to continue her study of the French language. She definitely is a great role model for the class. If only all the students could be like your daughter! I also hope my own daughters become like yours...
Having said that, it would really be a pity and it would sadden me a lot if Jayashri was not going to continue to the next level as she truly is a role model for the rest of the class. Jayashri is quite lively, fun, jovial and bubbly and makes the class interesting. Of course, I know this is not a core module, and simply an elective one. However, I am sure you will agree with me that if she can speak French one day, it will definitely open doors for her.
Should you wish to contact me regarding the progress of your daughter or for any other reasons whatsoever, you can rest assured that I am at your entire disposal and you can contact me at my DID phone line number, which is: XXXXXXXX or on my hand phone at: XXXXXXXX.
I look forward to meeting you sometime in the future. At the same, I would like to take this opportunity to wish you a Happy Festive Season, a Merry Christmas and a Happy New Year.
Yours sincerely,
Jean-Marc Vilaire

I mean, LOL! I really didn't see that coming. What's with the funny progress report remarks too... which I will post when I overcome my laziness to go get my report card.

LOLOLOLOL!
But surgery? I hope he's alright :/

Anyway, have a GREAT Christmas [though once again I do not understand its significance] and Happy New Year! & Start studying cos we won't have much time during the term.

Cheers,
Jayashri



JAYASHRI(:

GROUND RULE:
LOVE YOUR PHYSICS TEXTBOOK!

[Paul Hewitt, Conceptual Physics 10th Ed. Pearson International Edition.]


I like this picture. I really do.




  • November 2008
  • December 2008